Wednesday, March 17, 2010

Space














"The surface of the Earth is the shore of the cosmic ocean. On this shore we've learned most of what we know. Recently, we've waded a little way out, maybe ankle-deep, and the water seems inviting. Some part of our being knows this is where we came from."
– Carl Sagan


For thousands of years, humans have wondered about the void beyond the blue sky, about the glowing orbs of light that inhabit it and about the darkness that blankets it all on a regular basis. Where did it come from? How was it created? What, exactly is it? In attempts to explain it all, different cultures at different times have used folklore, legend and religion.

During the last few centuries, scientific explanations have gained steam. Some of the world's greatest minds have created and applied the laws of physics and geometry to interpret the size, shape and age of the universe. And although they have, over time, gotten a better sense of the dimensions and characteristics of planet Earth and some of its neighbouring planets, moons and stars, the universe beyond remains mostly a mystery.

Only recently has technology progressed to the point where humans have been able to venture beyond our planet's atmosphere - first only visually with telescopes, then with the help of rockets. And although the advances in technology have come fast and furious over the last few centuries, the universe remains largely unknown.






Space pictures

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Humans in Space










Not everyone got caught up in the Mars methane maelstrom though! We have a bunch of great posts about the past, present and future of humans in space and the (awesome) technology that we might use.

OrbitalHub has an interesting article about the historic Soyuz 4/5 mission, which successfully carried out the first docking and crew transfer between two spacecraft 40 years ago.

Collectspace has the answer to the age-old question: “What do the first American to command five space missions, the first commander of the ISS and the first satellite repairman have in common?”

Over at the awesomely named Potentia Tenebras Repellendi, Alexander DeClama will tell you all about the very cool Chariot lunar rover which made an appearance in the inaugural parade. It can drive sideways!

lunarroverSpeaking of the Obama administration, Bruce Cordell at 21st Century Waves outlines ten space trends for 2009 and speculates about how the current issues facing the administration will influence the near-future of the space program.

Sometime in the slightly-less-near future, we will be back on the moon, so before you buy your one-way ticket to the moon base, you will want to take a look at Out of the Cradle and Ken Murphy’s review of a new book about the challenges of establishing a lunar outpost. (Hint: Driving the Chariot rover is the easy part)

Given the new administration’s commitment to energy independence and sustainability, the sun may be shining on Space-Based Solar Power. Alex and Ralph at The Discovery Enterprise have a posted their very interesting debate about whether Space-Based Solar Power is really feasible.

Solar power may also be crucial for our return to the moon, but the long lunar night makes it somewhat problematic. To hear about some ideas to work around this problem, check out the summary of a 1989 paper on “Solar Power for the Lunar Night” at Altair VI.

The problem with all these ambitious plans in space is that it’s really hard, and therefore rather pricey, to launch things into orbit (and beyond). That’s why I was happy to read over at Next Big Future that a Cambridge University team is making progress on creating carbon nanotube ribbons, a vital component of that coolest-of-cool ideas, the space elevator.

marsterraformed600kn0Once we have unlimited, cheap access to space, and clean, endless power from space-based solar arrays and are cruising around on the surface of the moon, will we be satisfied? Heck no! We’re going to Mars! And when we get there, we’re going to terraform it! It’s easy! Ethan Siegel over at Starts With a Bang concludes that there are only three things that we would really need to do.

And then, once we have settled Mars and are getting really cocky, we’ll want to start looking for other planets outside our solar system. And after all the work of terraforming, we’ll probably want to just skip that step and look for habitable planets. Luckily, Paul Gilster at Centauri Dreams reports that vegetation on distant planets is detectable!

Sony Vaio W-Series vs Lenovo S12 vs Asus 1101HA vs Samsung NC20














Two of these netbooks have 12.1 inch displays that almost make them notebooks rather than netbooks, one has an 11.6 inch screen and the 4th has a teeny tiny 10.1 inch panel but all pack a larger than average resolution to make the best use of their screen real estate.

A higher screen resolution can make a big difference when working on documents and wanting to open more windows to view them side by side. Most netbooks have the standard 1024 x 600 resolution but there are a breed of usually larger (but not always) sized netbooks that offer a bit more.

We have lined up 4 of the best and most recently released netbooks that all give us what we want in the screen resolution department but do they measure up elsewhere? Check out the comparison below to find out.

Compare the specifications of these netbooks, compare prices and also head over to our netbook rankings to see where each places and if they are worth your money.

Nokia 2710 to take over the low-end Navigation market

2710_nav_front

The 2.2″ screen does seem a tad bit small for navigation , however the S40 interface is well adapted for small screens. You get the usual feature set including bluetooth 2.1 , FM Radio and a 1020 mAh battery goor for about 6 hours of non-stop navigation.

2710_nav_cradle

Included with the device is a car holder and all relevant maps are preloaded onto the device. In select regions the device will also be bundled with Nokia Life-Tools which shows that the 2710 is intended for rural areas or atleast those areas where proper internet connectivity can be a hurdle. Priced at approximately 110 euros , the device could be a sleeper hit for Nokia.

Endeavour STS-130 Mission Scheduled For Feb 7, 2010

It's that time again - The Kennedy Space Center in Florida will be buzzing this week as Space shuttle Endeavour's STS-130 mission is scheduled to begin within the next few days. The shuttle is set to depart from Launch Pad 39A, and the packing of astronauts' spacesuits into Endeavour started already on Monday.

The mission will consist of six members - with the STS-130 crew flying to the international Space Station. The crew has also already entered into quarantine on Sunday in preparation for the launch.


The six crew members will consist of George D. Zamka (Commander), Terry W. Virts Jr. (Pilot), Nicholas J. M. Patrick (Mission Specialist), Robert L. Behnken (Mission Specialist), Stephen K. Robinson (Mission Specialist), and Kathryn P. Hire (Mission Specialist)


This mission will feature 3 spacewalks, and deliver a third connecting module - called the 'Tranquility node', as well as a seven-windowed cupola, which will be used as a control room for robotics. The mission is scheduled to last 13 days.



Image above: (From left) Mission Specialist Nicholas Patrick, Pilot Terry Virts, Mission Specialists Robert Behnken and Kathryn Hire, Commander George Zamka and Mission Specialist Stephen Robinson.
Image credit: NASA


Endeavour is scheduled to launch on February 7, 2010 at 4:39:47 a.m. EST

BIC Mobile Phone




















Europe : The BIC phone is to be launched in Spain by Orange after its success in France. The BIC phone is pictured above and is an off the shelf ready to use mobile phone. It’s purchased with a fully charged battery, the SIM card in place and the battery is rechargeable.

Focusing on ease of purchase and also ease of use, the BIC phone can be bought at supermarkets, petrol stations and airports etc. Want a basic phone – then this one has all the basic functions for calls and texting.

The Spanish BIC phone has the same features as the French version and is on sale at the RRP of 29 Euros. It comes with 20 minutes of calls which have to be used within 60 days of the BIC phone being activated.

In France, over 110,000 BIC phones were sold since August 2008. A survey conducted by LH2 which involved 600 respondents clearly showed that the BIC phone was a “must-have” phone for people who were looking for ease of use and simplicity.

Lenovo IdeaPad S10e vs S10-2 vs S10-3 vs S10-3t















The Lenovo IdeaPad 10 inch comparison – we’re comparing Lenovo’s IdeaPad range of 10 inch netbooks including the previous S10e model, the current S10-2 netbook and the about to be released S10-3 netbook and its sibling, the S10-3T tablet, which is very similar in specification but with a multitouch screen turning it into a tablet.

The S10e was a popular netbook and, whilst the S10-2 has not fared so well with reviewers, currently propping up our overall netbook rankings table, we are expecting bigger and brighter things from the new models – the S10-3 and S10-3T netbook multitouch tablet.

These brand new netbooks have similar specs and are suitably equipped with Intel’s pine-trail Atom processor and Windows 7. The big difference is in the screen, the S10-3T has a multitouch screen turning the netbook into a tablet. The S10-3 also seems a solid netbook with a decent review from Laptopmag so far.

The Lenovo S10e and S10-2 netbooks can be found in our netbook rankings and the other models will join in shortly once enough reviews are released for the new models.

Let’s get on with the comparison, how do these great Lenovo netbooks compare?

Ovi Maps 3.0 Graduates From Beta











Formally known as Nokia Maps, Ovi Maps 3.0 has graduated from Nokia Beta Labs and is now officially available to download, for any compatible handset, from Nokia.com/maps. Nokia maps originally began pretty simple, with other applications offering a better experience without the need of a PC. Ovi Maps still requires you to have a PC in order to load maps (Mac support coming soon). However you can head over here where Ricky Cadden of Symbian Guru has managed to locate the relevant .sis files in order to allow all Mac and Linux users to install the apllication too.

