| Discovery | |
|---|---|
| Discovered by | Aldo S. Bonomo et al. |
| Discovery date | 25 October 2011 |
| Transit method | |
| Orbital characteristics | |
| 0.0268 ± 0.0005 AU (4,009,000 ± 75,000 km) [1] | |
| 1.4857108 ± 0.0000002 [1] d | |
| Inclination | 87.22 ± 0.15 [1] |
| Star | Kepler-17 |
| Physical characteristics | |
| 1.33 ± 0.04 [1] RJ | |
| Mass | 2.47 ± 0.10 [1] MJ |
Mean
density | 1.30 ± 0.14 g/cm3 (0.0470 ± 0.0051 lb/cu in) [1] |
| 3.54 ± 0.03 m/s2 (11.614 ± 0.098 ft/s2) [1] | |
| Temperature | 2229+50 −58 K. [2] |
Kepler-17b is a planet in the orbit of star
Kepler-17, first observed by the
Kepler spacecraft observatory in 2011. Kepler-17b is a
gas giant nearly 2.45 times the mass of
Jupiter, and is sometimes described as a "
super-Jupiter".
The planet is likely to be tidally locked to the parent star. In 2015, the planetary nightside temperature was estimated to be equal to 2229+50
−58
K.
[2]
The study in 2012, utilizing a Rossiter–McLaughlin effect, have determined the planetary orbit is probably aligned with the equatorial plane of the star, misalignment equal to 0±15°. [3]
References
- ^ a b c d e f g Bonomo, A. S.; Hébrard, G.; Santerne, A.; Santos, N. C.; Deleuil, M.; Almenara, J.; Bouchy, F.; Díaz, R. F.; Moutou, C.; Vanhuysse, M. (2012). "SOPHIE velocimetry of Keplertransit candidates". Astronomy & Astrophysics. 538: A96. arXiv: 1110.5462. Bibcode: 2012A&A...538A..96B. doi: 10.1051/0004-6361/201118323. S2CID 118528032.
- ^ a b A Comprehensive Study of Kepler Phase Curves and Secondary Eclipses:Temperatures and Albedos of Confirmed Kepler Giant Planets
- ^ Albrecht, Simon; Winn, Joshua N.; Johnson, John A.; Howard, Andrew W.; Marcy, Geoffrey W.; Butler, R. Paul; Arriagada, Pamela; Crane, Jeffrey D.; Shectman, Stephen A.; Thompson, Ian B.; Hirano, Teruyuki; Bakos, Gaspar; Hartman, Joel D. (2012), "Obliquities of Hot Jupiter Host Stars: Evidence for Tidal Interactions and Primordial Misalignments", The Astrophysical Journal, 757 (1): 18, arXiv: 1206.6105, Bibcode: 2012ApJ...757...18A, doi: 10.1088/0004-637X/757/1/18, S2CID 17174530
 | This extrasolar-planet-related article is a stub. You can help Wikipedia by expanding it. |
| Discovery | |
|---|---|
| Discovered by | Aldo S. Bonomo et al. |
| Discovery date | 25 October 2011 |
| Transit method | |
| Orbital characteristics | |
| 0.0268 ± 0.0005 AU (4,009,000 ± 75,000 km) [1] | |
| 1.4857108 ± 0.0000002 [1] d | |
| Inclination | 87.22 ± 0.15 [1] |
| Star | Kepler-17 |
| Physical characteristics | |
| 1.33 ± 0.04 [1] RJ | |
| Mass | 2.47 ± 0.10 [1] MJ |
Mean
density | 1.30 ± 0.14 g/cm3 (0.0470 ± 0.0051 lb/cu in) [1] |
| 3.54 ± 0.03 m/s2 (11.614 ± 0.098 ft/s2) [1] | |
| Temperature | 2229+50 −58 K. [2] |
Kepler-17b is a planet in the orbit of star
Kepler-17, first observed by the
Kepler spacecraft observatory in 2011. Kepler-17b is a
gas giant nearly 2.45 times the mass of
Jupiter, and is sometimes described as a "
super-Jupiter".
The planet is likely to be tidally locked to the parent star. In 2015, the planetary nightside temperature was estimated to be equal to 2229+50
−58
K.
[2]
The study in 2012, utilizing a Rossiter–McLaughlin effect, have determined the planetary orbit is probably aligned with the equatorial plane of the star, misalignment equal to 0±15°. [3]
References
- ^ a b c d e f g Bonomo, A. S.; Hébrard, G.; Santerne, A.; Santos, N. C.; Deleuil, M.; Almenara, J.; Bouchy, F.; Díaz, R. F.; Moutou, C.; Vanhuysse, M. (2012). "SOPHIE velocimetry of Keplertransit candidates". Astronomy & Astrophysics. 538: A96. arXiv: 1110.5462. Bibcode: 2012A&A...538A..96B. doi: 10.1051/0004-6361/201118323. S2CID 118528032.
- ^ a b A Comprehensive Study of Kepler Phase Curves and Secondary Eclipses:Temperatures and Albedos of Confirmed Kepler Giant Planets
- ^ Albrecht, Simon; Winn, Joshua N.; Johnson, John A.; Howard, Andrew W.; Marcy, Geoffrey W.; Butler, R. Paul; Arriagada, Pamela; Crane, Jeffrey D.; Shectman, Stephen A.; Thompson, Ian B.; Hirano, Teruyuki; Bakos, Gaspar; Hartman, Joel D. (2012), "Obliquities of Hot Jupiter Host Stars: Evidence for Tidal Interactions and Primordial Misalignments", The Astrophysical Journal, 757 (1): 18, arXiv: 1206.6105, Bibcode: 2012ApJ...757...18A, doi: 10.1088/0004-637X/757/1/18, S2CID 17174530
|
| This extrasolar-planet-related article is a stub. You can help Wikipedia by expanding it. |