Jump to content

HAT-P-15

Coordinates: Sky map 04h 24m 59.5348s, +39° 27′ 38.3124″
From Wikipedia, the free encyclopedia

This is an old revision of this page, as edited by Supernova58 (talk | contribs) at 03:52, 3 August 2020 (Adding local short description: "Star in the constellation Perseus", overriding Wikidata description "star" (Shortdesc helper)). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.

HAT-P-15
Observation data
Epoch J2000      Equinox J2000
Constellation Perseus
Right ascension 04h 24m 59.5348s[1]
Declination +39° 27′ 38.3124″[1]
Apparent magnitude (V) 12.41
Characteristics
Spectral type G5V
Astrometry
Radial velocity (Rv)31.21 km/s
Proper motion (μ) RA: 14.403 mas/yr
Dec.: -9.377 mas/yr
Parallax (π)5.1664 ± 0.0544 mas[1]
Distance631 ± 7 ly
(194 ± 2 pc)
Details[2]
Mass1.013±0.043 M☉
Radius1.080±0.039 R☉
Luminosity1.00±0.11 L☉
Surface gravity (log g)4.38±0.03 cgs
Temperature5684±25 K
Metallicity0.272±0.031
Rotational velocity (v sin i)2.0±0.5 km/s
Age6.8+2.5
−1.6 Gyr
Other designations
Gaia DR2 179498266829041664, TYC 2883-1687-1, GSC 02883-01687, 2MASS J04245952+3927382[1]
Database references
SIMBADdata

HAT-P-15 is a G-type main-sequence star about 630 light-years away. The star is older than Sun yet has a concentration of heavy elements roughly 190% of solar abundance.[2] The star has no noticeable starspot activity.[3]

The spectroscopic survey in 2015 have failed to find any stellar companions to it,[4] yet imaging survey have identified a possibly two companion red dwarf stars at projected separations 1210 and 1370 AU, respectively.[5]

The star was named Berehynia in December 2019 by the Ukrainian amateur astronomers.[6]

Planetary system

In 2010 a transiting hot superjovian planet b (named Tryzub in 2019[6]) was detected. It has an equilibrium temperature of 904±20 K.[7] The orbital simulation shown the planets inward of orbit of b would in-spiral and be destroyed within time-span of less than billion years.[8]

Size comparison of HAT-P-15 b and Jupiter
The HAT-P-15 planetary system[7]
Companion
(in order from star) 		Mass Semimajor axis
(AU) 		Orbital period
(days) 		Eccentricity Inclination Radius
b 1.946±0.066 MJ 0.0964±0.0014 10.863502±0.000027 0.19±0.019 89.1±0.2° 1.072±0.043 RJ

References

  1. ^ a b c d HAT-P-15 -- Star
  2. ^ a b Do Metal-Rich Stars Make Metal-Rich Planets? New Insights on Giant Planet Formation from Host Star Abundances, 2019, arXiv:1912.00255
  3. ^ An Ultraviolet Investigation of Activity on Exoplanet Host Stars, 2013, arXiv:1301.6192
  4. ^ FRIENDS OF HOT JUPITERS III: AN INFRARED SPECTROSCOPIC SEARCH FOR LOW-MASS STELLAR COMPANIONS, 2015, arXiv:1510.08062
  5. ^ A Lucky Imaging search for stellar sources near 74 transit hosts, 2015, arXiv:1506.05456
  6. ^ a b "Украина выбрала имена для звезды и экзопланеты". LIGA.net. Retrieved 2019-12-18.
  7. ^ a b {{citation|arxiv=1005.5300|title=HAT-P-15b: A 10.9-DAY EXTRASOLAR PLANET TRANSITING A SOLAR-TYPE STAR|year=2010
  8. ^ Small Inner Companions of Warm Jupiters: Lifetimes and Legacies, 2014, arXiv:1401.7217


Stub icon

This main-sequence-star-related article is a stub. You can help Wikipedia by expanding it.

Stub icon

This extrasolar-planet-related article is a stub. You can help Wikipedia by expanding it.

Retrieved from "https://en.wikipedia.org/w/index.php?title=HAT-P-15&oldid=970915932"