NASA's Tess satellite discovered a new world of life
The US Aeronautics and Space Agency (NASA) discovered another planet the size of a planet located in the "habitable zone" of its Transitional Planet Research Satellite (TESS).
According to the news on the "Space.com" website, TESS is about the same size as the Earth, in the constellation of Dolphins (Dorado), 101.5 light-years determined the existence of a planet.
NASA researchers, "TOI 700 d" called the other planet, its star, the Earth receives 86 percent of the energy received from the Sun, said it could allow living conditions.
Researchers stated that three other planets were discovered in orbit around the dwarf red star called "TESS Object of Interest 700". completed, the closest second star is 2.6 times the size of the Earth, the size of a mini-Neptune and completed the orbital tour in 16 days.
At the outermost, the TOI 700 d in the livable region is 20 percent larger than the Earth and completed the orbit tour in 37 days.
The researchers noted that the red dwarf star, which revolves around the TOI 700 d, is 40 percent larger and 50 percent warmer than the Sun, but does not show large flashes in the observations of the star, indicating that there is a relatively stable energy field that allows the planets to maintain their atmospheres steadily. he stressed.
The researchers underlined that the TOI 700 d was the first other planet to receive the same heat energy, close to Earth, discovered in the habitable zone of the star.
TESS's new findings were shared with researchers at the 235th annual meeting of the American Astronomical Society in Honolulu, Hawaii this week.
OTHER PLANET TALES
The TESS satellite, which includes 4 large cameras, each observing a quarter of the space gap in the direction it is looking for 27 days without interruption, is trying to detect the other planets in a so-called "transition".
Geçiş Transition anı refers to the moment when another planet passes the star in orbit.
Scientists are now able to determine the mass, core mass and atmospheric composition of the planets by measuring the amount of light emitted and absorbed by observing the reduction in the brightness of the star reflected in the cameras.
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