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Revision as of 12:42, 2 April 2018 editRathfelder (talk | contribs)Extended confirmed users548,588 edits Not a stub← Previous edit Revision as of 19:24, 14 October 2018 edit undoMike s (talk | contribs)Extended confirmed users21,551 edits update distance and replace refsNext edit →
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| constell = ]<ref name="Roman1987"/> | constell = ]<ref name="Roman1987"/>
| component1 = XO-2S | component1 = XO-2S
| ra1 = {{RA|07|48|07.4814}}<ref name="Gaia2016"/> | ra1 = {{RA|07|48|07.4814}}<ref name="Gaia DR2 XO-2S"/>
| dec1 = {{DEC|+50|13|03.254}}<ref name="Gaia2016"/> | dec1 = {{DEC|+50|13|03.2578}}<ref name="Gaia DR2 XO-2S"/>
| appmag_v1 = {{val|11.12|0.03}}<ref name="Burke2007"/> | appmag_v1 = {{val|11.12|0.03}}<ref name="Burke2007"/>
| component2 = XO-2N | component2 = XO-2N
| ra2 = {{RA|07|48|06.468}}<ref name="Høg2000"/> | ra2 = {{RA|07|48|06.4726}}<ref name="Gaia DR2 XO-2N"/>
| dec2 = {{DEC|+50|13|32.96}}<ref name="Høg2000"/> | dec2 = {{DEC|+50|13|32.9211}}<ref name="Gaia DR2 XO-2N"/>
| appmag_v2 = {{val|11.18|0.03}}<ref name="Burke2007"/> | appmag_v2 = {{val|11.18|0.03}}<ref name="Burke2007"/>
}} }}
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}} }}
{{Starbox astrometry {{Starbox astrometry
| component1 = XO-2S
| radial_v = | radial_v =
| prop_mo_ra = -34.7 ± 2.6<ref name="Høg2000" />
| prop_mo_dec = -153.6 ± 2.4<ref name="Høg2000" /> | prop_mo_ra = {{val|−29.317|0.063}}<ref name="Gaia DR2 XO-2S"/>
| prop_mo_dec = {{val|−154.398|0.044}}<ref name="Gaia DR2 XO-2S"/>
| parallax = 6.68
| p_error = 0.23 | parallax = 6.5765
| p_error = 0.0411
| parallax_footnote = <ref name="Gaia2016"/> | parallax_footnote = <ref name="Gaia DR2 XO-2S"/>
| absmag_v = | absmag_v =
| component2 = XO-2N
| radial_v2 =
| prop_mo_ra2 = {{val|−29.731|0.083}}<ref name="Gaia DR2 XO-2N"/>
| prop_mo_dec2 = {{val|−154.272|0.050}}<ref name="Gaia DR2 XO-2N"/>
| parallax2 = 6.4539
| p_error2 = 0.0603
| parallax_footnote2 = <ref name="Gaia DR2 XO-2N"/>
| absmag_v2 =
}} }}
{{Starbox detail {{Starbox detail
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'''XO-2''' Is a binary star. It consists of two components: '''XO-2S''' (Also known as '''XO-2A''') and '''XO-2N''' (Also known as '''XO-2B''').<ref name="Desidera2014" /> '''XO-2''' Is a binary star. It consists of two components: '''XO-2S''' (Also known as '''XO-2A''') and '''XO-2N''' (Also known as '''XO-2B''').<ref name="Desidera2014" />


This system is located approximately {{convert|150|pc|ly|disp=output number only}} ] away<ref name="Gaia2016"/> from ] in the ]. Both of these stars are slightly cooler than the Sun and are nearly identical to each other. The system has a ] of 11 and cannot be seen with the naked eye but is visible through a small ]. These stars are also notable for their large ]s.<ref name="Simbad XO-2S"/><ref name="Simbad XO-2N"/> This system is located approximately 500 ] away from ] in the ]. Both of these stars are slightly cooler than the Sun and are nearly identical to each other. The system has a ] of 11 and cannot be seen with the naked eye but is visible through a small ]. These stars are also notable for their large ]s.<ref name="Simbad XO-2S"/><ref name="Simbad XO-2N"/>


