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XO-1

Coordinates:Sky map16h 02m 12s, +28° 10′ 11″
From Wikipedia, the free encyclopedia
Star in the constellation Corona Borealis
For the laptop with the same name, seeOLPC XO-1.
XO-1 / Moldoveanu

This artist's impression shows a dramatic close-up of the extrasolar planet XO-1b passing in front of a Sun-like star 600 light-years from Earth. The Jupiter-sized planet is in a tight four-day orbit around the star.
Credit:NASA, ESA and G. Bacon (STScI)
Observation data
Epoch J2000.0      Equinox J2000.0
ConstellationCorona Borealis[1]
Right ascension16h 02m 11.8462s[2]
Declination+28° 10′ 10.420″[2]
Apparent magnitude (V)11.19 ± 0.03[3]
Characteristics
Spectral typeG1V[3]
Apparent magnitude (B)11.85 ± 0.04[3]
Apparent magnitude (V)11.19 ± 0.03[3]
Apparent magnitude (J)9.939 ± 0.022[4]
Apparent magnitude (H)9.601 ± 0.017[4]
Apparent magnitude (K)9.527 ± 0.015[4]
Variable typePlanetary transit variable[3]
Astrometry
Radial velocity (Rv)2.49±0.32[2] km/s
Proper motion (μ)RA: −17.349(12)mas/yr[2]
Dec.: 14.780(15)mas/yr[2]
Parallax (π)6.1489±0.0136 mas[2]
Distance530 ± 1 ly
(162.6 ± 0.4 pc)
Absolute magnitude (MV)5.02+0.14
−0.16
[5]
Details
Mass1.027+0.057
−0.061
[5] M
Radius0.94 ± 0.02[6] R
Luminosity0.86+0.12
−0.10
[5] L
Surface gravity (log g)4.50 ± 0.01[7] cgs
Temperature5738 ± 65[7] K
Metallicity[Fe/H]−0.06 ± 0.07[7] dex
Rotational velocity (v sin i)1.1 ± 1.0[7] km/s
Age1.0+3.1
−0.9
[5] Gyr
Other designations
Moldoveanu,BD+28 2507,TOI-2021,TIC 236312126,TYC 2041-1657-1,GSC 02041-01657,2MASS J16021184+2810105[8]
Database references
SIMBADdata
Exoplanet Archivedata

XO-1 is amagnitude 11G-type main-sequence star located approximately 530light-years away[2] in theconstellationCorona Borealis. XO-1 has amass andradius similar to theSun.In 2006 theextrasolar planetXO-1b was discovered orbiting XO-1 by thetransit method using theXO Telescope.[3]

The star XO-1 is namedMoldoveanu. The name was selected in theNameExoWorlds campaign byRomania, during the 100th anniversary of theIAU.Moldoveanu is the highest peak in Romania.[9][10][11]

Planetary system

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TheXO Project is an international team of professional and amateurastronomers which discovered theJupiter-sized planet orbiting around XO-1. The team, led byPeter R. McCullough of the Space Telescope Science Institute in Baltimore, includes four amateur astronomers from North America and Europe. The planet was confirmed using theHarlan J. Smith Telescope andHobby-Eberly Telescope atMcDonald Observatory of theUniversity of Texas.[3] An independent confirmation of the planet was made by theWide Angle Search for Planets project.[12] In 2019, the planet was namedNegoiu, afterNegoiu Peak inRomania.

Further observations with theNICMOS instrument on board theHubble Space Telescope detected the presence of water vapor,methane, andcarbon dioxide in the atmosphere of XO-1b.[13] However an independent reinvestigation of the same data was unable to reproduce these results.[14]

The XO-1 planetary system[15][16]
Companion
(in order from star)
MassSemimajor axis
(AU)
Orbital period
(days)
EccentricityInclinationRadius
b / Negoiu0.907±0.022 MJ0.04914±0.000453.94150514(20)<0.01988.84±0.22°1.199±0.017 RJ