The final version includes support for S60 5th edition devices, traffic data for more countries, weather updates, an enhanced and tweaked interface and general bug fixes. Rafe Blanford of AAS has written a detailed review of Ovi Maps 3.0 and I advise you check it out.

Here’s the full list of compatible devices:

* S60 3rd Edition Feature Pack 1 (E63, E66, E71, E90 Communicator, N81, N81 8GB, N82, N95, and N95 8GB)
* S60 3rd Edition Feature Pack 2 (E55, E75, N78, N79, N85, N86 8MP, N96, 5320 XpressMusic, 5630 XpressMusic, 5730 XpressMusic, 6210 Navigator, 6220 Classic, 6650, 6710 Navigator, and 6720 Classic)
* S60 5th Edition (5800 XpressMusic and N97)

Don’t forget to leave some comments on what you think of the new Ovi Maps solution. If you are reluctant to purchase the licence, Nokia is offering a free 7-day trial here. So hop on over and navigate your way through a new and improved 3D world.

HP 2140 Mini vs HP 2133 Mini Comparison









HP consistently make solid and well built netbooks, we compare the main features of their first, the HP 2133 Mini-Note with the latest, the HP 2140 Mini.

The HP 2133 Mini-Note was one of the first netbooks by one of the big laptop manufacturers and sold well with perhaps the best keyboard and very good screen.

The latest model, the HP 2140 brings the netbook specification up to date but how does it compare with its older sibling?

So if you are in the market for a HP netbook then this comparison table should help you decide which one is best for you.


« Dell Inspiron Mini 9 vs Inspiron Mini 10 vs Inspiron Mini 12 comparison Asus Eee PC 901 Specification » Asus Eee PC 901 vs 1000H vs 1000HE Asu


















The good value Asus Eee PC comparison, this time between the Asus Eee PC 901, the Asus Eee PC 1000H and the Asus Eee PC 1000HE, all of which have fantastic battery life.

All of these Asus netbooks have a good specification including Draft N, 3 USB ports and practically all day use with the 901 featuring an SSD hard disk instead of the conventional hard disks in the 1000H and 1000HE netbooks.

The 901 is more portable, as it is lighter and slightly smaller but still manages to pack a lot in. It is also the cheapest of the 3 at only around £240. But then you don’t have to pay much more for the 1000H, which is available for just less than £260. The 1000HE is the real workhorse of the 3 will the longest battery life and a slightly faster processor but is also the most expensive.

In our view all of these 3 Eee PC’s offer great value for money. But what then are the differences that are important to you with regards to these 3 Asus netbooks and which should you think about buying? Have a look at the comparison table below.

ElectroSelf™ - The Revolutionary Power Source That...Powers Itself?












Backup generators are noisy and add pollutants to our air. They are also expensive and not very dependable when looking at long stretches of power outages. No wonder why some people think twice about spending $500 and upward to have a piece of equipment that collects dust most of the time.

A new company in Italy called Electro Power Systems SpA has been designing a useful alternative back up power that is clean and reliable since their inception in 2005. Last year, this unit called the ElectroSelf™ began receiving the praise that it deserved.

ElectroSelf™ is a self-contained and self-recharging fuel-cell system that runs solely on water. There are no batteries, no diesel fumes or any other type of expensive and inconvenient factors to contend with. ElectroSelf leverages the water that is produced by the fuel cell during a power outage to generate clean H2, feeding the fuel cell during the next unscheduled power shortage.

This unit can also be incorporated with a main power source in an on grid and placed anywhere in the world. For the prospect of selling power back to utility companies in very rural country, this potential is very possible. As a self-contained unit, the ElectroSelf is capable of operating in temperatures ranging between -20 degrees C to 45 degrees C, indoors or out. Forming a business from a community co-op can also become a reality within the proper realms.

Adriano Marconetto is founder and CEO of Electro Power Systems SpA and anticipates green networks such as his company have introduced to become increasingly attractive to alternative fuels already in place. The fact that ElectroSelf is 100% self-sufficient in creating its own hydrogen opens doors for other companies to search out more flexible and totally green designs in all aspects of fuel free energy.

Not only is this new design virtually maintenance free and guaranteed to return upfront costs but is also a very real option for disaster areas, areas of extreme temperatures and isolated regions. Operating costs are minimal because of the absence of moving parts and topping off with water once per year is the only regular requirement.

ElectroSelf™ was included in the Global Cleantech 100 of 2009 and at the GSMA's Mobile Innovation EMEA event in June 2009, ElectroSelf was awarded "Most Innovative Product Enabling a Greener World". This is a fascinating use of green energy by combining Hydrogen (H2) and Oxygen (O2) to create energy; hydrogen fuel by electrolysis of demineralised wastewater of the power generation phase.

Each day, innovators from around the world are creating alternative methods to aid our planet while allowing us to hold on to the luxuries that we have become accustomed to. Hydrogen fuel by electrolysis is just the first step to bigger and better energy creativity to come.

Toshiba NB200 vs Toshiba NB300 vs Toshiba NB305













The NB200 has always been famed for its huge battery life and so has been especially popular with mobile workers and those who travel a lot. With the greater energy efficiency offered by the Intel Atom N450 processor, the Toshiba NB300 and NB305 can get even more juice out of their batteries and so battery life has gone up from an already impressive figure.

The newer models also provide Draft N wireless and bluetooth, and at a reasonable price, which means that the Toshiba NB300 and NB305 should be looked on as favourably by reviewers and the general public alike. The Toshiba NB200 is still available to purchase and it is possible to pick up a bargain with Laptops Direct offering Grade A1 models

Major update for Nokia Maps 3.0 with Ovi Maps










Firstly, Nokia Maps team would like to thank those who have provided feedback, bugs, blog entries, suggestions and surveys over the last few months - This has been extremely helpful in enhancing and “fine tuning” the product – so please keep them coming in! :-) We do review all of your suggestions and where possible we look for opportunities to build them into the product.

Now to the exciting stuff….the Nokia Maps Team is pleased to announce an updated release of Maps 3.0Beta. One of the eagerly awaited news is that this updated version now supports S60 3rd Edition Feature Pack 1 devices and N96!

In addition to this, there are also some new features/enhancements to the previous release:

  • Start-up sequence takes you to your current position as soon as position is found. If your position is not found in few seconds, you are taken to last known position
  • You can rotate the map, so you can for example view 3D landmarks from all directions. Just press 4 and 6 in map view. Pressing 5 takes you back to 'north up' view
  • In 3D view mode, you can tilt the view by pressing 2 and 8
  • 2D/3D mode works with all map modes, i.e. with Map/Satellite/Terrain
  • My Favourites menu is cleaned up and History list is moved higher in menu
  • My Places has option "Point me to" for any saved place/landmark, you the direction to that place on the map
  • In addition to the synchronisation of Favourites and Collections with Ovi maps Beta and vice versa (use in online mode, enable Internet connection), you can now plan routings on Ovi Beta and synchronise to your device
  • Finally, many bugs have now been fixed
Maps 3.0Beta works with all Nokia devices based on:
S60 3rd Edition Feature Pack 1 (E71, E66, 6110 Navigator, N95, N95 8GB, N82)
S60 3rd Edition Feature Pack 2 (N96, N85, N79, 6650, 6210 Navigator, 6220 Classic, N78)

new Nokia Ovi Maps














There is a new version of Ovi Maps application for your Nokia with a some enhanced features and services such as high resolution satellite and terrain maps – both in 2D and 3D views, 3D landmarks for over 200 cities, rotation, tilting, night view, and fly-overs and fly-throughs.

Other additions include enriched POI information, weather service that provides 24 hour and 5-day forecasts, and ability to walk from one place to another using their pedestrian navigation with routing optimized for those on foot. Oh, and traffic updates too including traffic camera locations and such.

There’s also the website “www.maps.ovi.com” which lets you find stuff online, organize them, and sync over-the-air between Ovi Maps on your compatible mobile device… Via

Acer Laptops












Unveiled in the mid of February, the new Netbook Acer Aspire One 532g has a lot of talk lately as advertised as the first netbook with Atom Pineview Processor N450 and the graphics Nvidia ION new generation. Here is a little more about the Acer Aspire One 532g including its release date and price.