XO-2N and XO-2S have a separation of approximately {{formatnum:4600}} ].<ref name="Burke2007" /> XO-2N and XO-2S have a separation of approximately {{formatnum:4600}} ].<ref name="Burke2007" />
Line 119: Line 128:
<ref name="Fernandez2009">{{cite journal | title=The Transit Light Curve Project. XII. Six Transits of the Exoplanet XO-2b | url=http://iopscience.iop.org/article/10.1088/0004-6256/137/6/4911 | last1=Fernandez | first1=Jose M. | last2=Holman | first2=Matthew J. | last3=Winn | first3=Joshua N. | last4=Torres | first4=Guillermo | last5=Shporer | first5=Avi | last6=Mazeh | first6=Tsevi | last7=Esquerdo | first7=Gilbert A. | last8=Everett | first8=Mark E. | display-authors=1 | journal=The Astronomical Journal | volume=137 | issue=6 | pages=4911–4916 | year=2009 | arxiv=0903.2687 | bibcode=2009AJ....137.4911F | doi=10.1088/0004-6256/137/6/4911 }}</ref> <ref name="Fernandez2009">{{cite journal | title=The Transit Light Curve Project. XII. Six Transits of the Exoplanet XO-2b | url=http://iopscience.iop.org/article/10.1088/0004-6256/137/6/4911 | last1=Fernandez | first1=Jose M. | last2=Holman | first2=Matthew J. | last3=Winn | first3=Joshua N. | last4=Torres | first4=Guillermo | last5=Shporer | first5=Avi | last6=Mazeh | first6=Tsevi | last7=Esquerdo | first7=Gilbert A. | last8=Everett | first8=Mark E. | display-authors=1 | journal=The Astronomical Journal | volume=137 | issue=6 | pages=4911–4916 | year=2009 | arxiv=0903.2687 | bibcode=2009AJ....137.4911F | doi=10.1088/0004-6256/137/6/4911 }}</ref>


<ref name="Gaia DR2 XO-2S">{{cite DR2|934346740559239296}}</ref>
<ref name="Gaia2016">{{cite journal | title=Gaia Data Release 1. Summary of the astrometric, photometric, and survey properties | url=https://www.aanda.org/articles/aa/full_html/2016/11/aa29512-16/aa29512-16.html | journal=Astronomy and Astrophysics | volume=595 | at=A2 | year=2016 | last1=Brown | first1=A. G. A | last2=Vallenari | first2=A | last3=Prusti | first3=T | last4=De Bruijne | first4=J. H.J | last5=Mignard | first5=F | last6=Drimmel | first6=R | last7=Babusiaux | first7=C | last8=Bailer-Jones | first8=C. A.L | last9=Bastian | first9=U | last10=Biermann | first10=M | last11=Evans | first11=D. W | last12=Eyer | first12=L | last13=Jansen | first13=F | last14=Jordi | first14=C | last15=Katz | first15=D | last16=Klioner | first16=S. A | last17=Lammers | first17=U | last18=Lindegren | first18=L | last19=Luri | first19=X | last20=o'Mullane | first20=W | last21=Panem | first21=C | last22=Pourbaix | first22=D | last23=Randich | first23=S | last24=Sartoretti | first24=P | last25=Siddiqui | first25=H. I | last26=Soubiran | first26=C | last27=Valette | first27=V | last28=Van Leeuwen | first28=F | last29=Walton | first29=N. A | last30=Aerts | first30=C | display-authors=1 | arxiv=1609.04172 | bibcode=2016A&A...595A...2G | doi=10.1051/0004-6361/201629512 }}</ref>


