Monthly Archives: January 2006

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So please, make yourselves at home. Have a look around. We’re glad to see you!

Steller Cartography

Most of us at some point had to learn the names of the nine planets, but for some reason few of us know anything about the geography of our immediate galactic neighborhood. You’re probably aware that the Alpha-Centauri system is the closest to our sun, but can you name any other close stars?

I couldn’t. Since we geeks have been dreaming of traveling the stars at least since the golden age of sci-fi, you’d think we’d know more about where we’d like to travel.

nearstar.gif

Click image to enlarge.

Here are the closest 10 star systems (from closest on out):

  1. Alpha Centauri is a triple star system located about 4.3 light years away. The closest of the three stars is the tiny red dwarf, Proxima Centauri. The other two stars rotate around each other at the distance Saturn is from our Sun. They are both close to our sun in size and temperature.

    most astronomers believe that stars of spectral types from about F5 to K5 are hot enough, but long-lived and stable enough, to support potential Earthlike worlds.

    Both Alpha Centauri A and B fall within this range. Alpha Centauri A is a G star like our Sun, Alpha Centauri B is a K1 star. The star types, from hottest to coolest are O, B, A, F, G, K, M.

    According to Wikipedia, Alpha Centauri A and B rotate at a sufficient distance to allow rocky earth-like worlds with liquid water to rotate either star. Such worlds rotating either star would have a secondary sun at night for half of its year – a prolonged twilight.

    Outer gas giants like Jupiter could not exist in this binary system, and that could be a problem because gas giants are thought to be responsible for bringing comets in to seed inner planets with water and other biological building blocks. But if the twin stars served the same purpose for each other, this might not be a problem at all.

    Viewed from near Alpha Centauri, the sky (other than the Alpha Centauri stars) would appear very much as it does to observers on Earth, with most of the constellations such as Ursa Major and Orion being almost unchanged. However, Centaurus would be missing its brightest star and our Sun would appear as a 0.5-magnitude star in Cassiopeia. Roughly speaking, the // of Cassiopeia would become a ///, with the Sun at the leftmost end…

    You know…in case you ever find yourself in the Alpha Centauri system and need to find your way back home. It’s only “news you can use” around here my friends.

  2. Barnard’s Star is a red dwarf located 5.96 light years away. A red dwarf is a class M star – a star that is too cool to be considered a good candidate for life-bearing worlds.
  3. Wolf 359 is a red dwarf 7.78 light years away.
  4. Lalande 21185 is a red dwarf 8.29 light years away. It is known to have two gas giant planets. A third large planet is suspected.
  5. Sirius is a binary system containing one star that’s thought to be too hot for life (Sirius A) and a white dwarf (Sirius B) that’s far too cool. White dwarves are even cooler than red dwarves. This binary system is 8.58 light years away.
  6. Luyten 726-8 is a binary system of two red dwarves.
  7. Ross 154 – a red dwarf.
  8. Ross 248 is another red dwarf.
  9. Epsilon Eridani is a K1 star, so it falls within the class of stars thought to be capable of supporting life. It is not thought to be a good candidate for complex life though because the star is young, it has an extremely variable spectrum (burning hot then cold), and is orbited by a Jupiter-like gas giant called Epsilon Eridani B in a highly eccentric orbit.

    This star is 10.52 light years away.

  10. Lacaille 9352 is yet another red dwarf 10.74 light years away.

This large number of red dwarves is not unusual. Four out of five stars in the universe are red dwarves. In fact, the only other stars within 13 light years that fall within the F5 to K5 range are Epsilon Indi and Tau Ceti.

Epsilon Indi is orbited at a great distance by a pair of brown dwarves that orbit each other. It is on the cool side of stars capable of supporting Earth-like planets.

Since Epsilon Indi is sort of like a distant cousin to Sol, some speculate whether it might just be bright enough to support Earth-type life on a planet lucky enough to orbit in its water zone. The distance from Epsilon Indi where an Earth-type planet could possibly have liquid water on its surface is centered around only 0.38 AU — around Mercury’s orbital distance in the Solar System.

[an AU, or Astronomical Unit, is the distance between the Earth and the Sun]

Tidal lock might begin to be a problem that close to a star. A planet within the liquid water zone might tend to keep one side toward it’s star like the Moon to the Earth. Such a planet would be burned on one side, rare on the other.

Tau Ceti has a different set of problems. Because it is a metal deficient star it is thought to be unlikely to harbor rocky planets. Tau Ceti is surrounded by a dusty disk filled with comets.

