30 Arietis: Difference between revisions

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	'''30 Arietis''' (abbreviated '''30 Ari''') is a 6th-] ]<ref name="Clavin2015"/> in the ] of ]. ''30 Arietis'' is 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 both binaries with a composite spectra belonging to ]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\|jstor=40675565\|doi-access=free}}</ref> The 30 Arietis system is 910 million years old, one fifth the age of the ].		'''30 Arietis''' (abbreviated '''30 Ari''') is a 6th-] ]<ref name="Clavin2015"/> in the ] of ]. ''30 Arietis'' is 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 both binaries with a composite spectra belonging to ]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\|jstor=40675565\|doi-access=free}}</ref> The 30 Arietis system is 910 million years old, one fifth the age of the ].

	==Planetary system==		==Planetary system==

Revision as of 18:46, 29 December 2020

30 Arietis
Observation data Epoch J2000 Equinox J2000

Constellation	Aries
30 Arietis A
Right ascension	02 37 00.5235
Declination	+24° 38′ 49.9880″
30 Arietis B
Right ascension	02 36 57.7449
Declination	+24° 38′ 53.0026″
Astrometry
30 Arietis A
Proper motion (μ)	RA: 136.862±0.137 mas/yr Dec.: −15.188±0.141 mas/yr
Parallax (π)	22.1261 ± 0.0726 mas
Distance	147.4 ± 0.5 ly (45.2 ± 0.1 pc)
30 Arietis B
Proper motion (μ)	RA: 141.411±0.083 mas/yr Dec.: −10.677±0.086 mas/yr
Parallax (π)	22.3641 ± 0.0516 mas
Distance	145.8 ± 0.3 ly (44.7 ± 0.1 pc)
Orbit
Primary	30 Arietis A
Companion	30 Arietis BC
Period (P)	34000 yr
Semi-major axis (a)	40" (1670 AU)
Orbit
Primary	30 Arietis B
Companion	30 Arietis C
Period (P)	80 yr
Semi-major axis (a)	22.3 AU
Characteristics
Spectral type	F5 V / F6 V
B−V color index	0.410 / 0.510
Details
30 Arietis A
Mass	1.31 ± 0.04 `M`_☉
Radius	1.37 ± 0.03 `R`_☉
30 Arietis B
Mass	1.16 ± 0.04 `M`_☉
Radius	1.13 ± 0.03 `R`_☉
Other designations
CCDM 02370+2439, WDS 02370+2439 30 Arietis A BD+24°376, HD 16246, HIP 12189, HR 765, SAO 75471 30 Arietis B 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 (abbreviated 30 Ari) is a 6th-apparent-magnitude quadruple star in the constellation of Aries. 30 Arietis is the Flamsteed designation. 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 both binaries with a composite spectra belonging to 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. In 2020, after the inclination of the planetary orbit was measured, the "planet" was found to fall in the mass range of the red dwarf star.

The 30 Arietis B planetary system
Companion (in order from star)	Mass	Semimajor axis (AU)	Orbital period (days)	Eccentricity	Inclination	Radius
b	148 ₋₂₇ M_J	1.01±0.01	345.4±3.8	0.18±0.11	4.14 _−0.90°	—

References

^ 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.
^ 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.
^ Whitney Clavin (2015). "Planet 'Reared' by Four Parent Stars | NASA". NASA. Retrieved 4 March 2015.
^ Know the Star, Know the Planet. III. Discovery of Late-Type Companions to Two Exoplanet Host Stars, 2015, arXiv:1503.01211
^ 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.
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. JSTOR 40675565.
^ Determining the true mass of radial-velocity exoplanets with Gaia 9 planet candidates in the brown-dwarf/stellar regime and 27 confirmed planets, 2020, arXiv:2009.14164
Kane, Stephen R.; et al. (2015). "On the Stellar Companion to the Exoplanet Hosting Star 30 Arietis B". The Astrophysical Journal. 815 (1). 32. arXiv:1511.01533. Bibcode:2015ApJ...815...32K. doi:10.1088/0004-637X/815/1/32. S2CID 16794035.

External links

Constellation of Aries

Stars

Bayer	α (Hamal) β (Sheratan) γ (Mesarthim) δ (Botein) ε ζ η θ ι κ λ μ ν ξ ο π ρ ρ ρ σ τ τ
Flamsteed	1 4 7 10 11 14 15 16 19 20 21 23 26 27 29 30 31 33 35 36 38 39 (Lilii Borea) 40 41 (Bharani) 47 49 50 51 52 53 54 55 56 59 60 62 64 65 66 54 Cet 85 Cet
Variable	TZ UX VZ (16 Tri)
HR	577 728 803 952 999
HD	12661 20367
Other	BD+20°307 HIP 14810 HAT-P-25 Teegarden's Star WASP-11/HAT-P-10 WD 0145+234

Exoplanets	α Arietis b HD 12661 b c HIP 14810 b c d Teegarden's Star b c WASP-11b/HAT-P-10b

Galaxies

NGC	677 680 691 694 695 716 765 770 772 781 803 817 820 821 871 877 900 901 903 904 918 935 938 972 990 992 1024 1134 1156
Other	1ES 0229+200 3C 79 4C +28.07 AO 0235+164 IC 167 IC 1801 PSO J0309+27 Segue 2 UGC 2140

Galaxy clusters	MS 0302+17

Astronomical events	GRB 060218

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