Gliese 588: Difference between revisions

From Wikipedia, the free encyclopedia
Browse history interactively
← Previous editNext edit →
Content deleted Content added
VisualWikitext
Citation bot (talk | contribs)
Bots
4,924,811 edits
Alter: title. Add: pages, issue, volume, journal, doi, authors 1-8. Formatted dashes. | Use this bot. Report bugs. | Suggested by Abductive | Category:Durchmusterung objects | #UCB_Category 3004/3725
Burgasser, Adam J.
Line 78: Line 78:
<ref name="Thome1894">{{cite journal |last=Thome |first=J. M. |author-link=John M. Thome |title=Cordoba Durchmusterung declination -32 to -42. |year=1894 |journal=Resultados del Observatorio Nacional Argentino |volume=17 | pages=1–538 |bibcode=1894RNAO...17....1T}} [http://articles.adsabs.harvard.edu//full/1894RNAO...17....1T/0000491.000.html Page 468 (CD -40 9712)]; [http://articles.adsabs.harvard.edu//full/1894RNAO...17....1T/0000482.000.html page 459 (CD -40 7021)]</ref>
<ref name="Thome1894">{{cite journal |last=Thome |first=J. M. |author-link=John M. Thome |title=Cordoba Durchmusterung declination -32 to -42. |year=1894 |journal=Resultados del Observatorio Nacional Argentino |volume=17 | pages=1–538 |bibcode=1894RNAO...17....1T}} [http://articles.adsabs.harvard.edu//full/1894RNAO...17....1T/0000491.000.html Page 468 (CD -40 9712)]; [http://articles.adsabs.harvard.edu//full/1894RNAO...17....1T/0000482.000.html page 459 (CD -40 7021)]</ref>
<ref name="Porter1930">{{cite journal |last1=Porter |first1=J. G. |last2=Yowell |first2=E. J. |last3=Smith |first3=E. S. |title=A catalogue of 1474 stars with proper motion exceeding four-tenths year. |year=1930 |journal=Publications of the Cincinnati Observatory |volume=20 | pages=1–32 |bibcode=1930PCinO..20....1P}} [http://articles.adsabs.harvard.edu//full/1930PCinO..20....1P/0000022.000.html Page 21 (Ci 20 934).]</ref>
<ref name="Porter1930">{{cite journal |last1=Porter |first1=J. G. |last2=Yowell |first2=E. J. |last3=Smith |first3=E. S. |title=A catalogue of 1474 stars with proper motion exceeding four-tenths year. |year=1930 |journal=Publications of the Cincinnati Observatory |volume=20 | pages=1–32 |bibcode=1930PCinO..20....1P}} [http://articles.adsabs.harvard.edu//full/1930PCinO..20....1P/0000022.000.html Page 21 (Ci 20 934).]</ref>
<ref name="Kirkpatrick2012">{{cite journal | author-link=J. Davy Kirkpatrick | last1=Kirkpatrick | last2=Gelino |first1=J. D. | first2=C. R. | last3=Cushing | first3=M. C. | last4=Mace | first4=G. N. | last5=Griffith | first5=R. L. | last6=Skrutskie | first6=M. F. | last7=Marsh | first7=K. A. | last8=Wright | first8=E. L. | last9=Eisenhardt | first9=P. R. | last10=McLean | first10=I. S. | last11=Mainzer | first11=A. K. | last12=Burgasser | first12=A. J. | last13=Tinney | first13=C. G. | last14=Parker | first14=S. | last15=Salter | first15=G. | s2cid=119279752 | title=Further Defining Spectral Type "Y" and Exploring the Low-mass End of the Field Brown Dwarf Mass Function | year=2012 | journal=[[The Astrophysical Journal]] | volume=753 | issue=2 | pages=156 | arxiv=1205.2122 | doi=10.1088/0004-637X/753/2/156 | bibcode=2012ApJ...753..156K}}</ref>
<ref name="Kirkpatrick2012">{{cite journal | author-link=J. Davy Kirkpatrick | last1=Kirkpatrick | last2=Gelino |first1=J. D. | first2=C. R. | last3=Cushing | first3=M. C. | last4=Mace | first4=G. N. | last5=Griffith | first5=R. L. | last6=Skrutskie | first6=M. F. | last7=Marsh | first7=K. A. | last8=Wright | first8=E. L. | last9=Eisenhardt | first9=P. R. | last10=McLean | first10=I. S. | last11=Mainzer | first11=A. K. | last12=Burgasser | first12=Adam J. | last13=Tinney | first13=C. G. | last14=Parker | first14=S. | last15=Salter | first15=G. | s2cid=119279752 | title=Further Defining Spectral Type "Y" and Exploring the Low-mass End of the Field Brown Dwarf Mass Function | year=2012 | journal=[[The Astrophysical Journal]] | volume=753 | issue=2 | pages=156 | arxiv=1205.2122 | doi=10.1088/0004-637X/753/2/156 | bibcode=2012ApJ...753..156K}}</ref>


}}
}}

Revision as of 02:51, 7 August 2021

Gliese 588
Observation data
Epoch J2000      Equinox J2000
Constellation Lupus
Right ascension 15h 32m 12.93186s[1]
Declination −41° 16′ 32.1081″[1]
Apparent magnitude (V) 9.311
Characteristics
Spectral type M2.5V[2]
U−B color index +1.14[3]
B−V color index +1.51[3]
Astrometry
Radial velocity (Rv)15.50 km/s
Proper motion (μ) RA: -1176.447[4] mas/yr
Dec.: -1030.9703[4] mas/yr
Parallax (π)168.9965 ± 0.0270 mas[4]
Distance19.300 ± 0.003 ly
(5.9173 ± 0.0009 pc)
Absolute magnitude (MV)10.44[5]
Details[6]
Mass0.43±0.05 M☉
Radius0.42±0.03 R☉
Surface gravity (log g)4.82±0.08 cgs
Temperature3555±41 K
Metallicity [Fe/H]0.06±0.08 dex
Other designations
CD-40° 9712, GJ 588, HIP 76074, LHS 397, LTT 6210, TYC 7844-1976-1, 2MASS J15321302-4116314[2]
Database references
SIMBADdata

Gliese 588 is a nearby red dwarf star of spectral type M2.5, located in the constellation Lupus at 19.34 light-years from Earth.[1] It emits a very stable light flux, with no detectable pulsations.[6]

History of observations

According to Luyten's (1979) (catalogue LHS, as well as NLTT), this object was discovered by Innes.[7][8] In 1903–1927 Innes was the director of the Union Observatory (UO), South Africa.