Though the star Tau Ceti is similar to the Sun, any planets it has are unlikely to be havens for life, say a team of UK astronomers. Using submillimeter images of the disk of material surrounding Tau Ceti, they found that it must contain more than ten times as many comets and asteroids than there are in the Solar System.

Bottom line: our best bet for a close Earth-like neighbor lies within the Alpha Centauri system.

naechste.jpg

Self-Driving Cars

Per Ray Kurzweil, it’s a question of when, not whether. And probably sooner rather than later:

A U.K. government think tank has forecast RFID-tagged driverless cars on roads by 2056.

“Given the ability of several cars to navigate a complex route in the recent DARPA competition completely autonomously and a General Motors project to demonstrate driverless cars traveling at 60 miles per hour by 2008, the projection of RFID-controlled cars by the year 2056 is a good example of linear thinking,” says Ray Kurzweil. “I believe we can anticipate cars to be doing much of our driving for us in the 2020s if not sooner.”

No word on flying cars. Personally, I think anybody who says we won’t have them by 2010 is engaged in linear thinking. But then, I’m no Kurzweil.

UPDATE FROM STEPHEN: “Beyond Tomorrow” had a segment recently about an anti-collision radar system for passenger cars. Such a system could really cut down on distracted driver-type accidents. It also looked to be ready to market in Europe.

The Mercedes test vehicle has long range and short range radar systems that surround the car. The car is programmed to stop rather than rearend somebody if the driver is distracted.

There are a couple of practical reasons why we’ll have driver assist systems for awhile before we’ll see complete automation. First, these initial driver assist systems won’t have to be anywhere near as sophisticated as those systems that competed in the DARPA Grand Challenge.

Second, there’s the issue of products liability. This Mercedes is equipped with a “driver assist” system, not full automation. It’s a little like a driver’s ed car. There’s a safety brake, but you are still the driver in command. If you have an accident, then (arguably) you couldn’t blame the manufacturer unless a system malfunction directly caused the accident.

But if the car is doing it’s own driving, then obviously the car manufacturer would have a difficult time avoiding responsibility in the event of an accident.

So, we’ll see a slow march toward full automation via various “driver assist” systems. At first it will be simple collision avoidance by braking, then collision avoidance by steering out of the way of a crash.

Eventually these systems will take on all the tasks associated with driving. Then you’ll just give it a destination and sit back and enjoy the ride.

UPDATE AGAIN: Well, that didn’t take long. Apparently Honda UK is offering a driver’s assist sytem that amounts to a full freeway autopilot.

I’ll be taking a wait-and-see approach.

H/T to eisendorn.

Better All The Time #28




Dispatches from a rapidly changing, rapidly
improving world

#28
01/28/06

Welcome to the first edition of Better All the Time for 2006. Our somewhat
belated new year’s resolution is to bring you more good news than ever before.
So beginning with this edition, we will be featuring 12 — that’s right, 12!
— good news stories with each and every edition. So let’s get started!

 

Energy Race Update

Russia wants in on “the energy race” too.

We are planning to build a permanent base on the moon by 2015 and by 2020 we can begin the industrial-scale delivery… of the rare isotope Helium-3,” Nikolai Sevastyanov, head of the Energia space corporation, was quoted by ITAR-TASS news agency as saying at an academic conference.

The International Space Station (ISS) would play a key role in the project and a regular transport relay to the moon would be established with the help of the planned Clipper spaceship and the Parom, a space capsule intended to tug heavy cargo containers around space, Sevastyanov said.

Jules Verne's Elephant

robotelephant2_small.jpgThis is what you get when you cross an Imperial Walker from Star Wars with the Oliphants from The Lord of the Rings – a 30-foot tall robotic elephant!

The 30 foot tall robot elephant was built especially as a part of a Jules Verne centennial celebration. Verne, the author of classics like Twenty Thousand Leagues Under the Sea, and Journey to the Centre of the Earth, would have been absolutely delighted.

The robot not only walked through the streets amazing the crowds, it actually sprayed water on them from its trunk!

Don’t miss the video.

Earth-Like Planet Found

This is pretty cool:

An international team of astronomers reportedly has discovered the smallest, Earth-like planet outside our Solar System.

