TOI-700 d
Goldilocks terrestrial planet orbiting TOI-700 From Wikipedia, the free encyclopedia
Goldilocks terrestrial planet orbiting TOI-700 From Wikipedia, the free encyclopedia
TOI-700 d is a near-Earth-sized exoplanet, likely rocky, orbiting within the habitable zone of the red dwarf TOI-700, the outermost planet within the system. It is located roughly 101.4 light-years (31.1 pc) away from Earth in the constellation of Dorado. The exoplanet is the first Earth-sized exoplanet in the habitable zone discovered by the Transiting Exoplanet Survey Satellite (TESS).[4][5][6]
An artist's depiction of TOI-700 d, depicted here as a possible ocean planet. The actual appearance of the planet is not currently known. | |
| Discovery[1] | |
|---|---|
| Discovered by | Emily Gilbert et al. |
| Discovery date | 3 January 2020 |
| Transit | |
| Orbital characteristics[2] | |
| 0.1633±0.0027 AU | |
| Eccentricity | 0.042+0.045 −0.030 |
| 37.42396+0.00039 −0.00035 d | |
| Inclination | 89.80°+0.12° −0.10° |
| 10°+120° −140° | |
| Star | TOI-700 |
| Physical characteristics | |
| 1.073+0.059 −0.054 R🜨[2] | |
| Mass | ≙1.72+1.29 −0.63 ME[1] |
| Temperature | Teq: 268.8 K (−4.3 °C; 24.2 °F)[3] |
TOI-700 d orbits its star at a distance of 0.163 AU (24,400,000 km; 15,200,000 mi) from its host star with an orbital period of roughly 37.4 days and has a radius of around 1.19 times that of Earth. It has been estimated that the planet receives about 86% the energy that the Earth receives from the Sun.[7]
It was discovered in early January 2020 by the Transiting Exoplanet Survey Satellite (TESS).
TOI-700 d is Earth-sized, an exoplanet that has a radius and mass similar to the Earth. It has a radius of about 1.07 R🜨; its mass has not been measured, but is predicted to be around 1.72 ME.[1] If it has an Earth-like atmosphere, then its average temperature would be about 268.8 K (−4.3 °C; 24.2 °F).[3] A small chance of a runaway greenhouse effect exists.[8]
TOI-700 is a red dwarf of spectral class M that is about 40% the mass and radius, and very roughly 50% of the temperature of the Sun.[6] The star is bright with low levels of stellar activity. Over the 11 sectors observed with TESS, the star does not show a single white-light flare. The low rotation rate is also an indicator of low stellar activity.[1]
TOI-700 d orbits its host star with an orbital period of 37.42 days. It has an orbital radius of about 0.163 AU (24.4 million km; 15.2 million mi), less than half of that of Mercury to the Sun in the Solar System. It receives about 86% of Earth's sunlight from its host star.
TOI-700 d orbits in the habitable zone of its host star. The solar wind ram pressure and intensity of the interplanetary magnetic field are expected to be similar to the Earth's, therefore retention of the planetary atmosphere is likely.[9][10]
TOI-700 d was discovered by a team of astronomers led by Emily Gilbert using the Transiting Exoplanet Survey Satellite (TESS) in early January 2020. This was the first Earth-sized exoplanet in the habitable zone discovered by TESS.[11]
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