| Revision as of 18:12, 7 July 2022 editMammoth500 (talk | contribs)155 editsmNo edit summaryTags: Reverted Visual edit← Previous edit | Revision as of 00:19, 9 July 2022 edit undoGoingBatty (talk | contribs)Autopatrolled, Extended confirmed users, IP block exemptions, Pending changes reviewers, Rollbackers637,980 edits General fixes & manual cleanup, typo(s) fixed: February 23, 2020 → February 23, 2020,, turkish → Turkish, approximatley → approximately, Univeristy → UniversityTags: AWB RevertedNext edit → | ||
| Line 69: | Line 69: | ||
| {{Starbox end}} | {{Starbox end}} | ||
| '''XO-2''' is a Delta scuti type ]. 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 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-2 star was discovered by a team of |
'''XO-2''' is a Delta scuti type ]. 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 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-2 star was discovered by a team of Turkish ]s lead by Mustafa Turan Saglam on February 23, 2020, using the 0.4 meter ] of the ] in ].<ref>{{Cite web |last=Nowakowski |first=Tomasz |last2=Phys.org |title=Turkish astronomers discover new short-period pulsating variable star |url=https://phys.org/news/2022-07-turkish-astronomers-short-period-pulsating-variable.html |access-date=2022-07-07 |website=phys.org |language=en}}</ref> | ||
| ⚫ | The star ] period was mesuered to be P~0.95 hours with the star's mass being around 1.5 to 1.7 ]es. XO-2 effective temperature lies about 7,725 degrees ] (]) and a solar luminosities of 9.93. The absolute magnitude in V-band of approximately 2.76.<ref>{{Cite journal |last=Sağlam |first=Mustafa Turan |last2=Çördük |first2=Meryem |last3=Aliş |first3=Sinan |last4=Özgül |first4=Görkem |last5=Özgüllü |first5=Olcaytuğ |last6=Göktürk |first6=Fatih Erkam |last7=Gündüz |first7=Rahmi |last8=Fişek |first8=Süleyman |last9=Yelkenci |first9=F. Korhan |last10=Ülgen |first10=Eyüp Kaan |last11=Güver |first11=Tolga |date=2022-06-21 |title=Discovery of a Short Period Pulsator from Istanbul University Observatory |url=http://arxiv.org/abs/2206.14632 |journal=Turkish Journal of Astronomy and Astrophysics |doi=10.55064/tjaa.1103590 |issn=2757-7295}}</ref> | ||
| ⚫ | The star ] period was mesuered to be P~0.95 hours with the star's mass being around 1.5 to 1.7 ]. XO-2 effective temperature lies about 7,725 degrees ] (]) and a solar luminosities of 9.93. The absolute magnitude in V-band of |
||
| ==Planetary systems== | ==Planetary systems== | ||
| Line 116: | Line 115: | ||
| }} | }} | ||
| {{Orbitbox end}} | {{Orbitbox end}} | ||
| == See also == | == See also == | ||
| Line 164: | Line 162: | ||
| {{Stars of Lynx}} | {{Stars of Lynx}} | ||
| {{DEFAULTSORT:XO-2 (star)}} | |||
| ] | ] | ||
| ] | ] | ||
Revision as of 00:19, 9 July 2022
Star system in the constellation Lynx| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| 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 |
| Distance | 496 ± 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 |
| Distance | 505 ± 5 ly (155 ± 1 pc) |
| Details | |
| XO-2S | |
| Mass | 0.982 ± 0.034 M☉ |
| Radius | 1.02 R☉ |
| Temperature | 5399 ± 55 K |
| Metallicity | 0.39 ± 0.05 dex |
| Age | 7.1 ± −2.9 Gyr |
| XO-2N | |
| Mass | 0.971 ± 0.034 M☉ |
| Radius | 0.976 −0.016 R☉ |
| Temperature | 5340 ± 32 K |
| Metallicity | 0.44 ± 0.02 dex |
| Age | 6.3 ± 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 | |
| SIMBAD | XO-2S |
| XO-2N | |
XO-2 is a Delta scuti type 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. XO-2 star was discovered by a team of Turkish astronomers lead by Mustafa Turan Saglam on February 23, 2020, using the 0.4 meter Schmidit-Cassegrain telescope of the Istanbul University Observatory in Turkey.
The star pulsation period was mesuered to be P~0.95 hours with the star's mass being around 1.5 to 1.7 solar masses. XO-2 effective temperature lies about 7,725 degrees kelvin (K) and a solar luminosities of 9.93. The absolute magnitude in V-band of approximately 2.76.
Planetary systems
There are two known exoplanets orbiting XO-2N star. XO-2Nb (TYC 3413-210-1b and 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 and XO-2Nc was discovered in 2015 using the radial velocity method. The planets right ascension is 07 48 07 .479 with its declination of +50 13 03 .25.
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.
| 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 | — | — |
| 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 |
| c | 1.8 MJ | — | >6200 | — | — | — |
See also
References
- 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
- ^ 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.
- ^ 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. S2CID 13468914.
- ^ 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.
- ^ 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. S2CID 118567085.
- ^ 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. S2CID 7113991.
- ^ "TYC 3413-210-1". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2018-01-28.
- ^ "TYC 3413-5-1". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2018-01-28.
- Nowakowski, Tomasz; Phys.org. "Turkish astronomers discover new short-period pulsating variable star". phys.org. Retrieved 2022-07-07.
- Sağlam, Mustafa Turan; Çördük, Meryem; Aliş, Sinan; Özgül, Görkem; Özgüllü, Olcaytuğ; Göktürk, Fatih Erkam; Gündüz, Rahmi; Fişek, Süleyman; Yelkenci, F. Korhan; Ülgen, Eyüp Kaan; Güver, Tolga (2022-06-21). "Discovery of a Short Period Pulsator from Istanbul University Observatory". Turkish Journal of Astronomy and Astrophysics. doi:10.55064/tjaa.1103590. ISSN 2757-7295.
- Damasso, M.; et al. (2015). "A comprehensive analysis of the XO-2 stellar and planetary systems". Astronomy & Astrophysics. 575. A111. doi:10.1051/0004-6361/201425332.
- "XO-2c". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-06-09.
- "Open Exoplanet Catalogue - XO-2S b". www.openexoplanetcatalogue.com. Retrieved 2022-07-07.
- 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. S2CID 119269227.
- 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. S2CID 56545385.
External links
- NASA PlanetQuest: Planet race heats up: 1 month, 32 discoveries
- "XO-2". Exoplanets. Retrieved 2009-04-28.
