Methane!

An Organic Molecule Worth Detecting

Organic molecules are the key ingredients for life. They are what scientists call life’s “building blocks.” So, it’s a big deal when astronomers detect such things in interstellar space. Even more so when they find them in places where life might form — like on extrasolar planets.

Astronomers using the Hubble Space Telescope have made the first detection ever of molecules of the gas methane in the atmosphere of a planet orbiting another star. As you can imagine, this is a huge breakthrough because identifying signs of life on other planets depends on finding evidence of such organic molecules. Under the right circumstances methane can play a key role in the chemical reactions that have to occur in the life-creation chain.

Methane has been detected on most of the planets, and many moons and comets in our Solar System in both gas and ice form. However, this is the first time any organic molecule like methane has been detected on a world orbiting another star. It was found in the atmosphere of a Jupiter-sized planet called HD 189733b by scientists using HST’s Near-infrared Camera and Multi-object Spectrograph (NICMOS) to break down the light from a more-distant star as it passed through the planet’s atmosphere. The planet happened to pass in front of the star, and as the star’s light traveled through the atmosphere, some of it was absorbed by gases, including methane and water vapor. That left a unique fingerprint in the spectral data, telling the astronomers that those gases exist at the planet.

Methane is composed of carbon and hydrogen. On Earth, methane is a naturally occurring product, and is also produced by a processes and life forms as varied a cattle, termines, the decay of matter in ocean and wetland environments, waste landfills and as a by-product of energy generation. It’s pretty unlikely that the methane on the distant planet around HD 189733b is generated by life, since the planet’s atmosphere is much too hot. Chances are HST noted higher methane levels on the night side of the planet, where the gas can exist in greater amounts. On the day side, the higher heat would tear apart the molecules, resulting in a lower amount of methane.

These measurements are a big step toward understanding other atmospheric conditions at this planet, or others where organic molecules will be found with HST, Spitzer, and the future James Webb Telescope.

RIP Sir Arthur C. Clarke

A Titan Passes

In recent weeks, I’ve been re-reading some of my favorite older science fiction, including some of Sir Arthur Clarke’s works: 2001: A Space Odyssey, 2010, Childhood’s End, Songs of Distant Earth, and Fountains of Paradise. These works, and many books by Robert A. Heinlein were among the first science fiction books I read.

Clarke’s visions of the future were amazing, and I come back to his stories again and again. This is largely because they posited a future with possible things, like the geostationary satellites we now all take for granted for telecommunications and weather studies. And, Arthur wrote evocatively, something that (as a fellow writer) I can appreciate.

This re-fascination with his works presages news today from the the Associated Press, which reports that Sir Arthur Clarke has died at the age of 90. He had not been well for some years, but he kept on cranking out work. (His quite extensive biography on Wikipedia has already been updated with news of his death.)

I never had a chance to meet him personally, but we corresponded briefly back when I was an editor at Sky & Telescope. We adapted some of his work for a special edition of SkyWatch, and it was my pleasure to work with him on that project. I heard from him a few times after I left the magazine, but mostly kept tabs on his health and work through the Internet. When the tsunami hit Sri Lanka in 2006, he wrote a quick note to his wide circle of correspondents, reporting on conditions and letting people know he was all right.

It’s with great sadness I salute the passing of Sir Arthur C. Clarke. Here’s to ya, lad!