37 Geminorum

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37 Geminorum
Observation data
Epoch J2000       Equinox J2000
Constellation Gemini
Right ascension 06h 55m 18.66636s [1]
Declination +25° 22′ 32.5036″ [1]
Apparent magnitude  (V)5.74 [2]
Characteristics
Evolutionary stage main sequence [1]
Spectral type G0 V [3]
U−B color index +0.01 [4]
B−V color index 0.573±0.010
Astrometry
Radial velocity (Rv)−14.94±0.15 [5] km/s
Proper motion (μ)RA: −37.595 [1] mas/yr
Dec.: +24.234 [1] mas/yr
Parallax (π)57.4559±0.0907  mas [1]
Distance 56.77 ± 0.09  ly
(17.40 ± 0.03  pc)
Absolute magnitude  (MV)4.56 [2]
Details
Mass 1.08 [6]   M☉
Radius 1.08 [6]   R☉
Luminosity 1.29 [6]   L☉
Surface gravity (log g)4.40 [6]   cgs
Temperature 5,913 [6]   K
Metallicity [Fe/H]−0.25 [7]   dex
Rotation 25.0 d [8]
Rotational velocity (v sin i)1.89 [9]  km/s
Age 5.49 [10]   Gyr
Other designations
BD+25°1496, GJ 252, HD 50692, HIP 33277, HR 2569, SAO 78866 [11]
Database references
SIMBAD data

37 Geminorum is a solitary [12] Sun-like star located at the northwest part of the northern constellation of Gemini, about three degrees to the east of the bright star Epsilon Geminorum. [13] The apparent visual magnitude of 37 Geminorum is 5.74, [2] which is just bright enough to be visible to the naked eye on a dark night. It is located at a distance of 57  light years from the Sun based on parallax. [1] This star is drifting closer with a radial velocity of −15 km/s, and is predicted to come as near as 13.8 light-years in approximately a million years. [5] It is positioned close enough to the ecliptic to be subject to lunar occultations, such as happened on April 8, 1984. [14]

Contents

Properties

The stellar classification of 37 Geminorum is G0 V, [3] which indicates it is an ordinary G-type main sequence star that is generating energy through core hydrogen fusion. In 2007, J. C. Hall and associates categorized it as a solar-type with a high mean activity level. [15] The star is around 5.5 [10]  billion years old and is spinning with a rotation period of 25 days. [8] It is slightly larger and more massive than the Sun, [6] with a lower abundance of heavier elements based on its abundance of iron. [7] 37 Geminorum is radiating 1.1 times the luminosity of the Sun from its photosphere at an effective temperature of 5,913  K . [6]

As of 2012, no extrasolar planets or debris disks have yet been discovered around it. [16] The center of the star's habitable zone lies at a distance of 1.32  AU . [17]

Teen Age Message

There was a METI message sent to 37 Geminorum. It was transmitted from Eurasia's largest radar, 70-meter Yevpatoria Planetary Radar. The message was named the Teen Age Message, it was sent on September 3, 2001, and it will arrive at 37 Geminorum in December 2057. [18]

Catalog of Nearby Habitable Systems

The Catalog of Nearby Habitable Systems (HabCat) is a list of approximately 17,000 relatively close stars similar to the sun and considered able to support a planet habitable by humans. 37 Geminorum is on the HabCat list. [19]

