A “fingerprint” for Earth could help identify exoplanets capable of supporting life, researchers report.
The researchers used over a decade of observations of Earth’s atmosphere taken by the SCISAT satellite to construct a transit spectrum of Earth, a sort of fingerprint for Earth’s atmosphere in infrared light, which shows the presence of key molecules in the search for habitable worlds. This includes the simultaneous presence of ozone and methane, which scientists expect to see only when there is an organic source of these compounds on the planet. Such a detection is called a “biosignature.”
The findings could help scientists determine what kind of signal to look for in their quest to find Earth-like exoplanets (planets orbiting a star other than our Sun).
The Canadian Space Agency developed SCISAT to help scientists understand the depletion of Earth’s ozone layer by studying particles in the atmosphere as sunlight passes through it. In general, astronomers can tell what molecules are found in a planet’s atmosphere by looking at how starlight changes as it shines through the atmosphere. Instruments must wait for a planet to pass—or transit—over the star to make this observation.
With sensitive enough telescopes, astronomers could potentially identify molecules such as carbon dioxide, oxygen, or water vapor that might indicate if a planet is habitable or even inhabited.
“A handful of researchers have tried to simulate Earth’s transit spectrum, but this is the first empirical infrared transit spectrum of Earth,” says Nicolas Cowan, a professor at the McGill Space Institute at McGill University. “This is what alien astronomers would see if they observed a transit of Earth.”
Hunting for life on exoplanets
Cowan was explaining transit spectroscopy of exoplanets at a group lunch meeting when Yi Huang, an atmospheric scientist and fellow member of the McGill Space Institute, noted that the technique was similar to solar occultation studies of Earth’s atmosphere, as SCISAT does.
Since the first discovery of an exoplanet in the 1990s, astronomers have confirmed the existence of 4,000 exoplanets. The holy grail in this relatively new field of astronomy is to find planets that could potentially host life—an Earth 2.0.
A promising system that might hold such planets, called TRAPPIST-1, will be a target for the upcoming James Webb Space Telescope, set to launch in 2021. Evelyn Macdonald, a physics student, and Cowan built a simulated signal of what an Earth-like planet’s atmosphere would look like through the eyes of this future telescope which is a collaboration between NASA, the Canadian Space Agency, and the European Space Agency.
The TRAPPIST-1 system located 40 light years away contains seven planets, three or four of which are in the so-called “habitable zone” where liquid water could exist. The astronomers say this system might be a promising place to search for a signal similar to their Earth fingerprint since the planets are orbiting an M-dwarf star, a type of star which is smaller and colder than our Sun.
“TRAPPIST-1 is a nearby red dwarf star, which makes its planets excellent targets for transit spectroscopy. This is because the star is much smaller than the Sun, so its planets are relatively easy to observe,” explains Macdonald.
“Also, these planets orbit close to the star, so they transit every few days. Of course, even if one of the planets harbors life, we don’t expect its atmosphere to be identical to Earth’s since the star is so different from the Sun.”
According to their analysis, the researchers affirm that the Webb Telescope will be sensitive enough to detect carbon dioxide and water vapor using its instruments. It may even be able to detect the biosignature of methane and ozone if enough time is spent observing the target planet.
Cowan and his colleagues at the Montreal-based Institute for Research on Exoplanets are hoping to be some of the first to detect signs of life beyond our home planet. The fingerprint of Earth Macdonald assembled for her senior undergraduate thesis could tell other astronomers what to look for in this search.
The research appears in Monthly Notices of the Royal Astronomical Society.
Funding for the research came from the Natural Sciences and Engineering Research Council of Canada, the Fonds de recherche du Québec-Nature et technologies, and a McGill Science Undergraduate Research Award.
Source: McGill University