KELT-18b: Difference between revisions
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'''KELT-18b''' is a [[hot Jupiter]] orbiting a hot type F4V star. It is one of the most inflated planets known around a hot star.<ref name=discovery /> |
'''KELT-18b''' is a [[hot Jupiter]] orbiting a hot type F4V star. It is one of the most inflated planets known around a hot star.<ref name=discovery /> |
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No additional planets in the system was discovered as in 2020.<ref>{{citation|arxiv=2010.11977|title=Search for planets in hot Jupiter systems with multi-sector TESS photometry. I. No companions in planetary systems KELT-18, KELT-23, KELT-24, Qatar-8, WASP-62, WASP-100, WASP-119, and WASP-126|year=2020}}</ref> |
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== References == |
== References == |
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{{reflist}} |
{{reflist}} |
Revision as of 01:54, 26 October 2020
Discovery | |
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Discovery date | February 6, 2017 |
Transit | |
Orbital characteristics | |
0.0455 ± 0.00069 AU (6,807,000 ± 103,000 km)[1] | |
Eccentricity | 0[1] |
2.8717518 ± 2.8e-06[1] d | |
Inclination | 88.86+0.79 −1.2[1] |
Star | KELT-18 |
Physical characteristics | |
1.57+0.042 −0.035[1] RJ | |
Mass | 1.18 ± 0.18[1] MJ |
Mean density | 0.377 ± 0.040 g/cm3 (0.0136 ± 0.0014 lb/cu in)[2] |
Temperature | 2,120 K[1] |
KELT-18b is a hot Jupiter orbiting a hot type F4V star. It is one of the most inflated planets known around a hot star.[2]
No additional planets in the system was discovered as in 2020.[3]
References
- ^ a b c d e f g "Planet KELT-18 b". exoplanet.eu. Retrieved 2017-06-22.
- ^ a b KELT-18b: Puffy Planet, Hot Host, Probably Perturbed Kim K. McLeod 6 Feb 2017 doi:10.3847/1538-3881/aa6d5d arXiv:1702.01657
- ^ Search for planets in hot Jupiter systems with multi-sector TESS photometry. I. No companions in planetary systems KELT-18, KELT-23, KELT-24, Qatar-8, WASP-62, WASP-100, WASP-119, and WASP-126, 2020, arXiv:2010.11977