Planets Just Keep Surprising Us

They Show Up in the Darndest Places!

So, planets aren’t just for our solar system anymore. The Kepler Mission is showing us that in the field of view it’s viewing, there are probably well over a thousand worlds circling distant stars (maybe more).  Before Kepler blasted off on its planet-finding survey, ground-based astronomers were finding worlds, too.  Add to that the current crop of ground-based telescopes and the COROT mission findings and the field of planetary exploration beyond our solar system is wide open for discovery!

Every time astronomers spot more planets, the findings rewrite the rule books about planets and where they could possibly exist.  Astronomers once thought that pulsars couldn’t have planets. And, that massive, Jupiter-type planets probably formed well away from their stars. And that clusters packed with stars probably didn’t have planets.

Well, all of those rules have been broken. There WAS a pulsar with a planet spotted in 1992, and it was a great discovery.  More recently, there have been enough so-called “hot Jupiters” discovered close to their stars that astronomers have been reconsidering theories of planetary formation to account for just how those hot bad boys get up close and personal with their stellar hosts.

Astronomers have discovered two gas giant planets orbiting stars in the Beehive cluster, a collection of about 1,000 tightly packed stars. Image credit: NASA/JPL-Caltech

Now, the first time, astronomers using a ground-based instrument at the Smithsonian Astrophysical Observatory’s Fred Lawrence Whipple Observatory in Arizona found two planets as they studied the crowded inner regions of the Beehive Cluster, which is a pretty crowded place for a planet to grow up.  They found these so-called “hot Jupiters” by measuring the slight gravitational wobble that orbiting planets cause in the motions of their parent stars.

This was something of a surprise because earlier searches of other clusters had turned up two planets around massive stars but none had been found around stars like our Sun until now.

The two new Beehive planets are called Pr0201b and Pr0211b. The star’s name followed by a “b” is the standard naming convention for planets.

So, what does this discovery mean?  Identifying a couple of boiling hot planets in a crowded starfield is pretty good evidence that planets can sprout up just about anywhere. I mean, if they can exist near pulsars, which are pretty hostile environments created by the deaths of supermassive stars, then cropping up in a region where the stars are thick (but not yet dying) may not be so difficult.

If you’ve never seen the Beehive, it’s a cluster most easily visible overhead starting in early spring.  All its stars formed from the same nebular birthplace, so they have pretty much the same chemical compositions.  So, at least two of the stars have enough heavy elements surrounding them in circumstellar space to create planets.

Want to learn more about these Beehive Bad Boys?  Check out the NASA press release right here!

What’s Infrared and Why Do We Care?

The James Webb Space Telescope Will Tell Us

What a person looks like in infrared wavelengths of light. Courtesy IPAC/CoolCosmos.

Infrared astronomy is not new — it’s been around for decades, but it continues to shake up our view of the cosmos. In particular, it lets us peek into warm places in the universe that we couldn’t see into with other types of telescopes and detectors tuned to visible light or other parts of the electromagnetic spectrum.

Infrared radiation is given off by warm things. YOU glow in the infrared, although you probably never gave it much thought.

Out in the larger universe, infrared radiation from hot young stars, for example, can slip through the clouds of gas and dust that surround them. This makes these once-hidden objects detectable to us — “visible”, in a sense and in a way they weren’t when we looked at those same clouds of gas and dust with optical telescopes.

The best way to study the universe in infrared wavelengths is to send spacecraft out beyond our infrared-interfering atmosphere. So, in recent decades such telescopes as the Spitzer Space Telescope, the Herschel Observatory and new instruments on the Hubble Space Telescope have extended our view of the planets, stars and galaxies into new realms of discovery.

There’s a new kid on the infrared detection block called the James Webb Space Telescope that is being readied for launch in a few years. It will be a high-resolution eye on the infrared universe and answer a lot of questions about processes of star formation, the activities of hidden black holes at the hearts of galaxies, and the search for worlds around other stars.

Want to learn more about it?  NASA has a great little video out that answers a lot of questions about JWST and the infrared universe. You can see the video and read more about the project at the JWST web site.

CROWD-SOURCE SCIENCE FUNDING:  WE CAN DO IT!

Speaking of cutting-edge research, my friends over at the Uwingu project are nearing the end of their crowd-sourcing campaign. They have only a few hours left today (Friday, September 14th, 2012) before campaign ends.

These guys are absolutely serious about funding good science research that isn’t getting funded and should be. Here’s where you come in.  You can join the push for funding for as little as $10 (or even less) and you get some cool perks along with your contribution.

What’s not to like?

You part with the equivalent cost of a Venti latté and a brownie, or a personal pan pizza and a drink, or a beer and some wings, or maybe some music downloads, and in the not-too-distant future, a researcher gets a chance to answer a burning scientific question — with YOUR help. So, head on over to their Web site and make a difference.  I did!   And, after you join up, they’ll send you some perks and keep you posted on an exciting new product they’ll be selling to help fund science into the indefinite future. Check it out!