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User:Mike s/draft2

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Mike s/draft2
Observation data
Epoch J2000      Equinox J2000
Constellation Leo[1]
Right ascension 11h 17m 47.7836s[2]
Declination 03° 51′ 59.006″[2]
Apparent magnitude (V) 10.165(46)<
Characteristics
Apparent magnitude (J) 10.034(22)[3]
Apparent magnitude (H) 9.549(22)[3]
Apparent magnitude (K) 9.454(25)[3]
Variable type Planetary transit[4]
Astrometry
Radial velocity (Rv)−8.92(6) km/s
Proper motion (μ) RA: −20.400(17) mas/yr[2]
Dec.: 26.329(17) mas/yr[2]
Parallax (π)9.16531±0.0172 mas[2]
Distance355.9 ± 0.7 ly
(109.1 ± 0.2 pc)
Details
Mass0.949+0.022
−0.019
 M
Radius1.335+0.025
−0.029
 R
Surface gravity (log g)4.23(2) cgs
Temperature5842(14) K
Metallicity [Fe/H]−0.19(1) dex
Rotational velocity (v sin i)2.31(53)[5] km/s
Age9.656(1.002) Gyr
Other designations
Gaia DR3 3811989156889528320, TYC 266-622-1, 2MASS J11174778+0351590[6]

K2-36

Stellar system

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Planetary system

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K2-36b

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Discovery

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[4]

Orbit

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Atmosphere

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The Mike s/draft2 planetary system[7]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b 3.9(1.1)[8] M🜨 0.02288(10) 1.422614(38) <0.093 84.45+0.78
−0.48
°
1.43(8)[8] R🜨
c 7.9(2.8) M🜨 0.05528(23) 5.340888(86) <0.089 86.917+0.066
−0.056
°
3.20(30) R🜨

References

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  1. ^ Roman, Nancy G. (1987). "Identification of a constellation from a position". Publications of the Astronomical Society of the Pacific. 99 (617): 695. Bibcode:1987PASP...99..695R. doi:10.1086/132034. Constellation record for this object at VizieR.
  2. ^ a b c d Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy and Astrophysics. 674: A1. arXiv:2208.00211. Bibcode:2023A&A...674A...1G. doi:10.1051/0004-6361/202243940. S2CID 244398875. Gaia DR3 record for this source at VizieR.
  3. ^ a b c Skrutskie, M. F.; et al. (2006). "The Two Micron All Sky Survey (2MASS)". The Astronomical Journal. 131 (2): 1163–1183. Bibcode:2006AJ....131.1163S. doi:10.1086/498708. Vizier catalog entry
  4. ^ a b Damasso, M.; et al. (2019). "So close, so different: characterization of the K2-36 planetary system with HARPS-N". Astronomy & Astrophysics. 624 A38. arXiv:1902.01881. Bibcode:2019A&A...624A..38D. doi:10.1051/0004-6361/201834671.
  5. ^ Rainer, M.; et al. (2023). "The GAPS programme at TNG: XLIV. Projected rotational velocities of 273 exoplanet-host stars observed with HARPS-N". Astronomy & Astrophysics. 676 A90. arXiv:2306.13468. Bibcode:2023A&A...676A..90R. doi:10.1051/0004-6361/202245564. Vizier catalog entry
  6. ^ "K2-36". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2025-06-04.
  7. ^ Bonomo, A. S.; et al. (2023). "Cold Jupiters and improved masses in 38 Kepler and K2 small planet systems from 3661 HARPS-N radial velocities: No excess of cold Jupiters in small planet systems". Astronomy & Astrophysics. 677 A33. arXiv:2304.05773. Bibcode:2023A&A...677A..33B. doi:10.1051/0004-6361/202346211.
  8. ^ a b Brinkman, Casey L.; et al. (2024-12-01). "Revisiting the Relationship Between Rocky Exoplanet and Stellar Compositions: Reduced Evidence for a Super-Mercury Population". The Astronomical Journal. 168 (6) 281. arXiv:2409.08361. Bibcode:2024AJ....168..281B. doi:10.3847/1538-3881/ad82eb.
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