This Netbook and should disembark from the end of March in Europe suggested retail price of under 500 $ with the following configuration:
Dalle 10.1”WSVGA LED Backlight (1024 × 600)
Pineview Intel Atom N450 (1.66 GHz)
RAM Installed (Max) 1 GB DDR2 667 MHz
Storage Space 320 GB (a priori) at 5400 rpm
Graphics Card Nvidia ION Gefoce new generation GT 218 512 MB dedicated DDDR3 and Intel GMA X3150.

Audio System 2 Speakers
Wi-Fi b / g / n + Ethernet
Bluetooth Yes Bluetooth 2.1 + EDR
Card Reader 4 in 1
Output (s) video HDMI (HDCP), VGA
Input (s) / Output (s) Headset, Microphone
USB 2 USB 2.0
OS 7 Windows Home Premium
Li-Ion 6 cells, 63Whr a priori
Autonomy announced 10 hours max, max 5 hours with the ION
Dimensions (mm)
Weight 1 kg

Its presence on the left side VGA, an air vent and front USB port and an HDMI output then positioned on the right are the card reader 4 in 1, audio ports, USB, a Kensington and an attached Ethernet connector. The design is very similar to the Acer Aspire One 532H with a hull and interior bright blue / black. The keyboard has keys flat matte slightly spaced from each other and the multi-touch touchpad that has a button bar is well integrated into the chassis.

As we noted in our article dedicated ION 2 versions of next generation are proposed by Nvidia. This is the first, which is intended to Netbooks from 9 to 10 inches, found embedded in the Acer Aspire One 532g. This version of the ION has 8 cores, 16 cores cons to that which can be integrated with ultraportables from 11 inches, like the Asus Eee PC 1201PN.

From the first tests of a pre-release of the Acer Aspire One 532g, it gets a score of 3049 points in 3DMark03. It would probably improve if optimized drivers come out. In all cases, the ION input range of new generation can theoretically provide greater autonomy to the ION first generation, thanks to technology Nvidia Optimus.

This is indeed capable as the tasks performed by the user to determine if the Netbook can operate solely on the graphics Intel GMA X3150 integrated processor or if it must use the power of Ion. In the first case, for example in office, the ION is not activated unlike machines equipped with the ION first generation. But the ION consuming more energy than the graphics Intel GMA autonomy should boost.

Recall that the ION delivers superior performance to the Intel GMA chips and can play a few tracks resource-efficient but also to read smoothly 1080p HD video, what can not the lack of Atom Netbooks ION or a chip Broadcom decoder. Should in all cases to expect the first tests the Acer Aspire One 532g finalized version to get a real idea of its performance and its autonomy.


Acer Aspire One 532G: Netbook with ION 2 Dedicated Graphics















The new Acer Aspire One 532G sets the netbook trend in the digital world where Hi-Def viewing online is growing dramatically. Acer presents the world’s first netbook with dedicated next-generation NVIDIA ION graphics acceleration enabling users to enjoy Hi-Def content online as well as playback at 720p; alternatively, connect through HDMI output to a secondary Hi-Def TV/LCD monitor for sharing Hi-Def content with friends at a larger 1080p resolution.


With up to 10 hours* of battery life, integrated Wi-Fi , 10.1″ Hi-Def LED backlit display and optional 3G, the Aspire One 532G matches outstanding performance with an ultra-compact design, offering all the power you need. Netbook users can now enjoy flawless Hi-Def web content streaming and multiple Internet applications with ease.


Flawless web Hi-Def acceleration and Hi-Def entertainment
Go beyond simple Internet browsing to experience full high-definition video on sites like YouTube HD, Hulu and Facebook, Aspire One 532G with dedicated graphics accelerates web Hi-Def content streaming effortlessly. Enjoy smooth and flawless 3D computing, mainstream PC gaming, boost the performance of editing and converting videos, face-tagging photos and Hi-Def video playback up to 1080p via HDMI-output to HDTV; and effectively perform everyday Internet browsing, emailing, chats, photo viewing, document editing and such on the Aspire One 532G. All of these are achieved with the new Intel Atom N450 platform and next-generation NVIDIA ION GPU with dedicated 512MB memory.


Smart power and Hi-Def performance

The Aspire One 532G makes no compromise on great performance and battery life; it mobilizes online Hi-Def computing, at the same time lowers power consumption for longer-lasting battery. NVIDIA Optimus Technology intelligently, automatically, and seamlessly transitions between the powerful NVIDIA ION GPU, and battery-saving integrated graphics – depending on the needs of the application – delivering great battery life and great performance when you need it.


Care-free mobile companion
Making light work of Internet multi-tasking, the Aspire One 532G needs only a single charge for up to 10 hours* of cable-free power, enabling users to stay connected and get the most on-the-go. The innovative AC adapter is travel friendly, lighter than typical adapters, saves 1/3 charging time and comes with interchangeable AC converters. No matter where you are, you can always have the right plug.


Measuring only 1″ thin and about 1 kg in weight, the Aspire One 532G is available in three contemporary colors – Sapphire Blue, Ruby Red and Pearl Silver. Its compact form, fluid Hi-Def cinema and flawless Hi-Def flash video quality along with great battery life, truly realizes barrier-free communication.


This highly efficient netbook is Energy Star v5.0 qualified and compliant with RoHS and WEEE EU directives, regulating the use and disposal of hazardous substances in electrical and electronic equipment. It also features LED backlight, making it mercury free.


The Aspire One 532G will start shipping at the end of Q1 2010.

The Underwater Thinking Robot - Explorer














Canada has only three years to complete a deadline which is to compile enough evidence to support its claim to a vast Northern Territory in the Arctic. It has a critical mission, to map the sea floor in this area, and at a depth of up to 5 kilometers, there is enough pressure to crush a car to scrap metal, and kill a person long before that. How can they do this without risking life and limb?

In March of this year a small team will attempt to do just that. From an ice camp just above Borden island, over 4,000 kilometers from Toronto, they plan to launch a pioneer Autonomous unmanned vehicle, named Explorer. This six meter long, yellow torpedo shaped craft will be the first of it's kind to explore a dark and mountainous world in the deep Arctic Ocean, previously unseen until now. Creeping through the depths, Explorer will travel at the same speed as a fast canoe, and tell us so much about the Ocean floor.

Staying down up to four days at a time the Explorer with be an extremely expensive trailblazer, all by itself, with no contact from the outside world if there is trouble. If there is turbulent currents, a massive sea mount, or even some curious animal, this AUV has to fend for itself. It will have to use pre-programmed wits, it will have to decide for itself what to do in case of an emergency. Then after all of that, as it comes to the surface with it's lithium-ion batteries quickly dwindling, it will also have to find it's masters floating somewhere on one of the ice platforms in the warming seas of the Arctic.

This 'little' excursion is one of the risky, but most ambitious missions that has ever left a submersible alone in such unforgiving seas. Only the most advanced electronics and navigational systems in the world could pull this off. Who might you ask is the creator of the Explorer? It is actually a firm in the small town of Port Coquitlam, in B.C. Located here is the International Submarine Engineering Ltd., a group of ten select companies who have been competing for submersible contracts around to globe, and who have over 250 of these vehicles under their belts, selling to Naval and scientific agencies in 20 countries, including Japan and the United States.

With president of the company James McFarlane, and long time submarine designer James Furguson as vice president, this company has kept up with the technologies of underwater robots for years. They have had some wins and some losses, but are determined to be the best in the business.

DeltaWing Racing Concept















It has been a while since any radical new designs have been introduced in the world of car racing. That is all about to change. The radical DeltaWingIndyCar Concept is able to deliver 235mph laps with only half of the power as well as fuel consumption. This newly introduced car answers the call for high performance not only with efficiency but with sustainability as well.

This new car's design showcases the very latest in American technology and incorporates future trends in materials, manufacturing techniques, fuels and powertrains, computer modeling and occupant safety.

In Indianapolis, Indiana, the DeltaWing LLC was proud to introduce today's future of open wheel racing at the prestigious Chicago Auto Show. This new concept was aiming to realign America's racing tradition with its new technological advances that will return auto racing to cutting edge relevance that seeks to promote extreme performance with less environmental as well as financial resources.

A summary of the key technical features of the DeltaWing auto racing car includes:

Weight with the driver equal to 1,030 lbs.
A wheel base of 125 inches
Aerodynamic drag is equal to Cd 0.24
Front track is 24 inches
Horsepower is equal to 300 BHP
Rear track is 70 inches

Explanation of Key Technical Features


The engine as well as the transmission are known as "non-stressed members" of the structural design of the chassis that will allow teams to install a wide number of lightweight power trains. The prototype of this racing car will feature a 4-cylinder engine that is turbo charged which will produce about 300 horsepower at approximately 7,000 rpm and will weigh approximately 160lbs. fully dressed.

