A newly discovered planet 39 light-years away is being called the closest Earth-size exoplanet ever discovered — and a potential "Venus twin" — providing the mouth-watering opportunity for a close-up look at the environment on a rocky alien world.
One of the dire frustrations of studying planets around other stars (and, really, any astronomical object) is their distance from Earth, which makes it onerous or impossible to get many basic details about them. Exoplanets are doubly frustrating because any light they emit (light that would give hints about what's happening on the surface) is often overwhelmed by the light of the parent star.
But the new planet, called GJ 1132b, is only a cosmic stone's throw from Earth, orbiting a fairly dim star, and appears to be a rocky world with an atmosphere. And while its surface temperature indicates that it may have more in common with Venus than Earth, it is so perfectly primed for Earth-based studying, that astrophysicist Drake Deming hailed it as "arguably the most important planet ever found outside the solar system." [Watch: GJ 1132b - Closest Earth-size Alien Planet Explained]
Deming, a professor of astronomy at the University of Maryland, wrote about GJ 1132b in a "News & Views" article in the Nov. 12 issue of the journal Nature, noting that the "significance of this new world derives from several factors."
The first of those factors is its size — only 1.2 times the mass of Earth — and second is its proximity — only 39 light-years from our sun. These factors earned it the title "closest Earth-sized exoplanet yet discovered," by a statement from the Massachusetts Institute of Technology.
"Our galaxy spans about 100,000 light-years. So this is definitely a very nearby solar neighborhood star," Zachory Berta-Thompson, a postdoc in MIT's Kavli Institute for Astrophysics and Space Research and lead author of the paper announcing the discovery, said in the same statement.
Most of Earth-like or Earth-size planets known to science are hundreds or thousands of light-years away. Kepler-452b, discovered this past July and dubbed the most Earth-like planet found so far, is 1,400 light-years from Earth. Conversely, the recently discovered HD 219134b is only 21 light years from Earth, but is 4.5 times more massive as our home planet.
There's more that makes GJ 1132b prime for observations.
GJ 1132b was discovered using the MEarth-South telescope array, which consists of eight 40-centimeter telescopes located at the Cerro-Tololo Inter-America Observatory in Chile. The array hunts for exoplanets with the transit method (also used by the Kepler Space Telescope), which looks for regular "dips" in the amount of light coming from a star. The dips indicate that a planet is passing in front of the star.
It takes 1.6 days for GJ 1132b to make a single trip around Gliese 1132, its parent star (which means its orbit is smaller than Mercury's). This is a bonus for astronomers because it means the planet is frequently in view.
A Venus twin
And there's more: the transit method of exoplanet detection offers the possibility of studying the planet's atmosphere — if it contains oxygen and water, or even signs of life; the wind patterns; even the color of its sunsets, according to the statement from MIT. As the planet passes in front of the star, light passes through the planet's atmosphere, and picks up information about the chemistry therein.
Gliese 1132 is an M-dwarf star (also known as a red dwarf) only 21 percent the size of the sun, and emits only one-half a percent as much light. While the planet's size compared with its parent star makes it very non-Earth-like, this is also a significant advantage for observations because the light from the star doesn't completely overwhelm any reflected light that could be collected from the planet.
Despite this, GJ 1132b orbits very close to the star, receives significantly more radiation than Earth, and thus has a surface temperature much higher than Earth: 275 to 580 degrees Fahrenheit (135 to 304 Celsius), which would make it similar to Venus.
"Our ultimate goal is to find a twin Earth, but along the way we’ve found a twin Venus," said astronomer David Charbonneau of the Harvard-Smithsonian Center for Astrophysics (CfA), in a statement. "We suspect it will have a Venus-like atmosphere too, and if it does we can’t wait to get a whiff."
While this is too high for life (as we know it) to survive, it is cool enough to potentially maintain an atmosphere. According to the statement from CfA, CJ 1132b is "significantly cooler than any other exoplanet confirmed to be rocky. In comparison, well-known worlds such as CoRoT-7b and Kepler-10b possess scorching temperatures of 2,000 degrees Fahrenheit or more." At those temperatures, atmospheres similar to the one on Earth or Venus rarely survive. [10 Exoplanets That Could Host Alien Life]
"If we find this pretty hot planet has managed to hang onto its atmosphere over the billions of years it’s been around, that bodes well for the long-term goal of studying cooler planets that could have life," Berta-Thompson said. "We finally have a target to point our telescopes at, and [can] dig much deeper into the workings of a rocky exoplanet, and what makes it tick."
In the search for life elsewhere in the universe, some scientists think the community should target Earth-size planets around M-dwarfs because it is relatively easy to study their atmospheres, and because they may be fairly common in the galaxy. Perhaps, among this population of planets, scientists will find an alien world with the right setup to support life. GJ 1132b could be an important step toward that discovery.
"But even if life is abundant in the cosmos, finding unambiguous spectroscopic evidence of it is a daunting task that lies in the indefinite future," Deming wrote. "Observations of small stars, such as Gliese 1132, loom large in this task."
An in-depth study of GJ 1132b could be conducted by the Hubble Space Telescope, or better yet, the James Webb Space Telescope, scheduled to launch in 2018. Berta-Thompson said he thinks GJ 1132b is "going to be a favorite target of astronomers for years to come."
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Calla Cofield joined Space.com's crew in October 2014. She enjoys writing about black holes, exploding stars, ripples in space-time, science in comic books, and all the mysteries of the cosmos. Prior to joining Space.com Calla worked as a freelance writer, with her work appearing in APS News, Symmetry magazine, Scientific American, Nature News, Physics World, and others. From 2010 to 2014 she was a producer for The Physics Central Podcast. Previously, Calla worked at the American Museum of Natural History in New York City (hands down the best office building ever) and SLAC National Accelerator Laboratory in California. Calla studied physics at the University of Massachusetts, Amherst and is originally from Sandy, Utah. In 2018, Calla left Space.com to join NASA's Jet Propulsion Laboratory media team where she oversees astronomy, physics, exoplanets and the Cold Atom Lab mission. She has been underground at three of the largest particle accelerators in the world and would really like to know what the heck dark matter is. Contact Calla via: E-Mail – Twitter