<ref name="Gaia DR2 XO-2N">{{cite DR2|934346809278715776}}</ref>
<ref name="Høg2000">{{cite journal | url=http://articles.adsabs.harvard.edu/full/2000A%26A...355L..27H | title=The Tycho-2 catalogue of the 2.5 million brightest stars | last1=Høg | first1=E. | last2=Fabricius | first2=C. | last3=Makarov | first3=V. V. | last4=Urban | first4=S. | last5=Corbin | first5=T. | last6=Wycoff | first6=G. | last7=Bastian | first7=U. | last8=Schwekendiek | first8=P. | last9=Wicenec | first9=A. | display-authors=1 | journal=Astronomy and Astrophysics | volume=355 | pages=L27–L30 | date=2000 | bibcode=2000A&A...355L..27H | doi=10.1888/0333750888/2862 }} </ref>


<ref name="Narita2011">{{cite journal | title=XO-2b: a Prograde Planet with a Negligible Eccentricity and an Additional Radial Velocity Variation | url=https://academic.oup.com/pasj/article/63/6/L67/1455472 | last1=Narita | first1=Norio | last2=Hirano | first2=Teruyuki | last3=Sato | first3=Bun’ei | last4=Harakawa | first4=Hiroki | last5=Fukui | first5=Akihiko | last6=Aoki | first6=Wako | last7=Tamura | first7=Motohide | display-authors=1 | journal=Publications of the Astronomical Society of Japan | volume=63 | issue=6 | pages=L67–L71 | year=2011 | arxiv=1110.6136 | bibcode=2011PASJ...63L..67N | doi=10.1093/pasj/63.6.l67}}</ref> <ref name="Narita2011">{{cite journal | title=XO-2b: a Prograde Planet with a Negligible Eccentricity and an Additional Radial Velocity Variation | url=https://academic.oup.com/pasj/article/63/6/L67/1455472 | last1=Narita | first1=Norio | last2=Hirano | first2=Teruyuki | last3=Sato | first3=Bun’ei | last4=Harakawa | first4=Hiroki | last5=Fukui | first5=Akihiko | last6=Aoki | first6=Wako | last7=Tamura | first7=Motohide | display-authors=1 | journal=Publications of the Astronomical Society of Japan | volume=63 | issue=6 | pages=L67–L71 | year=2011 | arxiv=1110.6136 | bibcode=2011PASJ...63L..67N | doi=10.1093/pasj/63.6.l67}}</ref>

Revision as of 19:24, 14 October 2018

XO-2
Observation data
Epoch 2000      Equinox 2000
Constellation Lynx
XO-2S
Right ascension 07 48 07.4814
Declination +50° 13′ 03.2578″
Apparent magnitude (V) 11.12±0.03
XO-2N
Right ascension 07 48 06.4726
Declination +50° 13′ 32.9211″
Apparent magnitude (V) 11.18±0.03
Characteristics
Spectral type K0V + K0V
Astrometry
XO-2S
Proper motion (μ) RA: −29.317±0.063 mas/yr
Dec.: −154.398±0.044 mas/yr
Parallax (π)6.5765 ± 0.0411 mas
Distance496 ± 3 ly
(152.1 ± 1.0 pc)
XO-2N
Proper motion (μ) RA: −29.731±0.083 mas/yr
Dec.: −154.272±0.050 mas/yr
Parallax (π)6.4539 ± 0.0603 mas
Distance505 ± 5 ly
(155 ± 1 pc)
Details
XO-2S
Mass0.982 ± 0.034 M
Radius1.02 R
Temperature5399 ± 55  K
Metallicity 0.39 ± 0.05 dex
Age7.1 ±
−2.9 Gyr
XO-2N
Mass0.971 ± 0.034 M
Radius0.976
−0.016 R
Temperature5340 ± 32 K
Metallicity 0.44 ± 0.02 dex
Age6.3 ± 2.4 Gyr
Other designations
XO-2S: LSPM J0748+5013S, TYC 3413-210-1, GSC 03413-00210, 2MASS J07480748+5013032
XO-2N: LSPM J0748+5013N, TYC 3413-5-1, GSC 03413-00005, 2MASS J07480647+5013328
Database references
SIMBADXO-2S
XO-2N

XO-2 Is a binary star. It consists of two components: XO-2S (Also known as XO-2A) and XO-2N (Also known as XO-2B).