The configuration freedoms, engine capacity, and RPM are anticipated to only be given that rate of delivery of fuel to the engine which will be controlled by a specifically made fuel flow rate control unit. The distribution of this vehicle's weight must be more rearward than has been traditionally seen with approximately 72.5% of this car's mass on its larger rear tires. About 80% of the aerodynamic downforce will act on the rear of this car.

When the DeltaWing is under acceleration the inline traction can be felt through the rear tires because it is greatly enhanced not only by rearward weight but also through aerodynamic distributions. Approximately 60% of the braking force, which is unique among the racing cars of today, is generated behind gravity's center thus giving this car a dynamically stable response. The locking propensity is greatly reduced on the corner entry of the inside front wheel.

The transmission of this racing car will feature a 6-speed oval as well as 5-speed along with reverse road track configurations. The DeltaWing will also have sequential paddle shift actuation. The restraint layout, driver position as well as energy absorbency has been designed with all of the latest data concerning survival criteria. Advanced computer modeling of impact energy management, structures, vehicle dynamics, aerodynamics, and tires have all been used to develop the virtual DeltaWing.

CNC construction techniques as well as modern advanced materials have been applied in order to achieve gains not only in lightweight structures but occupant safety as well.

Porsche 911 GT3 R Hybrid Uses Kinetic Energy in a Unique Way




Pull up any article on alternative energy by way of kinetic energy and you will see such words as "fruitcake" or "nutcase" pretty close to the inventor's name. Kinetic energy, to a lot of people, means creating energy out of nothing, which everyone knows is physically impossible.

However, when presented in a different light by the company that first developed a hybrid car 110 years ago and is known for innovative hybrid technology, it just may be time to sit up and take notice to this once crazy idea.

Williams Hybrid Power partnering with Porsche recently showed off the Porsche 911 GT3 R Hybrid that features an electrical front axle drive with two electric motors onboard that supplement the 480-bhp, 4-liter capacity located in the rear of the race car. Instead of using regular batteries that are normally found in a hybrid vehicle, an electrical flywheel generator delivers energy to the twin motors.

The flywheel's rotor that is actually an electric motor spins at 40,000 rpm storing energy mechanically as rotation energy. Whenever the brakes are applied, the two motors reverse their function and charge the flywheel. As the braking action ceases and the gas is once again engaged, there is a powerful burst of energy (up to 120kW) that is available for 6 to 8 seconds.

There is no wasted heat from burning brakes, no wasted fuel by accelerating and much lower C02 emissions. Point made, the flywheel is nothing more than a mass rotating on an axis, a form of kinetic energy. In this particular scenario, the flywheel is used to store energy, taking the place of a chemical source found in a battery.

Porsche and Williams are not as intent on winning a race with their philosophy as they are proving a principle that Porsche bases all of their vehicles on the Porsche Intelligent Performance philosophy. Using less fuel, more efficiency, lower emissions and hybrid technology has brought them to where they stand today, complete with the new flywheel energy storage system (FES).

Notable other projects that have attempted to use the kinetic energy source in recent years have been magnetic tank guns and fusion ignition systems but the hot presentation by Porsche is rekindling interest in kinetic energy as never before. An option for automobiles, economical rural electrification systems and stand-alone power units can actually look at kinetic energy as a possibility.

Maybe kinetic energy isn't such an unbelievable idea after all. With innovative companies like Williams Hybrid Power and Porsche, they are proving that anything is possible if you work hard enough at it. Look for the biggest test of the Porsche 911 GT3 R Hybrid this spring at the Nordschleife of Nurbergring, a 24-hour distance race that will bring their new technology into the arena of racing, distance, hybrid and kinetics plus absolute know-how.


Major Component Designed For Hydrogen Cars














WEST LAFAYETTE, Ind. - Researchers have completed work on a crucial component for an experimental hydrogen storage system for cars, part of efforts to reduce pollution and the use of fossil fuels in transportation.

The system uses a fine metal powder to absorb hydrogen gas under high pressure. When the powder absorbs hydrogen, it becomes a "metal hydride," and the process is called "hydriding." By then decreasing the pressure in the vessel or warming the metal hydride, the hydrogen can be released to drive a fuel cell or engine.

A complication in perfecting the technology, however, is that the hydriding process generates heat, which hinders the absorption process and prevents the hydrogen storage vessel from being filled rapidly, said Issam Mudawar, a Purdue University professor of mechanical engineering who is leading the work with research assistant professor Timothée Pourpoint and doctoral student Milan Visaria.

"If you're driving your hydrogen car, you can't wait an hour at the filling station," Mudawar said. "For this system to be practical, you have to be able to cool the hydride efficiently so that the storage vessel can be filled within five minutes with enough fuel to drive 300 miles."

The researchers have made progress in solving the problem by designing, building and testing the system's heat exchanger and circulating coolant through tubes to remove heat and speed hydrogen storage, Mudawar said.

In February, Eric Lynch, innovation strategy manager for the Purdue Research Foundation’s Office of Technology Commercialization, filed a final patent on the engineers’ behalf for the heat exchanger, a coil of stainless steel tubing that fits inside a hydrogen storage "pressure vessel" 4 inches in diameter. Standard automotive coolant is circulated through the tubing.

Such a storage technology could help make hydrogen cars a reality if other researchers are successful in developing improved alloys for hydriding and better fuel cells, which generate electricity to power an electric motor. The hydrogen also could be burned instead of gasoline in internal combustion engines.

Due to space constraints, it is essential that the heat exchanger occupy the least volume possible inside the storage vessel. Using a theoretical model they developed, the researchers determined how to precisely position the tubing so that no fins are needed to dissipate heat.

Eliminating the fins reduces the cost, weight and size of the heat exchanger, Mudawar said.

The researchers designed a system that occupies the least space possible while also properly cooling the hydride. Whereas an earlier prototype occupied 30 percent of the vessel, leaving 70 percent for the metal hydride, the new design occupies 7 percent, leaving 93 percent for the hydride.

"The idea behind this latest design is to provide the coolant as close as possible to the hydride while eliminating the need for bulky heat spreading components like fins," Mudawar said. "The main advantages of this design are simplicity and flexibility. It can easily be adapted depending on cooling and size requirements." Issam Mudawar, at left, a Purdue professor of mechanical engineering, and doctoral student Milan Visaria display their first- and second-generation heat exchangers, a crucial component of a hydrogen storage system for cars. The final design is a coil of stainless steel tubing that fits inside a hydrogen storage "pressure vessel" 4 inches in diameter. Purdue has filed a final patent on the heat exchanger. (Purdue University photo/Andrew Hancock)


The work was conducted in Purdue's Hydrogen Systems Laboratory at the university's Maurice J. Zucrow Laboratories.

Monday, March 15, 2010

Acid











Acids are compounds that ionize (or break down) to yield hydrogen ions (H+) in water. Litmus paper shows that acid is present by turning red. Solutions with pH rated at seven or lower are considered acids.

Give me an example!

Have you ever tasted lemonade that doesn't have enough sugar in it? Remember the bite that it had? That taste is a characteristic of substances that contain acid. However, most acids are highly corrosive (like the stuff inside a car battery), so tasting things to detect acid is not a good idea!

Absorb Energy












What is it?

When energy tries to go through something and is blocked, whatever does the blocking is said to absorb energy.

Give me an example!

Have you ever "burned" the bottom of your foot by stepping on a sidewalk or street on a hot sunny day? The heat that you feel is mostly energy from the sun that has been absorbed by the pavement. When heat from the sun tries to pass through the concrete or asphalt barrier, it is blocked and you can certainly tell that when you touch it with your bare skin!

Absolute Temperature











An absolute temperature scale is one that has absolute zero as its zero.

Give me an example!

The Kelvin temperature scale is an example of an absolute temperature scale. Its zero is at absolute zero, the theoretical temperature 273 Celsius degrees below the freezing point of water. Absolute zero is the temperature where all molecular motion ceases.

Abacus












An abacus is an ancient kind of calculating machine that keeps track of numbers by moving beads in grooves or along bars.

Give me an example!

The abacus was invented in ancient China - and is still in use there today! The abacus is recognized as a working part of the mathematics curriculum in many parts of China - although most younger people prefer calculators. The great thing about an abacus is you never have to worry about running out of batteries!

Amperes Law











What is it?

Ampere's Law states that when current is flowing through a circuit it produces a magnetic field of a strength directly proportional to the amount of current flowing through the circuit

Give me an example!

If you had a circuit with 30 Amperes of current flowing through it, it would produce a magnetic field of a certain magnitude (let's call it "X"). If you doubled the number of Amps to 60, you would also increase the power of the magnetic field to 2X.

