K2-155d
| Discovery | |
|---|---|
| Discovered by | Teruyuki Hirano et al. [1] |
| Discovery site | Tokyo Institute of Technology |
| Discovery date | March 2018 |
| Transit method | |
| Designations | |
| LP 415-17 c, EPIC 210897587 c[2] | |
| Orbital characteristics | |
| 0.1886 (± 0.0066)[3] AU | |
| Eccentricity | unknown |
| 40.6835 (± 0.0031)[3] d | |
| Inclination | unknown |
| Star | K2-155 |
| Physical characteristics | |
| 1.64 +0.18 −0.17[3] R🜨 | |
Mean density | 5.41±1.11 g/cm3 |
| Temperature | 289 K (16 °C; 61 °F)[4] |
K2-155d is a potentially habitable Super-Earth exoplanet in the K2-155 system.[5] It is the outermost of three known planets orbiting around the K-type star K2-155 in the constellation Taurus.[6] It is one of 15 new exoplanets around red dwarf stars discovered by Japanese astronomer Teruyuki Hirano of the Tokyo Institute of Technology and his team.[1] The team used data from NASA's Kepler Space Telescope during its extended K2 "Second Light" mission. K2-155d orbits near the so-called habitable zone of its system, and has the potential to host liquid water.[7][5]
Discovery and observations
[edit]K2-155d is one of 15 exoplanets discovered by a team of Japanese astronomers led by Teruyuki Hirano at the Tokyo Institute of Technology.[5] Its discovery is based on data from the K2 mission of NASA's Kepler spacecraft.[5] The exoplanet has also been observed from ground-based telescopes including the Nordic Optical Telescope (NOT) in La Palma and the Subaru Telescope in Hawaii.[5] Its characteristics were confirmed using speckle imaging and high-dispersion optical spectroscopy.[3] The mass of K2-155d and the brightness of its host star may be measured by future observations from the W. M. Keck Observatory and the James Webb Space Telescope.[3] The brightness of its host star makes K2-155d a good target for future studies using instruments such as the James Webb Space Telescope.[3]
Characteristics
[edit]K2-155d is a super-Earth exoplanet with a radius 1.64 times that of Earth, near the transition zone between small rock-based and larger gaseous planets.[8][3][7] Climate models predict that it is located near its star's habitable zone and has an insolation 1.67 ± 0.38 (between 1.29 and 2.05) times that of Earth.[3] Its physical temperature is estimated to be 289 K (16 degrees Celsius or 61 degrees Fahrenheit).[4] Studies have shown that the planet would maintain a moderate surface temperature if its insolation is smaller than ~1.5 times that of Earth.[3]
K2-155d is one of three known planets in the system orbiting K2-155, a red dwarf star located 62.3 parsecs (203 ly) from Earth.[3] Its parent star has 88% less volume than the Sun.[9] K2-155d orbits its star with a 40.7 day period, but as the planet is tidally locked the same side always faces its sun.[5] K2-155d has an orbital radius of 0.1886 AU[8] and studies suggest that the planet has a low orbital eccentricity.[10]
Potential habitability
[edit]K2-155d has been labeled a potentially habitable planet that may be able to harbor liquid water.[7][5] A three-dimensional climate simulation was used to confirm the possibility of the existence of water.[5] However, its discoverer Teruyuki Hirano was cautious about the findings, stating that they do not guarantee K2-155d is habitable, as the ranges in its orbit and temperature allow the possibility of it being outside the habitable zone.[7] Factors such as the absence of solar flares could also decide if K2-155d is habitable.[5]
References
[edit]- ^ a b "15 new planets confirmed around cool dwarf stars". Tokyo Tech News. March 12, 2018.
- ^ "The Extrasolar Planet Encyclopaedia — K2-155 d". Extrasolar Planets Encyclopaedia. Retrieved 2024-04-29.
- ^ a b c d e f g h i j Hirano, Teruyuki; et al. (March 2018). "K2-155: A Bright Metal-poor M Dwarf with Three Transiting Super-Earths". The Astronomical Journal. 155 (3): 11. arXiv:1801.06957. Bibcode:2018AJ....155..124H. doi:10.3847/1538-3881/aaaa6e. S2CID 73590567. 124.
- ^ a b "HEC: Exoplanets Calculator (K2-155d)". Planetary Habibility Laboratory. Archived from the original on 2017-08-24. Retrieved 2018-03-30.
- ^ a b c d e f g h i Mack, Eric (March 13, 2018). "A super-Earth around a red star could be wet and wild". CNET.
- ^ "K2-155 PLANET HOST OVERVIEW PAGE". NASA Exoplanet Archive.
- ^ a b c d Dovey, Dana (March 14, 2018). "Super Earth 200 Light-Years Away May Hold Ideal Temperatures For Liquid Water And Life". Newsweek.
- ^ a b "Confirmed Planet Overview Page: K2-155d". NASA Exoplanet Archive. 2018.
- ^ "K2-155d". Exoplanet Data Explorer. 2018. Archived from the original on 2018-03-22. Retrieved 2018-03-21.
- ^ Eylen, Vincent; Albrecht, Simon (May 11, 2015). "Eccentricity from transit photometry: small planets in Kepler multi-planet systems have low eccentricities". The Astrophysical Journal. 808 (2): 126. arXiv:1505.02814. Bibcode:2015ApJ...808..126V. doi:10.1088/0004-637X/808/2/126. S2CID 14405731.
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