The planet, known as OGLE-2005-BLG-390Lb, orbits a star one-fifth the mass of the Sun, and has an estimated surface temperature of minus 364 Fahrenheit (minus 200 Celsius), astronomers Michael Albrow and Karen Pollard of Canterbury University told Television New Zealand. They said the discovery might one day lead to finding a twin Earth.

The planet is located about 20,000 light years from Earth; it orbits a star in the constellation Sagittarius. The astronomers who discovered it did so via a technique called gravitational microlensing, which enables distant objects to be detected through the light intensification caused by their gravity. This technique seems a little counter-intuitive. I would have though that a planet passing between us and a distant star would obscure the star somewhat and reduce the amount of light that reaches us. And in fact, maybe it does — but apparently we’ll never find any planets looking for that. Instead, we go looking for the tiny light spike that the planet’s gravity causes, and voila! Now we’re locating Earth-like planets.

I reiterate: pretty cool.

The Energy Race

A couple of days ago China announced plans to complete its tokamak fusion reactor by April of this year. China will start experimenting with the reactor – designated HT-7 – this summer with the hope of hitting a magic breakeven point that has, to date, never been reached in fusion research anywhere. They hope to produce more power than is required to contain the reaction.

Tokamak is a Russian acronym meaning “toroidal chamber in magnetic coils.” A tokamak reactor contains a giant donut-shaped magnet used to contain plasma within the reactor.

The United States has been betting on the success of a different tokamak project: the International Thermonuclear Experimental Reactor (ITER). The ITER has been in the design and planning phase so long (since 1985!) that China may have already leap-frogged the rest of the world with its cheaper reactor.

…Construction [on ITER] is expected to begin in 2008 and finish in 2016. ITER is designed to generate 500 MW (about 10 times the record held by JET) and will hopefully produce more energy than is required to keep the plasma heated and confined…

Which will mean little if China has already accomplished this with a reactor that cost 1/20th the price of the ITER.

Tokamak reactors are powered by deuterium harvested from seawater.

After nuclear fusion, the deuterium extracted from one liter of sea water will produce energy equivalent to 300 liters of gasoline.

This would be a practically inexhaustible supply of power, and China probably has the lead in deuterium fusion research at the moment. Maybe the U.S. will compete with a different form of fusion.

[Deuterium fusion critics] have noted that the neutrons released in the deuterium-tritium fusion would create secondary radiation within the metallic parts of the reactor chamber. This secondary radiation would create radiological waste disposal problem, and would also shorten the life of the components in the reactor through radiative metal fatigue…

If China gets their reactor working, it won’t be easy to operate or maintain. Fortunately, there is the possibility of a cleaner, easier to manage fusion fuel.

[Twenty years ago fusion expert Gerald Kulcinski] and a group of scientists met at a retreat south of Madison, Wisconsin to discuss the problems with the deuterium-tritium fuel cycle for fusion. They talked over what the options are for a better fuel. Helium-3 is what they came up with.

In fact, helium-3 is the perfect fusion fuel. It can produce an incredible amount of power with absolutely no radioactivity. And a helium-3 fusion reactor won’t have the same containment issues either.

Professor Kulcinski’s lab is running the only helium-3 fusion reactor in the world. He has an annual research budget that is barely into six figures and allows him to have five graduate research assistants working on the project. Compared to what has been spent on other fusion projects around the world, the team’s accomplishments are impressive. Helium-3 would not require a tokomak reactor like the multibillion-dollar one being developed for the international ITER project. Instead, his design uses an electrostatic field to contain the plasma instead of an electromagnetic field.

There’s a catch. Unlike the deuterium, which can be obtained from the ocean probably forever, there are only a few hundred kilograms of helium-3 on Earth. You have to go to the Moon to find helium-3 in useful quantities.

In January of 1986 Professor Kulcinski and his group contacted the Lunar and Planetary Institute at the Johnson Space Center. The soil samples from the Apollo missions are stored there. Every sample from the Moon had helium-3 in it. It didn’t matter if the sample was collected from right on the surface or from a core sample a meter deep…

Theoretical calculations of helium-3 abundances on the Moon suggest that it may have enough to supply current world energy demand for thousands of years. Even further out, the gas giant planets contain enough helium-3 to power human civilization for millions of years.

In the short run deuterium will be seen as the miracle fuel. We certainly have plenty of it right here at home. But it will wear out reactors and leave us with some nasty radioactive waste. Ultimately we will turn to helium-3 because it is abundant (if you look in the right places), safe, and manageable.

helium-3 moon map

This lunar map shows heavy deposits of helium-3 in red.