See also

References

  1. 1 2 3 4 5 6 7 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.
  2. 1 2 3 Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters. 38 (5): 331. arXiv: 1108.4971 . Bibcode:2012AstL...38..331A. doi:10.1134/S1063773712050015. S2CID   119257644.
  3. 1 2 Gray, R.O.; et al. (July 2006). "Contributions to the Nearby Stars (NStars) Project: spectroscopy of stars earlier than M0 within 40 pc-The Southern Sample". The Astronomical Journal . 132 (1): 161–170. arXiv: astro-ph/0603770 . Bibcode:2006AJ....132..161G. doi:10.1086/504637. S2CID   119476992.
  4. ↑ Mermilliod, J.-C. (1986). "Compilation of Eggen's UBV data, transformed to UBV (unpublished)". Catalogue of Eggen's UBV Data. SIMBAD. Bibcode:1986EgUBV........0M.
  5. 1 2 Bailer-Jones, C.A.L.; et al. (2018). "New stellar encounters discovered in the second Gaia data release". Astronomy & Astrophysics. 616: A37. arXiv: 1805.07581 . Bibcode:2018A&A...616A..37B. doi:10.1051/0004-6361/201833456. S2CID   56269929.
  6. 1 2 3 4 5 6 7 Stassun, Keivan G.; et al. (9 September 2019). "The Revised TESS Input Catalog and Candidate Target List". The Astronomical Journal. 158 (4): 138. arXiv: 1905.10694 . Bibcode:2019AJ....158..138S. doi: 10.3847/1538-3881/ab3467 . ISSN   0004-6256.
  7. 1 2 Holmberg, J.; et al. (2009). "The Geneva-Copenhagen survey of the solar neighbourhood. III. Improved distances, ages, and kinematics". Astronomy and Astrophysics . 501 (3): 941–947. arXiv: 0811.3982 . Bibcode:2009A&A...501..941H. doi:10.1051/0004-6361/200811191. S2CID   118577511. See Vizier catalogue V/130.
  8. 1 2 Judge, P. G.; et al. (March 2020). "Sun-like Stars Shed Light on Solar Climate Forcing". The Astrophysical Journal. 891 (1): 7. arXiv: 2002.04633 . Bibcode:2020ApJ...891...96J. doi: 10.3847/1538-4357/ab72a9 . S2CID   211082888. 96.
  9. ↑ Martínez-Arnáiz, R.; et al. (September 2010). "Chromospheric activity and rotation of FGK stars in the solar vicinity. An estimation of the radial velocity jitter" (PDF). Astronomy and Astrophysics. 520: A79. arXiv: 1002.4391 . Bibcode:2010A&A...520A..79M. doi:10.1051/0004-6361/200913725. S2CID   43455849. Archived from the original (PDF) on 2017-09-22. Retrieved 2018-11-04.
  10. 1 2 Vican, Laura (June 2012). "Age Determination for 346 Nearby Stars in the Herschel DEBRIS Survey". The Astronomical Journal. 143 (6): 135. arXiv: 1203.1966 . Bibcode:2012AJ....143..135V. doi:10.1088/0004-6256/143/6/135. S2CID   118539505.
  11. ↑ "* 37 Gem". SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2016-09-12.
  12. ↑ Fuhrmann, K.; et al. (February 2017). "Multiplicity among Solar-type Stars". The Astrophysical Journal. 836 (1): 23. Bibcode:2017ApJ...836..139F. doi: 10.3847/1538-4357/836/1/139 . 139.
  13. ↑ Sinnott, Roger W.; Perryman, Michael A. C. (1997). Millennium Star Atlas. Vol. 1. Sky Publishing Corporation and the European Space Agency. p. 154. ISBN   0-933346-84-0.
  14. ↑ Shaimukhametov, R. R.; Rizvanov, N. G. (September 1998). "Photoelectric Observations of Lunar Occultations at Engelhardt Astronomical Observatory". The Astronomical Journal. 116 (3): 1504–1507. Bibcode:1998AJ....116.1504S. doi: 10.1086/300482 .
  15. ↑ Hall, Jeffrey C.; et al. (March 2007). "The Activity and Variability of the Sun and Sun-like Stars. I. Synoptic Ca II H and K Observations". The Astronomical Journal. 133 (3): 862–881. Bibcode:2007AJ....133..862H. doi: 10.1086/510356 .
  16. ↑ Maldonado, J.; et al. (May 2012). "Metallicity of solar-type stars with debris discs and planets". Astronomy & Astrophysics. 541: A40. arXiv: 1202.5884 . Bibcode:2012A&A...541A..40M. doi:10.1051/0004-6361/201218800. S2CID   46328823.
  17. ↑ See, V.; et al. (October 2014). "The effects of stellar winds on the magnetospheres and potential habitability of exoplanets". Astronomy & Astrophysics. 570: 10. arXiv: 1409.1237 . Bibcode:2014A&A...570A..99S. doi:10.1051/0004-6361/201424323. S2CID   16146794. A99.
  18. ↑ Zaitsev, Alexander (2006). "Messaging to Extra-Terrestrial Intelligence". arXiv: physics/0610031 .
  19. ↑ Turnbull, Margaret C; Tarter, Jill C (2003). "Target Selection for SETI. I. A Catalog of Nearby Habitable Stellar Systems". The Astrophysical Journal Supplement Series. 145 (1): 181–198. arXiv: astro-ph/0210675 . Bibcode:2003ApJS..145..181T. doi:10.1086/345779. S2CID   14734094.
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