tech2 News StaffJan 08, 2020 09:22:46 IST
NASA’s planet-hunting space telescope, TESS, has found its first Earth-sized planet that is located in the habitable zone of its star. It has been named TOI 700 d and is relatively close to Earth — about 100 light-years away.
A habitable area of a star is the safe zone between a planet and its star; where it is not too far or too close to the star. The temperatures of the planet also allow for the presence of atmosphere and water.
TESS stands for Transiting Exoplanet Survey Satellite and NASA scientists confirmed the discovery using the Spitzer space telescope, which will be retiring at the end of this month.
“TESS was designed and launched specifically to find Earth-sized planets orbiting nearby stars,” said Paul Hertz, astrophysics division director at NASA Headquarters in Washington, in a statement. “Planets around nearby stars are easiest to follow-up with larger telescopes in space and on Earth. Discovering TOI 700 d is a key science finding for TESS. Confirming the planet’s size and habitable zone status with Spitzer is another win for Spitzer as it approaches the end of science operations this January."
The star — TOI 700
TESS had identified three planets, TOI 700 b, c and d that revolve around the star TOI 700 which is a small, cool M dwarf star in the southern constellation Dorado. It is around 40 percent of the Sun’s mass and size and about half its surface temperature.
According to ANI, the star was originally misclassified in the TESS database as being more similar to our Sun, which meant the planets appeared larger and hotter than they really are. Several researchers, including Alton Spencer, a high school student working with members of the TESS team, identified the error.
“When we corrected the star’s parameters, the sizes of its planets dropped, and we realized the outermost one was about the size of Earth and in the habitable zone,” said Emily Gilbert, a graduate student at the University of Chicago. The discovery was later confirmed by the Spitzer Space Telescope.
Gilbert and other researchers presented the findings at the 235th meeting of the American Astronomical Society in Honolulu, and three papers have been submitted to scientific journals.
TOI 700 b is the innermost planet, almost exactly the size of the Earth but it is probably rocky and completes an orbit every 10 days.
The middle planet, TOI 700 c, is 2.6 times larger than Earth — between the sizes of Earth and Neptune but completes its orbits once every 16 days. It is also most likely a gas-dominated world.
TOI 700 d, the outermost known planet in the system and the only one in the habitable zone, measures 20 percent larger than Earth, orbits every 37 days.
All of the planets are thought to be tidally locked to their star, which means they rotate once per orbit so that one side is constantly bathed in daylight, which is similar to our solar system.
Habitable conditions on TOI 700 d
While the exact conditions on TOI 700 d are unknown, scientists can use current information, like the planet's size and the type of star it orbits, to generate computer models and make predictions. Researchers at NASA's Goddard Space Flight Center in Greenbelt, Maryland, modelled 20 potential environments of TOI 700 d to gauge if any version would result in surface temperatures and pressures suitable for habitability.
Their 3D climate models examined a variety of surface types and atmospheric compositions typically associated with what scientists regard to be potentially habitable worlds. Since TOI 700 d is tidally locked to its star, the cloud formations of the planet and its wind patterns might be different from Earth's.
One simulation included an ocean-covered TOI 700 d with a dense, carbon-dioxide-dominated atmosphere similar to what scientists suspect surrounded Mars when it was young. The model atmosphere contains a deep layer of clouds on the star-facing side. Another model depicts TOI 700 d as a cloudless, all-land version of modern Earth, where winds flow away from the night side of the planet and converge on the point directly facing the star.
When the starlight passes through the atmosphere of a planet, it interacts with gaseous molecules like nitrogen and carbon dioxide and produces signals known as spectral lines. The researchers simulated spectra for the 20 modelled versions of TOI 700 d.
"Someday, when we have real spectra from TOI 700 d, we can backtrack, match them to the closest simulated spectrum, and then match that to a model. It's exciting because no matter what we find out about the planet, it's going to look completely different from what we have here on Earth," said Gabrielle Engelmann-Suissa.
With inputs from ANI
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