However, in the Ci 20 catalogue (see number 934) this star was designated as "CD -40 7021", not "UO".[9] This may indicate that GJ 588 was first catalogued earlier, in the Cordoba Durchmusterung by John M. Thome in 1894.[10][11] Note: the real CD designation of Gliese 588 is "CD-40 9712",[12] not "CD -40 7021":[9] GJ 588 has a RA of 15 hours, but the real CD -40 7021 has a RA of 11 hours.[13][10]

Planetary system

On 11 June 2019 two planets were detected by radial velocity around Gliese 588 among other 118 planets around M dwarf stars.[14]

The Gliese 588 planetary system
Companion
(in order from star) 		Mass Semimajor axis
(AU) 		Orbital period
(days) 		Eccentricity Inclination Radius
b (unconfirmed) 2.4+1.0
−0.9 M🜨 		0.049±0.005 5.8084+0.0016
−0.0018 		0.04+0.25
−0.04 		— —
c (unconfirmed) 10.3+6.9
−4.9 M🜨 		0.530+0.048
−0.054 		206.0+2.0
−3.3 		0.06+0.02
−0.06 		— —

References

  1. ^ a b c van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics. 474 (2): 653–664. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357. S2CID 18759600. Vizier catalog entry
  2. ^ a b "GJ 588". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 25 December 2016.
  3. ^ a b Mermilliod, J.-C. (1986). "Compilation of Eggen's UBV data, transformed to UBV (unpublished)". Catalogue of Eggen's UBV Data. Bibcode:1986EgUBV........0M.
  4. ^ a b c Brown, A. G. A.; et al. (Gaia collaboration) (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics. 649: A1. arXiv:2012.01533. Bibcode:2021A&A...649A...1G. doi:10.1051/0004-6361/202039657. S2CID 227254300. (Erratum: doi:10.1051/0004-6361/202039657e). Gaia EDR3 record for this source at VizieR.
  5. ^ "The One Hundred Nearest Star Systems". 2012. Retrieved 25 December 2016.
  6. ^ a b Berdiñas, Z. M.; Rodríguez-López, C.; Amado, P. J.; Anglada-Escudé, G.; Barnes, J. R.; MacDonald, J.; Zechmeister, M.; Sarmiento, L. F. (2017), "High-cadence spectroscopy of M-dwarfs – II. Searching for stellar pulsations with HARPS", Monthly Notices of the Royal Astronomical Society, 469 (4): 4268–4282, arXiv:1705.04690, doi:10.1093/mnras/stx1140
  7. ^ Luyten, Willem Jacob (1979). "LHS 397". LHS Catalogue, 2nd Edition.
  8. ^ Kirkpatrick, J. D.; Gelino, C. R.; Cushing, M. C.; Mace, G. N.; Griffith, R. L.; Skrutskie, M. F.; Marsh, K. A.; Wright, E. L.; Eisenhardt, P. R.; McLean, I. S.; Mainzer, A. K.; Burgasser, Adam J.; Tinney, C. G.; Parker, S.; Salter, G. (2012). "Further Defining Spectral Type "Y" and Exploring the Low-mass End of the Field Brown Dwarf Mass Function". The Astrophysical Journal. 753 (2): 156. arXiv:1205.2122. Bibcode:2012ApJ...753..156K. doi:10.1088/0004-637X/753/2/156. S2CID 119279752.
  9. ^ a b Porter, J. G.; Yowell, E. J.; Smith, E. S. (1930). "A catalogue of 1474 stars with proper motion exceeding four-tenths year". Publications of the Cincinnati Observatory. 20: 1–32. Bibcode:1930PCinO..20....1P. Page 21 (Ci 20 934).
  10. ^ a b Thome, J. M. (1894). "Cordoba Durchmusterung declination -32 to -42". Resultados del Observatorio Nacional Argentino. 17: 1–538. Bibcode:1894RNAO...17....1T. Page 468 (CD -40 9712); page 459 (CD -40 7021)
  11. ^ Dictionary of Nomenclature of Celestial Objects. CD entry. SIMBAD. Centre de Données astronomiques de Strasbourg.
  12. ^ Luyten, Willem Jacob (1979). "NLTT 40449". NLTT Catalogue.
  13. ^ Thome, John Macon (1892–1932). "CD -40 7021". Cordoba Durchmusterung.
  14. ^ Barnes, J. R.; Kiraga, M.; Diaz, M.; Berdiñas, Z.; Jenkins, J. S.; Keiser, S.; Thompson, I.; Crane, J. D.; Shectman, S. A. (11 June 2019). "Frequency of planets orbiting M dwarfs in the Solar neighbourhood". arXiv:1906.04644v1 [astro-ph.EP].
Stub icon

This article about a red dwarf is a stub. You can help Wikipedia by expanding it.

Retrieved from "https://en.wikipedia.org/w/index.php?title=Gliese_588&oldid=1037519688"