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'''30 Arietis''' (sometimes abbreviated '''30 Ari''') is a 6th-] ]<ref name="Clavin2015"/> in the ] ]. 30 Arietis A and B are separated by 38.1" or about 1500 ] at a distance of 130 ]s away. The main components of both systems are ]s, meaning they are ] ] in their cores.<ref name="Guenther2009"/> 30 Arietis A is itself a ] with an orbital period of 1.1 days.<ref>{{cite journal|title=A Search for Spectroscopic Binaries from Published Radial Velocity Data|author=Morbey, C. L. |
'''30 Arietis''' (sometimes abbreviated '''30 Ari''') is a 6th-] ]<ref name="Clavin2015"/> in the ] ]. 30 Arietis A and B are separated by 38.1" or about 1500 ] at a distance of 130 ]s away. The main components of both systems are ]s, meaning they are ] ] in their cores.<ref name="Guenther2009"/> 30 Arietis A is itself a ] with an orbital period of 1.1 days.<ref>{{cite journal|title=A Search for Spectroscopic Binaries from Published Radial Velocity Data|author=Morbey, C. L.|author2=Brosterhus, E. B.|journal=Publications of the Astronomical Society of the Pacific|volume=86|issue=512|pages=455|date=1974|doi=10.1086/129630|bibcode=1974PASP...86..455M}}</ref> The 30 Arietis system is 910 million years old, one fifth the age of the ]. | ||
==Planetary system== | ==Planetary system== | ||
On November 27, 2009, the discovery of a very massive planet was announced to be orbiting 30 Arietis B at a distance of about 1 AU.<ref name="Guenther2009"/> |
On November 27, 2009, the discovery of a very massive planet was announced to be orbiting 30 Arietis B at a distance of about 1 AU.<ref name="Guenther2009"/> | ||
{{OrbitboxPlanet begin | {{OrbitboxPlanet begin | ||
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{{Reflist|colwidth=30em|refs= | {{Reflist|colwidth=30em|refs= | ||
<ref name="Guenther2009">{{cite journal | title=A substellar component orbiting the F-star 30 Arietis B | url=http://www.aanda.org/articles/aa/full_html/2009/45/aa12112-09/aa12112-09.html | last1=Guenther | first1=E. W. | last2=Hartmann | first2=M. | last3=Esposito | first3=M. | last4=Hatzes | first4=A. P. | last5=Cusano | first5=F. | last6=Gandolfi | first6=D. | display-authors=1 | journal=Astronomy and Astrophysics | volume=507 | issue=3 | pages=1659–1665 | |
<ref name="Guenther2009">{{cite journal | title=A substellar component orbiting the F-star 30 Arietis B | url=http://www.aanda.org/articles/aa/full_html/2009/45/aa12112-09/aa12112-09.html | last1=Guenther | first1=E. W. | last2=Hartmann | first2=M. | last3=Esposito | first3=M. | last4=Hatzes | first4=A. P. | last5=Cusano | first5=F. | last6=Gandolfi | first6=D. | display-authors=1 | journal=Astronomy and Astrophysics | volume=507 | issue=3 | pages=1659–1665 | date=2009 | arxiv=0912.4619 | bibcode=2009A&A...507.1659G | doi=10.1051/0004-6361/200912112 }}</ref> | ||
<ref name="van Leeuwen2007">{{cite journal | title=Validation of the new Hipparcos reduction | url=http://www.aanda.org/index.php?option=com_article&access=bibcode&Itemid=129&bibcode=2007A%2526A...474..653VFUL | last1=van Leeuwen | first1=F. | journal=Astronomy and Astrophysics | volume=474 | issue=2 | pages=653–664 | |
<ref name="van Leeuwen2007">{{cite journal | title=Validation of the new Hipparcos reduction | url=http://www.aanda.org/index.php?option=com_article&access=bibcode&Itemid=129&bibcode=2007A%2526A...474..653VFUL | last1=van Leeuwen | first1=F. | journal=Astronomy and Astrophysics | volume=474 | issue=2 | pages=653–664 | date=2007 | arxiv=0708.1752 | bibcode=2007A&A...474..653V | doi=10.1051/0004-6361:20078357 }} </ref> | ||
<ref name="Schneider2011">{{cite web |url=http://exoplanet.eu/star.php?st=30+Ari |title=Notes for star 30 Ari B |author=Jean Schneider | |