This system is located approximately 500 light-years away from Earth in the Lynx constellation. Both of these stars are slightly cooler than the Sun and are nearly identical to each other. The system has a magnitude of 11 and cannot be seen with the naked eye but is visible through a small telescope. These stars are also notable for their large proper motions.

XO-2N and XO-2S have a separation of approximately 4,600 AU.

Planetary systems

One known exoplanet, XO-2Nb (or rarely XO-2Bb), which is classified as a hot Jupiter, was discovered by the XO Telescope using the transit method orbiting XO-2N (XO-2B) in 2007.

Two planets were reported to orbit around XO-2S in 2014 using radial velocity method. One of them is Jupiter-mass and another has a mass comparable to Saturn.

Both stars also show RV-trends, which may indicate the presence of additional long-periodic jovians or brown dwarfs around each of them.

The XO-2S planetary system
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b ≥ 0.259 ± 0.014 MJ 0.1344 ±0.0025 18.157 ± 0.034 0.18 ± 0.035
c ≥ 1.37 ± 0.053 MJ 0.4756 ±0.0087 120.8 ± 0.034 0.1528 ± 0.01
The XO-2N planetary system
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b 0.62 ± 0.02 MJ 0.0369 ±0.002 2.61586178 ± 0.00000075 0.045 ± 0.024 88.7 ± 1.3° 0.973 ± 0.03 RJ

See also

References

  1. Roman, Nancy G. (1987). "Identification of a Constellation From a Position". Publications of the Astronomical Society of the Pacific. 99 (617): 695–699. Bibcode:1987PASP...99..695R. doi:10.1086/132034. Vizier query form
  2. ^ Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
  3. ^ Burke, Christopher J.; et al. (2007). "XO-2b: Transiting Hot Jupiter in a Metal-rich Common Proper Motion Binary". The Astrophysical Journal. 671 (2): 2115–2128. arXiv:0705.0003. Bibcode:2007ApJ...671.2115B. doi:10.1086/523087.
  4. ^ Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
  5. ^ Desidera, S.; et al. (2014). "The GAPS programme with HARPS-N at TNG. IV. A planetary system around XO-2S". Astronomy and Astrophysics. 567 (6). L6. arXiv:1407.0251. Bibcode:2014A&A...567L...6D. doi:10.1051/0004-6361/201424339.
  6. ^ Fernandez, Jose M.; et al. (2009). "The Transit Light Curve Project. XII. Six Transits of the Exoplanet XO-2b". The Astronomical Journal. 137 (6): 4911–4916. arXiv:0903.2687. Bibcode:2009AJ....137.4911F. doi:10.1088/0004-6256/137/6/4911.
  7. ^ "TYC 3413-210-1". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2018-01-28.
  8. ^ "TYC 3413-5-1". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2018-01-28.
  9. Narita, Norio; et al. (2011). "XO-2b: a Prograde Planet with a Negligible Eccentricity and an Additional Radial Velocity Variation". Publications of the Astronomical Society of Japan. 63 (6): L67 – L71. arXiv:1110.6136. Bibcode:2011PASJ...63L..67N. doi:10.1093/pasj/63.6.l67.
  10. Sing, D. K.; et al. (2011). "Gran Telescopio Canarias OSIRIS transiting exoplanet atmospheric survey: detection of potassium in XO-2b from narrowband spectrophotometry". Astronomy and Astrophysics. 527. A73. arXiv:1008.4795. Bibcode:2011A&A...527A..73S. doi:10.1051/0004-6361/201015579.

External links


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