Archive for the ‘Other Contributors’ Category

A Younger Version of Our Solar System

By Bellatrix

New information about a neighboring star has shed some light on our theories of solar system formation and given hope to terrestrial planet hunters. The near by star Epsilon Eridani has features very similar to our own solar system, it is however much younger than our own system, perhaps giving us a glimpse to how our solar system might have looked in its very early stages.

The star itself is about 10.5 light years away. It is the third brightest star seen with the naked eye. The star is a K2 spectral type star; it is slightly smaller and less massive than the sun. It is thought to be less than a billion years old, where our sun is close to 5 billion years old. Because of it’s young age it has a much higher level of magnetic activity than the sun and a stellar wind about 30 times as strong.

Recently, using the Spitzer Space Telescope, astronomers have identified two areas of rocky rings, or asteroid belts, just like our solar system. It has an inner asteroid belt at an equivalent distance from its star as our asteroid belt to the sun. An outer asteroid belt is also present at about the position where our Uranus is. This outer belt contains about 20 times more material than the inner belt. A third ring of icy materials is set out about 35 to 100 AU from the star, very similar to our Kuiper Belt but with about 100 times more material. This extra material makes sense, given the systems age. Our solar system is much older and thus has had more time for collisions to take place and either destroy material or send it out of orbit.

Spitzer also noticed large gaps in these rings. The most logical explanation for these gaps is the presence of planets. Astronomers predict at least three planets with masses between that of Neptune and Jupiter, and another possible smaller planet may lie near the innermost ring. These gaps and the closeness of this star, plus evidence from other planet hunting techniques such as observing radial velocities, makes this star high on the list of planet hunters trying to find earth like planets, and even possibly life. With all the similarities noticed thus far between the two systems, one might think it surprising not to find smaller rocky planets in the inner part of the system.

Studying this system is exciting ad enlightening for astronomers. Seeing that our solar system is not totally unique means that our theories about how solar systems for may not be completely off base. Also, studying this solar system more intensely may show us things about our early solar system we wouldn’t have otherwise known. As the resolving power of our telescopes improve new discoveries from this system should be something to watch out for.

Votes from Space!

By Reynolds William

And to think some people can’t be bothered because “There wasn’t any parking at my polling place…” Actual quote.  Sigh…. Let me see if I got this straight, astronauts circling in orbit can cast their votes in the general election, but 1 parking spot too few is enough to delay your civic duty 4 more years?

I’m not trying to spin up some indignant rhetoric around patriotic duty and whatnot, but considering how many people have given their lives to obtain and protect the freedoms we enjoy – not the least of these being the right and privilege to determine our leadership through general elections – it seems a tad remiss to take a pass on casting a ballot because of a lack of convenience.

http://www.nasa.gov/mission_pages/station/expeditions/expedition18/vote_110408.html

Where’s That Antimatter Coming From?

By Bellatrix

One great mystery about our galaxy right now has to do with a cloud of antimatter near the center of the galaxy. No one knows exactly how or why this antimatter is being generated. However, data being looked at from the last four years, from the European Space Agency, may have had a bit of a break through.

Antimatter is the antiparticles to matter; where normal matter is made up of particles, antimatter is made of antiparticles. Each antiparticle has the same mass as its matter counterpart but is opposite in electric charge and magnetic properties, for example the antimatter partner to an electron is a positron. When matter and antimatter collide they annihilate releasing a large amount of energy.

This cloud of antimatter was discovered in the 1970’s. It is about 10,000 light years across and generates the energy of 10,000 suns. The cloud shines brightly with gamma rays; this is because of the antimatter colliding and annihilating with normal matter. Their interaction releases high-energy gamma rays, which allows for us to detect the antimatter’s presence. For years scientists have theorized the antimatter coming from radioactive elements produced in supernovae, or that the positrons are coming colliding stellar winds or other types of novae. But there was in evidence to really support any of these theories.

Now with data from the International Gamma-Ray Astrophysics Laboratory, or INTEGRAL, astronomers have noticed something new. The cloud extends further on the western side of the galactic center than on the eastern side. This location matches of very well with the distribution of a population of hard low-mass x-ray binary star systems. These star systems consist of a low mass star orbiting with either a neutron star or a black hole. X-rays are given off when gas from the low mass stars falls in on the neutron star or black hole. Because the positions of the binaries and antimatter line up so well astronomers believe that the binary systems are producing half or all of positrons seen in the cloud.

We now may have a good idea of where the antimatters coming from, however we still have no idea how/why exactly the binary systems are producing these positrons. Astronomers believe it has something to do with the jets of relativistic material and areas of strong magnetic fields that can be common with these types of systems. With the GLAST space telescope having been launched and starting to collect data, we could potentially gain a lot more insight into what exactly is going on very soon.

A Mirror of Our Creation

By Evan Finnes

In a planetary system only 10 light years away, Spitzer has discovered that there is much more to Epsilon Eridani besides a great setting for an Asimov novel. Epsilon Eridani is the star at the center of the planetary system closest to home. This Star is relatively young, perhaps less than a billion years old, and has a mass which is about .85 times the mass of the sun. As far as atomic creation goes, this sun is relatively inactive, producing not much more than Helium.

This system has been a source of great discovery; in the past it has been found to host two planets, an asteroid belt which orbits the star at a similar distance to which our asteroid belt orbits the Sun, and distant ring of dust and ice which is very similar to our Kuiper Belt. Recently, Spitzer observed that there is not just one, but two asteroid belts orbiting the not so distant star. What makes this discovery so exciting is the idea that by observing this system, we are basically looking back in history to observe our own creation.

According to the Nebular Hypothesis, solar systems are formed because massive clouds of dust and helium condense to form stars. This condensing occurs because these clouds are gravitationally unstable, so they collapse inwards into smaller clumps which accumulate to form a star, such as our Sun or Epsilon Eridani. As this star forms it sheds a disk of matter which over time begins to accumulate and form protoplanets. Although planetary formation is not well understood, it is thought by some that because of the gravitational pull of the forming star, the dense accumulating rock stays closer to and orbits the star, while the less dense gasses are able to stay further from the star in their orbit. This could be why the terrestrial planets such as Earth are closer to the Sun, while the gas giants such as Jupiter form much further out (of course there have been recent discoveries of gas giants closer to the sun than even Mercury).

Some theorize that the asteroid belts in our solar system are the result of the tidal forces produced by the gravitational pulls of the Sun and the gas giants. These tidal forces keep the rocks in the asteroid belt from coalescing to form protoplanets. The gas giants might also have another roll in solar system formation. It is possible that that the gas giants sweep out asteroids as they rotate the star, protecting the terrestrial planets from catastrophic impacts. However, some scientists also believe that the gas giants could act has a gravitational sling shot which could attract and hurl asteroids into the inner solar system.

One of the planets discovered to orbit Epsilon Eridani is located about 3.5 Au’s from the star, just outside of the range of the newly discovered asteroid belt. This is the first time a planetary system has been discovered to have an arrangement which is comparable to Jupiter and our asteroid belt.

Does this discovery prove that our solar system was formed with agreement to the Nebular Hypotheses? No, but it is defiantly worth observing this relatively young star system to see if its evolution correlates at all with any of our ideas. Who knows, maybe we could even watch as the formation of an Earthlike planet unfolds before our very eyes.