Explore key information about the chemical elements through this periodic table
Group 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18
Period
1 1
H

2
He
2 3
Li
4
Be

5
B
6
C
7
N
8
O
9
F
10
Ne
3 11
Na
12
Mg

13
Al
14
Si
15
P
16
S
17
Cl
18
Ar
4 19
K
20
Ca

21
Sc
22
Ti
23
V
24
Cr
25
Mn
26
Fe
27
Co
28
Ni
29
Cu
30
Zn
31
Ga
32
Ge
33
As
34
Se
35
Br
36
Kr
5 37
Rb
38
Sr

39
Y
40
Zr
41
Nb
42
Mo
43
Tc
44
Ru
45
Rh
46
Pd
47
Ag
48
Cd
49
In
50
Sn
51
Sb
52
Te
53
I
54
Xe
6 55
Cs
56
Ba
* 71
Lu
72
Hf
73
Ta
74
W
75
Re
76
Os
77
Ir
78
Pt
79
Au
80
Hg
81
Tl
82
Pb
83
Bi
84
Po
85
At
86
Rn
7 87
Fr
88
Ra
** 103
Lr
104
Rf
105
Db
106
Sg
107
Bh
108
Hs
109
Mt
110
Ds
111
Rg
112
Cn
113
Uut
114
Uuq
115
Uup
116
Uuh
117
Uus
118
Uuo

*Lanthanoids * 57
La
58
Ce
59
Pr
60
Nd
61
Pm
62
Sm
63
Eu
64
Gd
65
Tb
66
Dy
67
Ho
68
Er
69
Tm
70
Yb

**Actinoids ** 89
Ac
90
Th
91
Pa
92
U
93
Np
94
Pu
95
Am
96
Cm
97
Bk
98
Cf
99
Es
100
Fm
101
Md
102
No



New educational posters at the WebElements shop

Atomic orbitals poster
Buy Orbitron atomic orbitals poster
Atomic orbitals poster
Buy Chinese periodic table poster
.

Element 112 named copernicium

In honour of scientist and astronomer Nicolaus Copernicus (1473-1543), the discovering team around Professor Sigurd Hofmann suggested the name copernicium with the element symbol Cn (original suggestion was Cp) for the new element 112, discovered at the GSI Helmholtzzentrum für Schwerionenforschung (Center for Heavy Ion Research) in Darmstadt. It was Copernicus who discovered that the Earth orbits the Sun, thus paving the way for our modern view of the world. Thirteen years ago, element 112 was discovered by an international team of scientists at the GSI accelerator facility. The International Union of Pure and Applied Chemistry, IUPAC, recently confirmed their discovery. IUPAC has now confirmed the new element's name as copernicium.

What is this thing we call science? Here's one definition ...













Britain's Science Council has spent the past year working out a new definition of the word 'science'. But how does it measure up to the challenge of intelligent design and creationism?

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Laboratory. Photograph: Linda Nylind

The new definition focuses on the pursuit of knowledge rather than established knowledge. Photograph: Linda Nylind

It might have been the 16th century philosopher Francis Bacon who coined the term "science", but even if it wasn't, the word must have come into common usage around his time, in the western world at least.

Perhaps with an eye on that, the Science Council has seen fit to spend a year working out a new definition of science. It may be, they claim, the first "official definition of science" ever published.

Here's what they've come up with:


"Science is the pursuit of knowledge and understanding of the natural and social world following a systematic methodology based on evidence."

Not bad for a year's work ... But why bother with a new definition? In a statement from the Council, chief exec Diana Garnham says:

"In an era where practices such as homeopathy are becoming widespread, and 'detox' is an acceptable aim for a diet, a definition creates a clear distinction between what is genuine science, and what is pseudoscience."

So there you go.

I ran the definition past a couple of experts to see what they made of it. David Edgerton, professor of the history of science and technology at Imperial College, made two points:

"It defines science as a pursuit, an activity, related to the creation of new knowledge, rather than established knowledge itself. Science is seen as a species of research. Yet a definition of science needs to define the nature of the knowledge not the means of its creation only."

and

"The definition would include historical research and indeed some journalism! It does not demarcate something called science from the humanities. This is a good and sensible thing. From the context of the press release this is not something the Science Council seem to have realised."

The philosopher AC Grayling thinks the Council has done a good job:

"Because 'science' denotes such a very wide range of activities a definition of it needs to be general; it certainly needs to cover investigation of the social as well as natural worlds; it needs the words "systematic" and "evidence"; and it needs to be simple and short. The definition succeeds in all these respects admirably, and I applaud it therefore."

The new definition has left me with two mildly nagging doubts, though. I wonder what it means for those who suggest that intelligent design or creationism are based on science? And who are the Science Council anyway?

science-faith

Overview

The fundamental belief of Scibel is that mainstream Christian faith and mainstream science are in basic harmony. Those involved in any 'official' capacity, including those involved as speakers on science-faith issues, are expected to be active Christians who adhere to historic mainstream Christian beliefs and are in sympathy with modern science as a means of knowing more about the universe God has created.

History

Scibel was initially formed as Christian Students in Science (CSIS) in 1996. It was born out of a paper researching student opinions on science and Christianity, presented at a Christians in Science (CiS) conference. CSIS received support from a wide range of Christian organizations, all recognizing the importance of talking about science and Christianity with young people. The name CSIS seemed specific to christians who were students and working in science, and this led to a name change to Scibel to broaden its appeal. Today, Scibel helps young adults to think about some of the big questions in life - whether they are Christian or not, students or not, or studying science or not. Scibel has also progressed to use modern technology to reach people, no matter which country they are in.

Mainstream in Faith

'Mainstream faith' means identifying with historic Christian belief as reflected in particular in the Nicene creed, a modern English translation of which is as follows:


We believe in one God, the Father, the Almighty, maker of heaven and earth, of all that is seen and unseen. We believe in one Lord, Jesus Christ, the only Son of God, eternally begotten of the Father, God from God, Light from Light, true God from true God, begotten, not made, one in Being with the Father. Through him all things were made. For us men and women and for our salvation he came down from heaven: by the power of the Holy Spirit he was born of the Virgin Mary, and became human. For our sake he was crucified under Pontius Pilate; he suffered, died, and was buried. On the third day he rose again in fulfillment of the Scriptures; he ascended into heaven and is seated on the right hand of the Father. He will come again in glory to judge the living and the dead, and his kingdom will have no end. We believe in the Holy Spirit, the Lord, the giver of life, who proceeds from the Father and the Son. With the Father and the Son he is worshipped and glorified. He has spoken through the Prophets. We believe in one holy universal and apostolic Church. We acknowledge one baptism for the forgiveness of sins. We look for the resurrection of the dead, and the life of the world to come.


In the 'science-faith' context, Scibel would also emphasize speaker assent to the following biblical teachings:

Creation and Redemption: The universe is a consciously purposed creation of the Triune God; all things were created through the divine Word who was God and was with God (cf eg Colossians 1.15-16, John 1.1-3). That divine Word became flesh in Jesus, who was the unique incarnation of God, and through his death and resurrection forgiveness and redemption were made available to those who receive him in repentance and faith (cf eg John 1.14, Galatians 2.15-16).

Nature: The 'laws of nature' are not independent of God but reflect his continuing upholding will (cf eg Hebrews 1.3). God can work for his purposes through natural law, no less than on those occasions in which 'supernatural' miracles reflect his sovereign decision to alter his normal pattern of working in nature for purposes of grace (cf eg his natural 'creation' of winds Amos 4.13, and compare Luke 8.24).

Scripture: All Scripture given by inspiration of God is profitable for teaching the truth (cf eg 2 Timothy 3.16). What God says in Scripture is true, and is not of ‘private interpretation’ (cf eg 2 Peter 1.20 on prophecy). Rather, the meaning of Scripture may often be clarified by an understanding of the literary conventions and cultural contexts of its human writers, as well as by the divinely given spiritual wisdom embedded in the historical traditions of the Church (cf eg James 1.3).



Mainstream in Faith

The following are relevant aspects of mainstream science:

Definition: 'Science' is "a branch of knowledge constructed on objective principles involving the systematised observation of and experiment with phenomena, especially concerned with the material and functions of the physical universe" (Concise Oxford Dictionary). Science is thus an approach and activity, but also a body of received knowledge about the world, built up empirically over past centuries.

Actuality: The body of received knowledge which constitutes natural science is found in the disciplines of chemistry, physics, physiology, astronomy, biochemistry, geology, genetics etc. as taught in general science courses in our universities.



