Astronomy:Kepler-91b
| Discovery | |
|---|---|
| Discovery date | 2013 |
| Transit (Kepler Mission) | |
| Orbital characteristics | |
| 0.072+0.007 −0.002 AU | |
| Orbital period | 6.24658 d |
| Inclination | 68.5+1.6 −1 |
| Star | Kepler-91 |
| Physical characteristics | |
| Mean radius | 1.322+0.094 −0.086 |♃|J}}}}}} |
| Mass | 0.88+0.33 −0.17 |♃|J}}}}}} |
| Mean density | 0.44 g/cm3 (0.016 lb/cu in) |
| Albedo | 0.39 [1] |
| Physics | 2132 K |
Kepler-91b is a giant planet orbiting Kepler-91, a star slightly more massive than the Sun. Kepler-91 has left the main sequence and is now a red giant branch star.
Discovery and further confirmation
Kepler-91b was detected by analyzing the data of Kepler spacecraft where a transit-like signal was found. Initially thought to be a false positive due to light curve variations by a self-luminous object, it was later revealed that due to low density of Kepler-91's shape is distorted to slightly ellipsoidal shape due to gravitational effects of the planet. Ellipsoidal light variations caused by Kepler-91b constitute more than the third of light variations compared to transit depth. Ellipsoidal light variations also allowed to determine the planet's mass. It was also found that Kepler-91b reflects some of the starlight from its star.[2]
Further analysis managed to question the planetary nature of the object, suspecting that it is a self-luminous object.[3] However, the planetary nature was eventually confirmed again through both the radial velocity technique[4] and re-analysis of the light curve modulations.[5]
Characteristics
Kepler-91b is about 14% less massive than Jupiter while being more than 35% larger, making it less than half of the density of water. Kepler-91b orbits around the host star in about 6.25 days. Despite being one of the least edge-on orbits relative to Earth with inclination being about 68.5 degrees, transit was detected due to low semi-major axis to host star radius ratio.
Kepler-91b is expected to be engulfed by the parent star within about 55 million years.[2][1]
Possible trojan companion
The possibility of a trojan planet to Kepler-91b was suggested due to the presence of a small dim in the phase-folded light curve at phase 0.68.[2] This was subsequently studied but the conclusion was that the transit-signal was a false-positive.[6]
References
- ↑ 1.0 1.1 Esteves, Lisa J.; De Mooij, Ernst J. W.; Jayawardhana, Ray (2014). "Changing Phases of Alien Worlds: Probing Atmospheres of Kepler Planets with High-Precision Photometry". The Astrophysical Journal 804 (2): 150. doi:10.1088/0004-637X/804/2/150. Bibcode: 2015ApJ...804..150E.
- ↑ 2.0 2.1 2.2 Lillo-Box, J.; Barrado, D.; Moya, A.; Montesinos, B.; Montalbán, J.; Bayo, A.; Barbieri, M.; Régulo, C. et al. (2013). "Kepler-91b: A planet at the end of its life. Planet and giant host star properties via light-curve variations". Astronomy & Astrophysics 562: A109. doi:10.1051/0004-6361/201322001. Bibcode: 2014A&A...562A.109L.
- ↑ Sliski, David H.; Kipping, David M. (2014). "A High False Positive Rate for Kepler Planetary Candidates of Giant Stars using Asterodensity Profiling". The Astrophysical Journal 788 (2): 148. doi:10.1088/0004-637X/788/2/148. Bibcode: 2014ApJ...788..148S.
- ↑ Lillo-Box, J.; Barrado, D.; Henning, Th.; Mancini, L.; Ciceri, S.; Figueira, P.; Santos, N. C.; Aceituno, J. et al. (August 2014). "Radial velocity confirmation of Kepler-91 b" (in en). Astronomy & Astrophysics 568: L1. doi:10.1051/0004-6361/201424587. ISSN 0004-6361. https://www.aanda.org/articles/aa/abs/2014/08/aa24587-14/aa24587-14.html.
- ↑ Barclay, Thomas; Endl, Michael; Huber, Daniel; Foreman-Mackey, Daniel; Cochran, William D.; MacQueen, Phillip J.; Rowe, Jason F.; Quintana, Elisa V. (2015). "Radial Velocity Observations and Light Curve Noise Modeling Confirm that Kepler-91b is a Giant Planet Orbiting a Giant Star" (in en). The Astrophysical Journal 800 (1): 46. doi:10.1088/0004-637X/800/1/46. ISSN 0004-637X. Bibcode: 2015ApJ...800...46B. http://stacks.iop.org/0004-637X/800/i=1/a=46.
- ↑ Placek, Ben; Knuth, Kevin H.; Angerhausen, Daniel; Jenkins, Jon M. (2015). "Characterization of Kepler-91b and the Investigation of a Potential Trojan Companion Using EXONEST". The Astrophysical Journal 814 (2): 147. doi:10.1088/0004-637X/814/2/147. Bibcode: 2015ApJ...814..147P.
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