See also

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References

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  1. ^Roman, Nancy G. (1987)."Identification of a constellation from a position".Publications of the Astronomical Society of the Pacific.99 (617): 695.Bibcode:1987PASP...99..695R.doi:10.1086/132034. Constellation record for this object atVizieR.
  2. ^abcdefVallenari, 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 atVizieR.
  3. ^abcdefgMcCullough, P. R.; et al. (2006)."A Transiting Planet of a Sun-like Star".The Astrophysical Journal.648 (2):1228–1238.arXiv:astro-ph/0605414.Bibcode:2006ApJ...648.1228M.doi:10.1086/505651.S2CID 8100425.
  4. ^abcSkrutskie, Michael F.; et al. (1 February 2006)."The Two Micron All Sky Survey (2MASS)".The Astronomical Journal.131 (2):1163–1183.Bibcode:2006AJ....131.1163S.doi:10.1086/498708.ISSN 0004-6256.S2CID 18913331.Vizier catalog entry
  5. ^abcdTorres, Guillermo; et al. (2008)."Improved Parameters for Extrasolar Transiting Planets".The Astrophysical Journal.677 (2):1324–1342.arXiv:0801.1841.Bibcode:2008ApJ...677.1324T.doi:10.1086/529429.S2CID 12899134.
  6. ^Burke, Christopher J.; et al. (2010)."NICMOS Observations of the Transiting Hot Jupiter XO-1b".The Astrophysical Journal.719 (2):1796–1806.arXiv:1006.1953.Bibcode:2010ApJ...719.1796B.doi:10.1088/0004-637X/719/2/1796.S2CID 118798621.
  7. ^abcdTorres, Guillermo; et al. (2012)."Improved Spectroscopic Parameters for Transiting Planet Hosts".The Astrophysical Journal.757 (2). 161.arXiv:1208.1268.Bibcode:2012ApJ...757..161T.doi:10.1088/0004-637X/757/2/161.S2CID 16580774.
  8. ^"TYC 2041-1657-1".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2018-10-14.
  9. ^"Romania | NameExoworlds". Archived fromthe original on 2019-12-18.
  10. ^"Approved names".NameExoworlds. Retrieved2020-01-02.
  11. ^"International Astronomical Union | IAU".www.iau.org. Archived fromthe original on 2022-12-05. Retrieved2020-01-02.
  12. ^Wilson, D. M.; et al. (2006)."SuperWASP Observations of the Transiting Extrasolar Planet XO-1b".The Publications of the Astronomical Society of the Pacific.118 (847):1245–1251.arXiv:astro-ph/0607591.Bibcode:2006PASP..118.1245W.doi:10.1086/507957.S2CID 118916713.
  13. ^Tinetti, G.; et al. (2010)."Probing the Terminator Region Atmosphere of the Hot-Jupiter XO-1b with Transmission Spectroscopy".The Astrophysical Journal Letters.712 (2):L139 –L142.arXiv:1002.2434.Bibcode:2010ApJ...712L.139T.doi:10.1088/2041-8205/712/2/L139.S2CID 118588637.
  14. ^Gibson, N. P.; et al. (2011)."A new look at NICMOS transmission spectroscopy of HD 189733, GJ-436 and XO-1: no conclusive evidence for molecular features".Monthly Notices of the Royal Astronomical Society.411 (4):2199–2213.arXiv:1010.1753.Bibcode:2011MNRAS.411.2199G.doi:10.1111/j.1365-2966.2010.17837.x.S2CID 118506224.
  15. ^Bonomo, A. S.; et al. (2017)."The GAPS Programme with HARPS-N at TNG . XIV. Investigating giant planet migration history via improved eccentricity and mass determination for 231 transiting planets".Astronomy and Astrophysics.602 A107.arXiv:1704.00373.Bibcode:2017A&A...602A.107B.doi:10.1051/0004-6361/201629882.S2CID 118923163.
  16. ^Southworth, John; et al. (2018)."Physical properties and optical-infrared transmission spectrum of the giant planet XO-1 b".Monthly Notices of the Royal Astronomical Society.481 (3):4261–4276.arXiv:1809.03775.Bibcode:2018MNRAS.481.4261S.doi:10.1093/mnras/sty2488.S2CID 119503789.

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