Harmonising Two Mainstreams

Scibel believe that classically, the many devout Christians involved in the historical development of science sought harmony between theology as the interpretation of Scripture (sometimes called the "book of God's word"), and science as the interpretation of nature (sometimes called the "book of God's works"). Theology and science are both fallible human activities, and mistakes can be made. Scibel, however, stands for the view that on the whole the received teachings of traditional bible-orientated Christianity, and the well-supported conclusions of modern science (though not necessarily the interpretations put on these by some scientists) are both trustworthy, and are capable of being seen as in fundamental harmony. Scibel believes in working to change the culture so that both Christians and non-Christians can see that Christian faith and science are compatible and can work in harmony.

Astrology is Science

Yes, it’s true. Astrology is Science. This is according to the definition of Science of the proponents of Intelligent Design (aka Creationism). For if we define science as the search for truth and knowledge, then it should also include an attempt to understand the supernatural. And so as we say goodbye to the Year of the Rat and welcome the Year of the Ox, let’s make believe that (Chinese) Astrology, is in fact, science.

What’s in store for us in the Year of the Ox?

Go to the site and see how your sign fares in the Year of the Ox. As a follow-up to last year’s vanity post, here’s what’s in store for the me in the Year of the Ox:

Here’s to good health, prosperity and success in the Year of the Ox! And as they say here in Hanoi, Chuc Mung Nam Moi.

Physics in Science Fiction

Good afternoon. My name is Andrew Love (andrew.love@jhuapl.edu). In my work at Johns Hopkins University's Applied Physics Laboratory I give presentations on a variety of dry topics. This time, though, I'm talking about a subject I really enjoy: the science, and particularly the physics that can be found and played with in various science fiction stories. I was inspired to create this talk after attending the "SF and Education" panels at the 1998 Worldcon; since then I've given versions of this talk at two college campuses and also put it on the web.

Before I start, I'd like to mention my background. I have both a bachelors and a masters degree in electrical engineering, and a masters in applied physics as well, but most of the concepts I'll be discussing require only high school physics to understand and only slightly more advanced mathematics to actually calculate the answers. I have found however that thinking about these SF cases often helps me get more intuition about the physics and sometimes by understanding the physics better I get a better feel for the story too.

Normally when I give this talk I can't assume that my audience knows much about science fiction, so I say a few words about the role of science in science fiction before starting the main body of the talk - i.e. the part of the talk with equations. With a more experienced audience I can skip through those slides pretty quickly.

There is no commonly accepted definition of Science Fiction - all of the above have been proposed. I'm going to stick with the third and fourth, but the other two aren't as silly as they seem. These are taken from a book called "Turning Points: Essays on the Art of Science Fiction" edited by Damon Knight (1977). Number 1 is attributed to Norman Spinrad, number 2 is an obvious generalization of number 1 (and I'm sure I've seen it used somewhere), number 3 is attributed to Theodore Sturgeon, and number 4 is Reginald Bretnor's definition, paraphrased by Robert Heinlein. "Extrapolation" and "future" are two words also strongly associated with SF.

The sciences usually associated with Science Fiction are physics, biology and sociology (broadly understood as including economics and group psychology), but one also runs across chemistry and linguistics and more unusual choices.

Today I'll be talking about stories with structures and events that can be analyzed with current, easy physics (by easy, I mean of course, physics that I can write and solve equations about).

The themes I'm going to touch on are, first, gravity, stability and tides, which can produce some nicely counterintuitive phenomena, second, space travel and orbits, and third, some weird stuff that doesn't quite fit in any of the categories but is too interesting to leave out. If I don't get to finish all of the topics I at least hope to interest you all enough that you read further - I've printed out the slides of this talk and the last few pages give plenty of references for further reading (and sources for the ideas I will have talked about). You'll notice that many of my detailed examples come from the works of Larry Niven. This is not because he's the only author who deals with concepts from physics, but merely because many structures in his stories are relatively simple to analyze and because he's an author whose work I'm very familiar with (I participate in a list-serve discussion group about his work and am often asked questions about the physics of Ringworld, etc.)

In a couple of places I've found accidental errors in a book's physics/mathematics. Science fiction writers seem uniquely accessible by fans - I sent Mr. Niven an e-mail asking about the errors I thought I'd found, and he replied, telling me to trust my equations. Of course in one very famous case, Mr. Niven actually wrote a sequel to one of his novels to remedy an oversight in the earlier book (I'll talk about that later).

Here's a big object: The Smoke Ring. It is a torus of gas circling an old neutron star, created from the atmosphere of the planet within the Ring. Its radius is about 26,000 kilometers and it gets light from the star that both it and the neutron star circle. It holds life. By the way, there is a gas torus around Saturn which one of Saturn's satellites (Titan) orbits within (see Niven's N-Space for details on how he was inspired to create the Smoke Ring).

Being so close to the high gravity of the neutron star, things in the Smoke Ring orbit the star pretty quickly. Niven gives a minimum period of 2 hours, while I get a typical period of a little less than 2 minutes (using this equation). I don't know what causes the discrepancy, unless it's a mistake on the author's part (this is the mistake I mentioned e-mailing Mr. Niven about). The mass of Voy is implied to be 0.5 solar mass which is about 1033 grams, but to get the right answer, the actual mass of Voy would have to be much less (about 1/10000th of a solar mass), which is a pretty implausible value for the mass of a neutron star mass.

The first time I gave this talk a student asked how a planet could have survived the supernova that created Voy - it's in the book that the planet came later and also that Voy is old enough that it is not rotating anymore and therefore not sweeping a radiation beam through the Smoke Ring periodically. Good questions though.

One of the life forms common in the Ring is the Integral tree. It's pretty big - people actually live on it. Now when people are simply in the Smoke Ring they're in free fall, but what if they live on a tree? It turns out that tides give an equivalent to gravity. The gravity of the neutron star is so great that the ends of the tree should be in significantly different orbits, but instead they're constrained to orbit together. Therefore anything attached to the upper end of the tree is moving too fast for its orbit and thus feels an acceleration outward.

Meanwhile, anything attached to the lower end is moving too slowly for its orbit and is accelerated inward towards Voy. The middle of the tree remains in free fall (otherwise the whole tree would accelerate into Voy or out of the Ring) - it's in the right orbit after all. Another way to think about it is that the whole tree is being swung around Voy, which should result in a centrifugal force outward on any object on the tree, but the gravitational force of Voy cancels out the centrifugal force exactly at the center of the tree, too much on the inner tuft and not enough at the outer tuft.

The equation for the acceleration experienced by something attached to the tree is remarkably simple - it's just 3 times square of the rotation rate of the tree around Voy times the distance of the object from the center of the tree. In other words, it's just the force that would be felt if Voy didn't exist, and the tree were being rotated around its center at the rate omega, plus the differential force due to change in Voy's gravity over the length of the tree.

Unfortunately while the book reports a maximum force of about 1/5 g at the ends of a tree, I get a force of almost 30 gees - probably because of the same miscalculation that caused the error in the period of objects in the Smoke Ring. However, that problem is easily resolved - just make the tree shorter. By the way, the same tidal force that creates pseudo-gravity for objects attached to the tree makes the orientation of integral trees very stable - each end of the tree is being pulled so that it lines up with the radial vector. If the tree ever got out of that orientation, it would oscillate a bit, but then settle down due to the damping effect of air resistance. We'll talk a little more about stability later, but I should note that man-made satellites orbiting the earth sometimes use tidal stabilization to remain oriented with one axis pointing towards the earth.

I'm sure all of you are familiar with Niven's Ringworld, which he described as halfway between a normal planet and a Dyson sphere (Freeman Dyson, the mathematician who established that Feynman's and Schwinger's approaches to quantum electrodynamics were equivalent, suggested in 1959 that a technological species would eventually need all its sun's energy, and that it could get that energy by surrounding the sun with an immense number of planetoids, so that all the light from the sun was captured. Nowadays, people usually use the phrase to mean a solid sphere surrounding the sun). Ringworld is a less audacious concept than a Dyson sphere but it's still so immense a construct that most minds boggle even after quite a lengthy exposure to the idea. Basically, Ringworld is a huge ribbon circling a star; the inside of the ribbon is habitable. An example of the scale of the Ringworld is this: on Ringworld, there is an ocean large enough that a full scale map of earth is a tiny archipelago separated from other such island groups by an ocean voyage of up to a half million miles, or twice the distance from the earth to the moon.

