Using data from NASA’s Spitzer Space Telescope, astronomers propose that helium atmospheres may be found on thousands of warm Neptune- and sub-Neptune-sized exoplanets in our galaxy.
They wouldn’t float like balloons or give you the chance to talk in high, squeaky voices, but planets with helium skies may constitute an exotic planetary class in our Milky Way galaxy. Researchers using data from NASA’s Spitzer Space Telescope propose that warm Neptune-size planets with clouds of helium may be strewn about the galaxy by the thousands.
“We don’t have any planets like this in our own solar system,” said Renyu Hu, NASA Hubble Fellow at the agency’s Jet Propulsion Laboratory in Pasadena, California, and lead author of a new study on the findings accepted for publication in the Astrophysical Journal. “But we think planets with helium atmospheres could be common around other stars.”
Prior to the study, astronomers had been investigating a surprising number of so-called warm Neptunes in our galaxy. NASA’s Kepler space telescope has found hundreds of candidate planets that fall into this category. They are the size of Neptune or smaller, with tight orbits that are closer to their stars than our own sizzling Mercury is to our sun. These planets reach temperatures of more than 1,340 degrees Fahrenheit (1,000 Kelvin), and orbit their stars in as little as one or two days.
In the new study, Hu and his team make the case that some warm Neptunes — and warm sub-Neptunes, which are smaller than Neptune — could have atmospheres enriched with helium. They say that the close proximity of these planets to their searing stars would cause the hydrogen in their atmospheres to boil off.
“Hydrogen is four times lighter than helium, so it would slowly disappear from the planets’ atmospheres, causing them to become more concentrated with helium over time,” said Hu. “The process would be gradual, taking up to 10 billion years to complete.” For reference, our planet Earth is about 4.5 billion years old.
Warm Neptunes are thought to have either rocky or liquid cores, surrounded by gas. If helium is indeed the dominant component in their atmospheres, the planets would appear white or gray. By contrast, the Neptune of our own solar system is a brilliant azure blue. The methane in its atmosphere absorbs the color red, giving Neptune its blue hue.
A lack of methane in one particular warm Neptune, called GJ 436b, is in fact what led Hu and his team to develop their helium planet theory. Spitzer had previously observed GJ 436b, located 33 light-years away, and found evidence for carbon but not methane. This was puzzling to scientists, because methane molecules are made of one carbon and four hydrogen atoms, and planets like this are expected to have a lot of hydrogen. Why wasn’t the hydrogen linking up with carbon to produce methane?
According to the new study, the hydrogen might have been slow-cooked off the planet by radiation from the host stars. With less hydrogen around, the carbon would pair up with oxygen to make carbon monoxide. In fact, Spitzer found evidence for a predominance of carbon monoxide in the atmosphere of GJ 436b.
The next step to test this theory is to look at other warm Neptunes for signs of carbon monoxide and carbon dioxide, which are indicators of helium atmospheres. The team says this might be possible with the help of NASA’s Hubble Space Telescope, and NASA’s upcoming James Webb Space Telescope may one day directly detect that helium.
Meanwhile, the wacky world of exoplanets continues to surprise astronomers.
“Any planet one can imagine probably exists, out there, somewhere, as long as it fits within the laws of physics and chemistry,” said co-author Sara Seager of the Massachusetts Institute of Technology in Cambridge and JPL. “Planets are so incredibly diverse in their masses, sizes, and orbits that we expect this to extend to exoplanet atmospheres.”
Reference: “Helium Atmospheres on Warm Neptune- and Sub-Neptune-Sized Exoplanets and Applications to GJ 436 b” by Renyu Hu, Sara Seager and Yuk L. Yung, 24 June 2015, The Astrophysical Journal.
DOI: 10.1088/0004-637X/807/1/8
A third author of the paper is Yuk Yung of the California Institute of Technology in Pasadena and JPL.
JPL manages the Spitzer Space Telescope mission for NASA’s Science Mission Directorate, Washington. Science operations are conducted at the Spitzer Science Center at the California Institute of Technology in Pasadena. Spacecraft operations are based at Lockheed Martin Space Systems Company, Littleton, Colorado. Data are archived at the Infrared Science Archive housed at the Infrared Processing and Analysis Center at Caltech. Caltech manages JPL for NASA.
Never miss a breakthrough: Join the SciTechDaily newsletter.
Follow us on Google and Google News.
2 Comments
All planets and dead stars will preferentially lose hydrogen leaving helium. In hundreds of trillions of years most of stars and planets will be helium. The hydrogen having been recycled by developing stars will use up the universe’s supply of hydrogen. The ratio of helium to hydrogen will grow and could be a way to measure the universe’s age.
Trillions of year? Might want to look up iron stars and maybe not put down blaringly obvious comments like you are some kind of astronomy wiz as anybody with a shred of sense that understands how stellar nuclear fusion works understands what you just wrote.