GSC 03089-00929

GSC 03089-00929 / Pipoltr

A light curve for V1434 Herculis, plotted from TESS data,[1] the 1.306 day interval between planet transits is shown in red.
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Hercules
Right ascension 17h 52m 07.0184s[2]
Declination +37° 32′ 46.237″[2]
Apparent magnitude (V) 12.4
Characteristics
Spectral type G
Apparent magnitude (B) 13.114 ±0.009[3]
Apparent magnitude (V) 12.402 ±0.006[3]
Apparent magnitude (I) 11.603000 ±0.010[3]
Apparent magnitude (J) 11.015 ±0.022[3]
Apparent magnitude (H) 10.655000 ±0.030[3]
Apparent magnitude (K) 10.608000 ±0.028[3]
Variable type planetary transits[3][4]
Astrometry
Proper motion (μ) RA: −24.462(10) mas/yr[2]
Dec.: 34.772(11) mas/yr[2]
Parallax (π)4.3106 ± 0.0091 mas[2]
Distance757 ± 2 ly
(232.0 ± 0.5 pc)
Absolute magnitude (MV)5.39±0.11[5]
Details
Mass0.928+0.028
−0.048[5] M☉
Radius0.826±0.012[6] R☉
Luminosity0.625+0.066
−0.058[5] L☉
Surface gravity (log g)4.57±0.01[6] cgs
Temperature5650±75[5] K
Metallicity [Fe/H]−0.19±0.08[5] dex
Rotational velocity (v sin i)1.5±1.0 km/s
Age0.9+2.8
−0.8[5] Gyr
Other designations
TrES-3 Parent Star, 1SWASP J175207.01+373246.3, UCAC2 45017453,[3] V1434 Her
Database references
SIMBADdata

GSC 03089-00929 is a magnitude 12 star located approximately 757 light-years away in the constellation of Hercules. This star is a G type main sequence star that is similar to but slightly cooler than the Sun.[3] This star is identified in SIMBAD as a variable star per the 1SWASP survey.[7]

The star GSC 03089-00929 is named Pipoltr. The name was selected in the NameExoWorlds campaign by Liechtenstein, during the 100th anniversary of the IAU. In the local dialect of Triesenberg, Pipoltr is a bright and visible butterfly.[8][9]

  1. ^ Cite error: The named reference MAST was invoked but never defined (see the help page).
  2. ^ a b c d Cite error: The named reference Gaia DR3 was invoked but never defined (see the help page).
  3. ^ a b c d e f g h i "NAME TrES-3 Parent Star". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2009-04-23.
  4. ^ Lister, T. A.; West, R. G.; Wilson, D. M.; Collier Cameron, A.; Clarkson, W. I.; Street, R. A.; Enoch, B.; Parley, N. R.; et al. (June 30, 2007). "SuperWASP-North extrasolar planet candidates: candidates from fields 17h<RA<18h" (PDF). Monthly Notices of the Royal Astronomical Society. 379 (2): 647–662. arXiv:0705.2603. Bibcode:2007MNRAS.379..647L. doi:10.1111/j.1365-2966.2007.11948.x. S2CID 14333676.
  5. ^ a b c d e f Cite error: The named reference Sozzetti2009 was invoked but never defined (see the help page).
  6. ^ a b Cite error: The named reference Püsküllü2017 was invoked but never defined (see the help page).
  7. ^ "Objects in reference 2007MNRAS.379..647L". Centre de Données astronomiques de Strasbourg. Retrieved 2009-05-03.
  8. ^ "Approved names". NameExoworlds. Archived from the original on 2019-12-19. Retrieved 2020-01-02.
  9. ^ "International Astronomical Union | IAU". www.iau.org. Retrieved 2020-01-02.