So what's it like on Ringworld? It's a big place - the surface area is about 3 million times the Earth's. Shadow squares (see diagram) provide a day-night cycle of 30 hours, but when the sun is not shadowed, it's always directly overhead - it never rises or sets. Unlike in a Dyson sphere you can see the stars, but the biggest feature of the sky is the Arch, the other side of the Ring from where you are. Somehow, the Ringworld became inhabited by primates half a million years ago or so and now there are dozens of species of human-like but non-human creatures filling the Ring, some intelligent, some not.

In several places in the book, the tangential velocity is given as 770 miles/sec, but 740 gives the right answer for the given period of rotation and the given surface gravity, than 770 does. This difference doesn't really affect much though, except trivia contests I suppose.

What are some implications of the how the Ring is laid out? There is surface "gravity" caused by the Ring's rotation and somewhat attenuated by the sun's gravity - in fact the surface gravity is almost identical to Earth's. However, the cost of gaining standard gravity with rotation is that it's not easy to get off the Ring. Orbital velocity near earth's surface is only about 5 miles per second and escape velocity is only about 7 miles a second - velocities that can be achieved with chemical rockets. On Ringworld, however, any object lofted away from the surface must achieve a velocity of 740 miles/second in the right direction or the velocity it already has by being on the Ringworld will slam the object into the Ringworld's surface with great force. On the other hand, if there were an way to get to the outside of the Ring, simply letting go would give you enough velocity to escape the star's gravity entirely. For that matter, of course, even landing on the Ringworld would be tricky, since matching the surface's velocity would be required and that velocity is far above the natural velocity of an object orbiting the Ringworld's sun at the Ringworld's radius. In the novel, the heroes crashland but this is not recommended for anyone without an impervious stasis field.

Exercise for the student of materials - how strong is the Ringworld's material? Very strong indeed to survive the tension induced by the tremendous spin, but can you calculate how strong it would have to be? How would you assemble the Ringworld? Can you calculate the trajectory of a rocket launching from the inside of Ringworld, relative to the Ringworld? Relative to inertial space?

Here's a demonstration of the difficulty in taking off from Ringworld. At 8 miles/second a rocket would leave earth easily, but on Ringworld at the same velocity a projectile crashes badly and is moved to the left of the takeoff point (assuming that the ring is rotating rightward). Aiming slightly left or right causes no real change except that the same angle of launch results in slightly different maximum altitudes and displacements on the ground (aiming against the spin improves the height by about 36 miles over aiming with the spin - not very useful).

I got a little carried away with calculating the differences between a planet's gravity and the pseudo-gravity on Ringworld. Here's a plot of the time a rocket would spend in flight if launched straight up with various initial speeds - not too much different with low speeds.

But quite different at only slightly higher speeds.

The same goes with maximum height achieved by the rocket. Not much difference at first -

A lot different later.

Two interesting not-obvious implications of the Ringworld's layout are the lack of natural resources and the lack of seasons. Resources are lacking because Ringworld just isn't that thick and was not formed by geological processes - there are no oil wells to tap or veins of metal to mine. If civilization falls, it will be tricky to revive. But what about seasons?

What causes seasons on earth? The change in length of day and angle of incidence of sunlight as the earth revolves around the sun changes the amount of heat the sun provides to a particular place on the earth. The distance from the sun to the earth does change but plays no significant effect on seasons - in fact the Earth is closest to the sun during January (northern hemisphere's winter).

On Ringworld, the length of day is constant. While this could be changed by adjusting the distance between the shadow squares (note that the shadow squares aren't in orbit around the sun either - they're connected by improbably strong wires and are spinning faster than necessary to stay in orbit), it's hard to imagine getting a useful amount of day length change over a long period and the mechanism to do so would be pretty complicated. Changing the distance to the sun is also possible (but see what happens two slides further), but since the Ringworld rotates with a period of 9 days or so, seasons would be very short.

But it turns out that there is one other thing to change about Ringworld.

Here's a concept called the Oscillating Ringworld. If we move the Ringworld so that the Sun is no longer in the plane of the Ringworld, gravity will act as a restoring force. With no friction, oscillation occurs and goes on indefinitely, changing the angle of incidence of light on the Ring - Seasons! The equations go as follows. There is a gravitational force on the Ring and an equal and opposite force on the sun. The Ring mass is about 1/1000th of the Sun, so the Sun's oscillation is a thousand times smaller than the oscillation of the Ring. The period turns out to be about 377 days, giving a reasonable length to the seasons. This analysis relies on a small angle approximation, but would be reasonably accurate for angles up to 10 or so degrees, which would give significant seasonal effects (insolation would vary by 1.5% due to the angle, and 3% due to the increase in distance from the sun, adding up to a variation of about 5%, which is significant enough - compare with the change in insolation over a year due to earth's orientation - another exercise for the student!). Note that there are two winters and two summers in each cycle - an "up winter," a "down winter," an "up-going summer" and a "down going summer". Also note that the period of 377 days is just the same as the period for a planet moving in the Ringworld's orbit. There are only so many ways to combine the gravitational constant, the mass of the sun and the mass of an object to get an answer in units of time, so it's not surprising that the same answer turns up in a few different places. By the way, the mass of the Ringworld is actually significant even compared to the huge mass of the sun, so for the calculation of the oscillation's period I need to include both masses, instead of neglecting the smaller mass, which can be done in most planetary orbit calculations.

Now for the bad news. Although moving the Ring so the sun is out of plane leads to a nice gravitational restoring force, moving the Ring so the sun is off center doesn't. This can be demonstrated without calculating the whole force on the Ring, just by calculating the forces due to gravity from small arcs of the Ring. On the near side, the arc contains a mass proportional to (R-x) and the effect of this mass is divided by a distance of (R-x) squared. On the far side, the opposite arc has mass proportional to R+x and the effect is divided by (R+x) squared. These two effects don't balance - any slight offcentering will get worse and worse. The fact that the Ring is rotating doesn't make anything worse or better - I think (someday I will do a full-up analysis to make sure though).

Note that a Dyson sphere is much better off. The mass contained in an arc at distance (R-x) is proportional to (R-x) squared, so when this is divided by (R-x) squared to get a force, that exactly balances the force due to the opposite arc. The sun can be placed anywhere inside the sphere and will feel no force moving it elsewhere. In Ringworld Engineers Larry Niven revealed that the Ringworld has attitude jets along its edge which convert solar wind into thrust, making the Ringworld stable by providing a restoring force that increases properly as the off-centering gets bigger. The only problem is that someone has stolen most of the jets.

Let's talk a little more about stability, since I mentioned it.

Stability is not the same as equilibrium - for a system to be in equilibrium all forces need to balance, but to be stable, the system has to be robust to small perturbations. A pencil balanced on its point is in equilibrium, but not stable. One on its side is in equilibrium and stable.

This chart shows the different kinds of stability. The lines are potential energy functions. The oscillating Ringworld is as stable in the vertical direction as a ball in a bowl is. Any perturbation simply changes the magnitude of the oscillation. In the horizontal direction though, the Ringworld is completely unstable - any perturbation causes a complete disaster as the Ring tends to get more and more off center. The Dyson sphere is neutrally stable. Any perturbation just moves the Sphere slightly but gives it no tendency to move further along or to return to the original position. Finally, with attitude jets, the Ringworld is probably meta-stable - it will recover from small perturbations, but be vulnerable to a large perturbation. Most systems in the real world are metastable; they will stay put, if they're not pushed too far - just like most people.

It's worth noting that if the impact of light on the shadow squares causes a greater outward force than gravity produces an inward one, then the shadow squares are stable horizontally but unstable vertically. In other words, because the dominant force is outward, not inward, all the signs reverse making stable situations for the Ringworld into unstable ones for the shadow squares and vice versa.

Here's the real Ringworld potential function, calculated by integrating the total force on the Ring - note the rapid drop off. That's why even with attitude jets, the Ring is probably only metastable - a big perturbation might overwhelm the jets' ability to restore the Ringworld to its proper place.

In Greg Benford's Tides of Light, a character named Killeen is dropped through a planet (long story). More recently, in John Cramer's Twistor, some valuable equipment takes the same kind of trip, when accidentally converted to a form of matter that is affected by no force but gravity. The question of what would happen in such a situation is interesting. It turns out that if we assume the earth has a uniform density and isn't rotating, that travel through a straight, frictionless tunnel is very simple to analyse. The force on the object in the tunnel is given by this equation, but it is only the force parallel to the tunnel's length that matters, so we get this equation. What simplifies this equation is that once the object is at (say) this point along its path, the gravitational force of this part of the earth completely cancels out. Only the mass here matters (this fact was discovered by Newton himself). When this fact is incorporated into the equation, it simplifies to the equation for simple harmonic motion. The length of the tunnel drops out entirely, so the total travel time is constant regardless of whether the endpoints are Baltimore and DC or Baltimore and L.A. The duration of a round trip depends only on the acceleration of gravity at the earth's surface and the radius of the earth and equals 84.4 minutes. This turns out to be a period that turns up frequently. It's also the period of a satellite orbiting just above the earth's surface (even at 500 km the period is only 94 minutes) and the period of a pendulum whose length is the radius of the earth. Not surprisingly the maximum speed of something dropped through the tunnel is about 5 miles per second, which is orbital velocity at the surface of the earth.

