HAT-P-36

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HAT-P-36 / Tuiren
Diagram showing star positions and boundaries of the Canes Venatici constellation and its surroundings
Location of HAT-P-36 (circled) within Canes Venatici
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Canes Venatici[1]
Right ascension 12h 33m 03.9061s[2]
Declination +44° 54′ 55.196″[2]
Apparent magnitude (V) 12.26
Characteristics
Spectral type G
Distance
958 ± 3 ly
(293.6 ± 0.9 pc)
Details
Gyr
TYC 3020-2221-1, 2MASS J12330390+4454552[3]
Database references
SIMBADdata

HAT-P-36, also referred to as Tuiren[4] is a 12th magnitude G-type main-sequence star estimated to be approximately 958 light-years away from Earth[2] in the constellation Canes Venatici. HAT-P-36 is too faint to be seen with the naked eye, but it is possible to view it with binoculars or a small telescope. In 2012 a hot Jupiter-type exoplanet was discovered orbiting HAT-P-36 with an orbital period of about 1.3 Earth days.[5] In December 2019, HAT-P-36 was named Tuiren and its planetary companion, HAT-P-36b, was named Bran as a result of Ireland's contribution to the 2019 NameExoWorlds campaign.[6] Bran has a mass approximately 1.8 times that of Jupiter and a radius 1.2 times larger.

Etymology

Tuiren (centre) as viewed in the Sloan Digital Sky Survey. The bright star to the top-left is TYC 3020-2195-1, an A-type main-sequence star approximately 3,156 light-years away.[7]

HAT-P-36 and its planet are named after characters from The Birth of Bran, a story in the book

hound by the fairy Uchtdealbh after Tuiren married her husband. Bran and Sceólan were the two puppies mothered by Tuiren while she was a dog. They were cousins of Fionn mac Cumhaill. The names were proposed by John Murphy, a teacher at Regina Mundi College, Cork.[8]

Planets

The HAT-P-36b planetary system[9]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b (Bran) ≥1.832±0.099 MJ 0.0238±0.0004 1.327347±0.000003 0.063±0.032 86±1.3° 1.264±0.071 RJ

HAT-P-36b (Bran) was discovered in 2012 by the

transit method.[5] A search for transit timing variation did not result in detection of additional planets in the system as at 2021.[10] Surprisingly, a planetary orbital period increase by 0.014 seconds per year was detected by 2021.[11]

Size comparison
Jupiter HAT-P-36b (Bran)
Jupiter Exoplanet

References

  1. ^ . Gaia DR3 record for this source at VizieR.
  2. ^ "HAT-P-36". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2023-02-23.
  3. ^ "IAU100 NameExoWorlds Approved Names" (PDF). NameExoWorlds. International Astronomical Union. Retrieved 24 July 2020.
  4. ^ a b "HAT-P-36". Open Exoplanet Catalogue. Retrieved 24 July 2020.
  5. ^ Smith, Niall (29 September 2019). "Sky Matters: Ireland has the chance to name a star and a planet - any ideas?". Irish Examiner. Retrieved 24 July 2020.
  6. ^ "TYC 3020-2195-1". Centre de Données astronomiques de Strasbourg. SIMBAD. Retrieved 24 July 2020.
  7. ^ Gorey, Colm (18 December 2019). "Cork teacher names exoplanet and star after Irish mythical dogs". Silicon Republic. Retrieved 24 July 2020.
  8. ^ "Planet HAT-P-36 b". Extrasolar Planets Encyclopaedia. Retrieved 24 July 2020.