New Clue to Extrasolar Planetary Systems- Lithium!

Astronomers have known for some time that sunlike stars with high iron content are more likely to harbor planetary systems than other stars. Now they have a new clue- the amount of lithium. As we know from class, using spectroscopy we can determine the composition of faraway stars. So now we know that if a star has high iron and low lithium it is very likely to have planets. But why low lithium?

Garek Israelian, with the Instituto de Astrofisica de Canarias in Spain have analysed data from 133 sunlike stars. The leading explanation is that having planets around a newly forming star slows the rotation- and allows the lithium to sink lower into the core of the star where it can be consumed by fusion as part of the star's energy source. Without the drag of the planets, the star spins faster and the lithium stays near the surface, where temperatures are too low for lithium fusion to occur.

This is only true of sunlike stars near the middle of the main sequence on the H-R diagram. Small red stars always burn up their lithium quickly regardless of whether there are planets or not; large blue stars experience layering that prevents the mixing of the elements.

Even more planets discovered via "wobble" method

An international group of astronomers using the High Accuracy Radial Velocity Planet Searcher (HARPS) have announced the discovery of 32 new planets, with many more announcements on the way. They had already announced the discovery of 43 other planets, bringing the total so far to 75. This is the result of a five year program of the European Southern Observatory that used a telescope in Chile.

Among the 75 planets discovered are 24 so-called super-Earths; planets with a mass just a few times that of Earth (not gas giants.) Only 28 super-Earths in total have been discovered by researchers around the world. This radial velocity method which looks for wobble is very good at finding these smaller planets.

The following link will show you an animation that demonstrates how the Radial Velocity Method works.

Radial Velocity Method

http://commons.wikimedia.org/wiki/File:Planet_reflex_sm.gif

Probe to crash into the moon on Parents Day!

A final location has been decided for the two-part lunar crash probe, part of the mission known as LCROSS (Lunar CRater Observation and Sensing Satellite), "On 9 October, at around 11:30 GMT, LCROSS will send its Atlas V's Centaur rocket upper stage towards the lunar surface (see pic). Four minutes after impact, LCROSS will descend through the plume using two "two near-infrared spectrometers, a visible light spectrometer, two mid-infrared cameras, two near-infrared cameras, a visible camera and a visible radiometer" to sniff the resulting chemical mix." (http://www.theregister.co.uk/2009/09/29/lcross_retargeted/ )

The LCROSS probe itself will then crash into the moon. The hope is that it will find evidence of water.

Well it all went as planned, and information about the event from NASA can be found at http://www.nasa.gov/mission_pages/LCROSS/main/index.html

A great video simulation can be found at http://www.nasa.gov/mov/391565main_LCROSS-MediaPreview.mov

A new, giant, massive ring has been discovered around Saturn- so large that a BILLION earths could fit in it! It is more than 300 Saturns wide! How could astronomers have missed it?

Well, it turns out the ring is almost invisible, that's how. While it is about 40 million kilometers across it is exceedingly thin. It is made of dust-like ice and rock particles that barely reflect any of the feeble sunlight that reaches Saturn- but the sun does heat them up. So it was the Spitzer infrared telescope that finally noticed the giant ring.

Remember the Rovers?

The Mars Rovers are the robots that were sent to Mars when today's juniors and seniors in high school were still in middle school. They had a three month mission. They've been at it about five years. In fact, just a month ago the rover Spirit celebrated its 2000th "sol", or Martian day. It's been experiencing some rough weather recently- dust storms.

Thr rover Opportunity, on the other hand, has been plodding away. In fact, in the photo below, you can see a photo of Opportunity taken by an orbiting satellite. If you look carefully, you can even see the wheel tracks it has left behind. Opportunity has travelled over 100 meters in a day. It is headed toward an interesting crater named Endeavor. At this rate, it will be thee in about two Earth years.

Credit: NASA/JPL/University of Arizona

New lease on life for Hubble

If you are a regular follower of this blog, then you know that last October it carried a story about the Hubble Space telescope upgrade being cancelled. (See http://sms-astro-08.blogspot.com/2008/10/hubble-time-to-say-goodbye.html)

Then of course the astronomy class is not offered again in the spring, so the blog hibernates. Well, last spring the Hubble was in fact rejuvenated- last May, shuttle astronauts did a series of repairs and upgrades and two new instruments were added. The official NASA press release can be found here.

It took three months of calibrations to get the telescope back on line, but today NASA released some of the images taken by the refurbished Hubble. Plans are to observe "Kuiper Belt objects at the fringe of our solar system; survey the birth of planets around other stars; and probe the composition and structure of extrasolar planet atmospheres; take the deepest-ever near-infrared portrait of the universe to reveal never-before-seen infant galaxies that existed when the universe was less than 500 million years old;and shed light on the behavior of dark energy, a repulsive force that is pushing the universe apart at an ever-faster rate."

The picture at the top of this blog gives some idea of the amount of detail the images contain; the image below is of colored stars in a cluster actually zoomable on the Hubble site itself.

Beautiful Astronomy

In class we were discussing telescopes, and how they can show us things our eyes can't see because they collect more light by having bigger "pupils" (apertures.) Another way to collect more light is to spend more TIME collecting the light- this is what cameras do. Dr. Belknap, who is now in Jordan, alerted me to the first annual Astronomy Photographer of the Year contest, sponsored by England's Royal Observatory. Two British newspapers have posted some of the entries on their web sites- the Telegraph and the Guardian.

These are worth looking at- hard to pick a favorite, but the image above is quite nice. It is from the Telegraph site, and is described as

This colourful nebula, known as the Gabriela Mistral Nebula, contains a mass of giant, hot young stars. The bright colours are caused by different chemical elements found in the nebula as energy released from the stars excites the atoms and causes them to glow with different colours of light. It is named after the Chilean poet Gabriela Mistral as it is thought to bear a striking resemblance to her in profile.By Steve Crouch