07/06/2005
A Huge Neighbor and a Small Planet
Astronomy and outer space offer no end of exciting events and discoveries these days. This week it was the remarkable success of Deep Impact, the probe that smashed into the comet Tempel 1 on July 4. This was one NASA mission that was flawless in its execution. The main objective of the mission was to expose the comet’s pristine composition, on the assumption that Tempel’s contents are the same materials that went into making up our solar system billions of years ago when it was being formed.
Coincidentally, I had planned to write this week about how solar systems are formed. However, with the possibility that some relevant results from Deep Impact might be available shortly, I’ll postpone that topic until next week. Besides, there’s other spectacular news on a new planet in another solar system and on the well-known Andromeda galaxy, which has suddenly become vastly larger than thought heretofore. Andromeda is the nearest major galaxy to our own Milky Way and is said to be visible to the naked eye as a fuzzy patch on a crystal clear night. (There are very few such nights in our area.) Andromeda is also the galaxy that’s headed our way in what should be a doozy of a deep impact!
Andromeda is a classic spiral galaxy and is usually the one shown in textbooks or encyclopedias. It’s a nice disc-shaped galaxy and its disc of stars and visible matter is roughly 100,000 light years (about 600,000,000,000,000,000 miles) in diameter. At least that was the general supposition until a meeting a few weeks ago of the American Astronomical Society in Minneapolis. An article on the meeting by Robert Irion in the June 17 issue of Science cites work reported by Nial Tanvir of the University of Hertfordshire in the UK and Rodrigo Ibata of the Strasbourg Observatory in France and their colleagues. They used the Isaac Newton Telescope on the Canary Islands to search the regions surrounding Andromeda’s main spiral disc. They were surprised to find swarms of faint stars in these outlying regions. These stars lie in what was considered to be a “halo” of stars from other disrupted galaxies that had their own deep impacts with the voracious Andromeda.
It was expected that these stars would be flitting about in a random manner and that they were not in the mainstream of the stars circling the core of Andromeda. However, when the Keck II telescope on Mauna Kea in Hawaii was brought into the picture by Scott Chapman and coworkers, they looked at about 5,000 stars and found that many revolved around smoothly as a huge extension of the disk we knew and loved. If you looked up in the sky with a telescope that could reveal these outer stars, you would see that Andromeda covers an amazing space equal to the width of a dozen full moons lined up in a row! Andromeda is three times bigger than we thought previously.
But wait, there may be more. Puragra Guhathakurta of Cal Tech and coworkers now claim to have found stars in Andromeda’s halo some 500,000 light years from its center. That would make Andromeda a million light years in diameter and its outer reaches would be a fifth of the distance to our Milky Way. That deep impact may come sooner than we thought!
Last week I noted that Jack Kilby received the Nobel Prize for his invention of the integrated circuit. I maintain that another invention, the CCD (charge-coupled device) invented by Willard Boyle and George Smith at Bell Labs, should be similarly acknowledged. Aside from its role in cameras, camcorders and the like, the CCD’s capability of detecting photons has opened up vast new worlds in astronomy, perhaps even the above Andromeda story. It certainly played a role in the recently headlined discovery of a new planet outside our solar system.
Finding these so-called extrasolar planets is by now old hat, with roughly 150 now on the books. We’ve talked before about how astronomers have detected these planets in most cases by looking at the “wobble” in a star’s light as the planet pushes and pulls the star slightly out of position as the planet orbits the star. A prime goal, of course, is to find another planet that resembles Earth sufficiently that it could harbor life. We’re getting closer.
About 8 years ago, Paul Butler of the Carnegie Institution in Washington, and Geoffrey Marcy of the University of California, Berkeley, were looking at a “wobbling” small star, Gliese 876, a red dwarf about a third the size of our Sun. In 1998, they reported finding a planet orbiting 876 that was about twice the size of Jupiter. They and their fellow researchers didn’t abandon 876 and in 2001 they found another planet about half the size of Jupiter.
As they gathered more data, the researchers found that the two planets were influencing each other’s motions such that they were in resonance. These two giant gas planets gravitational pulls on each other are akin to a dance, with the outer planet taking 60 days to orbit 876, the inner one just half as long, 30 days. If you’re a smart theorist, you can model the motion of a resonant duo and predict how the wobble of 876’s light should behave with time.
But there was a problem. When theorists Eugenio Rivera and Jack Lissauer plugged the numbers into their model for the two planets orbiting 876, there was a slight discrepancy that indicated a possible third planet. They needed more precise data. Last August, Steven Vogt, who designed the high resolution spectrometer used in the Keck telescope on Mauna Kea, worked with his Santa Cruz team to upgrade the spectrometer’s CCD detectors. Last month, the 876 team held a press conference at the National Science Foundation in Arlington, Virginia.
The upgraded CCD detectors provided the more precise data needed to confirm that there was indeed another planet. This planet is likely only 7 or 8 times the mass of Earth and about half the size of the smallest other extrasolar planet detected to date. Until now, the planets that have been detected outside our solar system have been large gaseous planets.
Unfortunately, the new small planet orbits very close to 876, only about two millions miles away and the temperature is probably 400 to 750 degrees Fahrenheit. At a minimum, it’s about the same temperature you’d set your oven to cook a tenderloin of beef. It’s a short year on the small planet – just a tad less than 2 full days! Not much time to adjust one’s wardrobe for the changing seasons! The composition of the planet is not pinned down with certainty but the researchers believe that it’s a rocky planet. However, there is a chance that it’s more like a smaller version of Neptune, with a thick atmosphere of hydrogen, water and other gases.
With the new upgraded CCD detectors, the hunt is on for planets around other red dwarfs such as Gliese 876. These red dwarfs put out less energy than our Sun and a small planet out far enough for a 10 or 20-day year might be cool enough for liquid water to exist. Maybe we’ll find a hospitable planet to colonize before Andromeda comes calling!
Allen F. Bortrum
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