HD 215497

Coordinates: Sky map 22h 46m 36.7543s, −56° 35′ 58.322″
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HD 215497
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Tucana
Right ascension 22h 46m 36.7540s[1]
Declination −56° 35′ 58.3285″[1]
Apparent magnitude (V) 8.96[2]
Characteristics
Spectral type K3V[2]
Apparent magnitude (B) 9.92
Apparent magnitude (J) 7.339
Apparent magnitude (H) 6.917
Apparent magnitude (K) 6.784
B−V color index 0.95
Variable type none
Astrometry
Proper motion (μ) RA: −54.660±0.041[1] mas/yr
Dec.: −61.028±0.045[1] mas/yr
Parallax (π)24.6339 ± 0.0324 mas[1]
Distance132.4 ± 0.2 ly
(40.59 ± 0.05 pc)
Absolute magnitude (MV)5.77
Details
Mass0.872 ± 0.023[2] M
Radius1.01 ± 0.11 R
Luminosity0.39[2] L
Surface gravity (log g)4.31 ± 0.17[2] cgs
Temperature5113 ± 93[2] K
Metallicity0.23 ± 0.07[2]
Other designations
CPD−57°10139, HIP 112441, SAO 247578, TYC 8826-00247-1, 2MASS J22463675-5635584[3]
Database references
SIMBADdata
Exoplanet Archivedata

HD 215497 is a star located approximately 132 light-years away in the constellation of Tucana. It is a K3V star with the characteristics very similar to the Sun.

The survey in 2015 have ruled out the existence of any additional stellar companions at projected distances from 26 to 300 astronomical units.[4]

Planetary system

Announced in 2009, two extrasolar planets were discovered to be orbiting the star.[2] Both planets are less massive than Jupiter. The inner planet HD 215497 b orbits very close to the star and is termed a “hot super-Earth”. The outer planet HD 215497 c is Saturn-sized and orbits a little bit further from the star as the Earth, at around 1.282 AU.[2]

The HD 215497 planetary system[2]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b ≥6.6 M🜨 0.047 3.93404 ± 0.00066 0.16 ± 0.09
c ≥0.33 MJ 1.282 567.94 ± 2.70 0.49 ± 0.04

References

  1. ^ a b c d e Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
  2. ^ a b c d e f g h i j Lo Curto, G.; et al. (2010). "The HARPS search for southern extra-solar planets. XXII. Multiple planet systems from the HARPS volume limited sample". Astronomy and Astrophysics. 512. A48. arXiv:1411.7048. Bibcode:2010A&A...512A..48L. doi:10.1051/0004-6361/200913523.
  3. ^ "HD 215497". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-11-08.
  4. ^ Mugrauer, M.; Ginski, C. (12 May 2015). "High-contrast imaging search for stellar and substellar companions of exoplanet host stars". Monthly notices of the royal astronomical society. 450 (3). doi:10.1093/mnras/stv771. Retrieved 19 June 2020.