It's interesting to see how the answer changes if you take into account the change in the density of the earth as a function of the earth's radius. When I first wondered about the effects of such variation I concentrated on the two obvious special cases:

By the way, I used to think that Arthur C. Clarke had gravity transport in mind in City and the Stars/Against the Fall of Night, but when I checked it out recently, it's not entirely clear that this is true.

Deciding which mass distribution results in the quickest trip is a good test of intuition. For the black hole case, the object accelerates down a gravity well that gets very deep, but spends a great deal of time in the very flat part of the well. In the hollow shell case, all the acceleration happens during the trip through the shell and the rest of the trip is at a constant speed - the question is what that constant speed is. It turns out that the delta velocity due to the trip through the shell gets smaller as the shell gets thinner, so the total time to get across the shell can get arbitrarily long (the velocity gained during the trip through a thin shell is the square root of the acceleration of gravity at the surface of the shell times the thickness of the shell - but watch the units).

For the black hole case, the funny thing is that the longer the trip, the shorter the time it takes. For a very short trip, the roundtrip time is only slightly shorter than the 84 minutes we arrived at for the solid earth case, because even for the solid earth case, almost all the mass of the earth can be treated as if it were compressed at the earth's center. For longer trips (trips that go closer to the center to the earth), the object gains a lot of velocity by cutting close to the infinite gravity well - simulations indicate that by going within a couple of miles of the black hole, the length of the round trip declines to about an hour.

It should be noted that the hollow earth case is one that a lot of authors get wrong. There is no gravitational force felt inside a really hollow sphere - so stories in which people are standing on the inside surface are wrong. On the other hand, if the sphere has an internal atmosphere, then there will be a small gravitational force pulling inwards, as Hal Clement noted in Still River

By the way, the size of the black hole holding all the earth's mass is pretty small (2GM/c/c=0.44 cm), so missing it by a few miles keeps you well away from its event horizon and keeps your maximum speed well less than light speed (no relativistic effects), but tides might be a problem (see tide equations on previous pages).

Now some of you are probably wondering about the effect of the Earth's rotation on this method of travel. There is one, but it's not as bad as it might seem. Tunnel 1 runs parallel to the earth's rotational axis, so the any acceleration due to the rotation is always perpendicular to the motion of Killeen's body, and so has no effect on that motion (as long as we assume the tunnel is completely frictionless). Tunnel 2 goes through the earth's rotational axis, so the acceleration due to the earth's rotation is always outward along the path of the tunnel. This requires some further analysis. The rotational velocity at the surface of the earth at latitude x is given by the distance of the surface from the axis and the period of the earth's rotation. The rotational velocity of a point in the tunnel is linearly related to that and to the distance of the object from the earth's axis. Combining these two factors we get a rotational velocity in terms of distance along the tunnel and the period of the earth's rotation. The acceleration due to this rotational velocity is given by this familiar equation, giving us the outward acceleration due to the earth's rotation (frictionless walls are really needed here, because the object would touch the walls throughout its trip). Combining this with the gravitational acceleration derived earlier, our differential equation is still simple and the solution is still harmonic motion, just with a different period. The new period of Killeen's oscillation through the earth is only 8 seconds longer than it was before. So, a trip that goes to an opposite latitude while staying at a given longitude is acceptable, a trip that goes to an opposite longitude at a given latitude is also acceptable, and in fact, any trip with a constant latitude (even if it did not go through the axis) would also be acceptable and have the same period as derived above. What's not acceptable? Well, any trip that changes latitude, but doesn't go to an opposite latitude would cause a rotational acceleration that was always in the same direction - Killeen would rocket out of the tunnel or perhaps get stuck part way through. I calculated one specific example - imagine a tunnel going from the North pole to the equator. It turns out that the final velocity of Killeen as he left the tunnel at the equator would be about 3 tenths of a mile per second - pretty fast. If the earth rotated as fast as Hal Clement's Mesklin (Mission of Gravity) the rate of egress would be a lot faster, but I wouldn't be justified in assuming a spherical Earth any more.

These are some of the handiest equations for dealing with orbital mechanics in a science fictional environment. The total velocity of an object at any point in its orbit is equal to a constant times the difference between twice the reciprocal of the current distance from the primary and the reciprocal of the average distance from the primary. What this gives you (among other things) is the delta-v for transfer orbits. If you want to travel from earth to Mars, simply calculate the current orbital velocity of earth, and then the orbital velocity of an object currently at earth's radius but with a maximum distance that just reaches Mars' orbit. That gives you the dV to apply. Once you reach Mars the same equation gives the dV that will put the spacecraft in the same orbit as Mars. What makes this equation particularly useful is that you can pick your units for your convenience. When I was taking courses I used units of astronomical units for r and a, and units of miles per second for velocity whenever possible, so that for calculations in the solar system I could determine GM by taking the earth case - all I needed to remember was the length of the year and the size of earth's orbit and I could determine the earth's orbital velocity, and since the distance term in my units was (2-1), GM was easy to solve for and easy to use for any subsequent solar system problem without the pain of memorizing G or M.

The applications to SF for these equations are pretty obvious, but one thing I'd like to highlight is that at any point in an orbit, increasing velocity increases your orbit's semi-major axis, and decreasing velocity decreases it. The trick is that for any given orbit, a nearby orbit with a larger semi-major axis will have a smaller velocity (this time r is changed as well as a), so if you attempt to "catch up" with something in a higher orbit by speeding up, you'll end up falling behind. As John Brunner said in Shockwave Rider, "see you later, accelerator"

There's an old saying in the Smoke Ring.

Is it true? Why? Imagine yourself in the Smoke Ring with a jet pack at your command and think about the equations on the previous page:

If you apply a thrust eastward (in the direction of your orbit), you put yourself in a higher orbit (you move Out);

If you apply a thrust Westward (against the direction of your orbit), you put yourself in a lower orbit (you move In);

If you apply a thrust outward, you put yourself in a slower orbit, so you move West relative to everything else in your old, faster orbit;

If you apply a thrust inward, you put yourself in a faster orbit and you move East relative to everything else in your old, slower orbit.

If you thrust to the left or right, you move to an orbit that is at an angle to your original orbit, but which intersects your original orbit at two points, one of which is the point at which you applied the thrust - hence you come back to where to started after one orbit.

The "old saying" compressed all that knowledge into a few sentences.

Now for that promised weird stuff that didn't quite fit in to the other categories.

Let's take a simple premise - that it is possible for a technological species to create vehicles with relativistic velocities. Within a few decades, we might be able to create such vehicles. They have the following characteristics:

  • Quick travel times - with a few decades of travel one could reach dozens or hundreds of other star systems.
  • High destructive potential - if one hit a planet, it would be worse than a huge asteroid strike, just because of the speed of the impact.
  • No conceivable defense - Defense against such a vehicle is very difficult because the huge momentum such an object has would be impossible to deflect, and mere detection would be difficult because the object is right behind the its own light.

Killing Star (by Pellegrino and Zebrowski) suggests that the possibility of such vehicles might lead all intelligent life forms to try to destroy all other intelligent life as soon as it's detected due to simple prudence. This is one of the key strategies of SF - taking a simple premise and finding the most outrageous (and horrifying) but plausible consequences.

Here's another simple premise: Teleportation - it's not very likely but what if it were possible?

What are the implications? Some are obvious (no airplanes or cars except for fun), some are less so.

A velocity damper is needed to absorb the potential energy difference that is produced when you teleport from a mountain to a valley and the velocity difference that occurs when you teleport from Canada to Florida (different tangential velocities due to different latitudes) or New York to LA (a vertical velocity due to the rotation of the earth).

A flash crowd is a crowd that appears whenever and wherever something interesting is happening. If we assume that teleportation is cheap and easy, a crowd can grow very quickly, since it draws on the whole world's population of possibly interested parties. We see some similar effects with popular web sites - "teleporting" to a web site is easy, so an overwhelming number of hits can happen to any site that is attractive.

No good reason, just a favorite quote, which captures the idea that knowing the causes of something does not dilute one's pleasure in seeing it.