<ref name="Schneider2011">{{cite web |url=http://exoplanet.eu/star.php?st=30+Ari |title=Notes for star 30 Ari B |author=Jean Schneider |date=2011 |publisher=] |accessdate=3 October 2011}}</ref> | ||
<ref name="Clavin2015">{{cite web |url=http://www.nasa.gov/jpl/planet-reared-by-four-parent-stars/index.html |title=Planet 'Reared' by Four Parent Stars | NASA |author=Whitney Clavin | |
<ref name="Clavin2015">{{cite web |url=http://www.nasa.gov/jpl/planet-reared-by-four-parent-stars/index.html |title=Planet 'Reared' by Four Parent Stars | NASA |author=Whitney Clavin |date=2015 |publisher=] |accessdate=4 March 2015}}</ref> | ||
}} | }} |
Revision as of 18:11, 4 June 2015
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Aries |
30 Arietis A | |
Right ascension | 02 37 00.52 |
Declination | +24° 38′ 50.0″ |
Apparent magnitude (V) | 6.48 |
30 Arietis B | |
Right ascension | 02 36 57.74 |
Declination | +24° 38′ 53.0″ |
Apparent magnitude (V) | 7.09 |
Astrometry | |
30 Arietis A | |
Radial velocity (Rv) | 14.9 km/s |
Proper motion (μ) | RA: 136.96 ± 0.60 mas/yr Dec.: –14.69 ± 0.43 mas/yr |
Parallax (π) | 23.95 ± 0.59 mas |
Distance | 136 ± 3 ly (42 ± 1 pc) |
Absolute magnitude (MV) | 3.46 |
30 Arietis B | |
Radial velocity (Rv) | 17.2 km/s |
Proper motion (μ) | RA: 150.75 ± 0.75 mas/yr Dec.: –12.79 ± 0.54 mas/yr |
Parallax (π) | 24.52 ± 0.68 mas |
Distance | 133 ± 4 ly (41 ± 1 pc) |
Absolute magnitude (MV) | 4.11 |
Characteristics | |
Spectral type | F5 V / F6 V |
U−B color index | 0.02 |
B−V color index | 0.410 / 0.510 |
Details | |
30 Arietis A | |
Mass | 1.31 ± 0.04 M☉ |
Radius | 1.37 ± 0.03 R☉ |
Luminosity | 3.6 L☉ |
Temperature | 6300 ± 100 K |
Age | (0.91 ± 0.03) × 10 years |
30 Arietis B | |
Mass | 1.16 ± 0.04 M☉ |
Radius | 1.13 ± 0.03 R☉ |
Luminosity | 1.964 L☉ |
Temperature | 6424 ± 180 K |
Metallicity | 0.07 ± 0.2 |
Age | (0.91 ± 0.03) × 10 years |
Other designations | |
CCDM 02370+2439, WDS 02370+2439 30 Arietis A BD+24°375, HD 16232, HIP 12184, HR 764, SAO 75470 | |
Database references | |
SIMBAD | data |
Exoplanet Archive | data |
Data sources: | |
Hipparcos Catalogue, CCDM (2002), Bright Star Catalogue (5th rev. ed.) |
30 Arietis (sometimes abbreviated 30 Ari) is a 6th-apparent-magnitude quadruple star in the constellation Aries. 30 Arietis A and B are separated by 38.1" or about 1500 AU at a distance of 130 light years away. The main components of both systems are F-type main-sequence stars, meaning they are fusing hydrogen in their cores. 30 Arietis A is itself a spectroscopic binary with an orbital period of 1.1 days. The 30 Arietis system is 910 million years old, one fifth the age of the Sun.
Planetary system
On November 27, 2009, the discovery of a very massive planet was announced to be orbiting 30 Arietis B at a distance of about 1 AU.
Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
b | ≥9.88 ± 0.94 MJ | 0.995 ± 0.012 | 335.1 ± 2.5 | 0.289 ± 0.092 | — | — |
See also
References
- ^ 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. Vizier catalog entry for A Vizier catalog entry for B
- ^ Guenther, E. W.; et al. (2009). "A substellar component orbiting the F-star 30 Arietis B". Astronomy and Astrophysics. 507 (3): 1659–1665. arXiv:0912.4619. Bibcode:2009A&A...507.1659G. doi:10.1051/0004-6361/200912112.
- Whitney Clavin (2015). "Planet 'Reared' by Four Parent Stars | NASA". NASA. Retrieved 4 March 2015.
- Morbey, C. L.; Brosterhus, E. B. (1974). "A Search for Spectroscopic Binaries from Published Radial Velocity Data". Publications of the Astronomical Society of the Pacific. 86 (512): 455. Bibcode:1974PASP...86..455M. doi:10.1086/129630.
- Jean Schneider (2011). "Notes for star 30 Ari B". Extrasolar Planets Encyclopaedia. Retrieved 3 October 2011.
External links
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