HD 10307

HD 10307 A/B
Observation data Epoch J2000.0 Equinox J2000.0
Constellation	Andromeda
Right ascension	01^h 41^m 47.143^s^[1]
Declination	+42° 36′ 48.12″^[1]
Apparent magnitude (V)	+4.95/+12.5
Characteristics
Spectral type	G1.5 V + M V
U−B color index	0.11
B−V color index	0.62
Variable type	None
Astrometry

Radial velocity (R_v)	+3.1 km/s
Proper motion (μ)	RA: 791.47 ± 0.48^[1] mas/yr Dec.: -180.80 ± 0.36^[1] mas/yr
Parallax (π)	78.50 ± 0.54^[1] mas
Distance	41.5 ± 0.3 ly (12.74 ± 0.09 pc)
Absolute magnitude (M_V)	4.30/11.9

Details
HD 10307 A
Mass	0.97^[2] M_☉
Radius	1.20 R_☉
Luminosity	1.44 L_☉
Surface gravity (log g)	4.35 cgs
Temperature	5,881 ± 4.0^[3] K
Metallicity	96% Sun
Age	7.0 × 10⁹^[4] years
HD 10307 B
Mass	0.29 M_☉
Luminosity	0.0013 L_☉
Orbit
Companion	HR 483 B
Period (P)	19.5 yr
Semi-major axis (a)	0.58"
Eccentricity (e)	0.43
Inclination (i)	103°
Other designations
BD+41 328, GJ 67, HD 10307, HIP 7918, HR 483, LHS 1284, NStars 0141+4236, SAO 37434, YPC 350
Database references
SIMBAD	data
ARICNS	data

HD 10307 (HR 483 A) is a star similar to the Sun in mass, temperature and metal content, situated about 41 light-years from Earth in the constellation Andromeda. Its companion, HR 483 B, is a little-studied red dwarf.

HD 10307 was identified in September 2003 by astrobiologist Margaret Turnbull from the University of Arizona in Tucson as one of the most promising nearby candidates for hosting life based on her analysis of the HabCat list of stars.

System

HR 483 is a binary located 41.2 ly away, in Andromeda. The two stars orbit one another elliptically (e=0.43), approaching as close as 4.2 AU and receding to 10.5 AU, with a period of just under twenty years. Due to the high margins of error on the mass estimates for the two stars, these orbital parameters are approximate.

HD 10307, the larger component, is a main sequence, yellow, sun-like star, only slightly brighter, hotter, larger, and older than the Sun - though with a slightly smaller mass. It has a low level of activity and is a candidate Maunder minimum analog.^[2] HR 483 B, the smaller component, appears to be a red dwarf, with as little as thirty percent the mass of the sun.

Possibility of planets and life

The presence of a moderately close companion could disrupt the orbit of a hypothetical planet in HD 10307's habitable zone. However, the uncertainty of the orbital parameters makes it equally uncertain exactly where stable orbits would be in this system.

METI message to HD 10307

There was a METI message sent to HD 10307. It was transmitted from Eurasia's largest radar, 70-meter Eupatoria Planetary Radar. The message was named Cosmic Call 2, it was sent on July 6, 2003, and it will arrive at HD 10307 in September 2044.^[5]

References

1 2 3 4 5 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
1 2 Lubin, Dan; Tytler, David; Kirkman, David (March 2012), "Frequency of Maunder Minimum Events in Solar-type Stars Inferred from Activity and Metallicity Observations", The Astrophysical Journal Letters, 747 (2): L32, Bibcode:2012ApJ...747L..32L, doi:10.1088/2041-8205/747/2/L32.
↑ Kovtyukh; et al. (2003). "High precision effective temperatures for 181 F-K dwarfs from line-depth ratios". Astronomy and Astrophysics. 411 (3): 559–564. arXiv:astro-ph/0308429. Bibcode:2003A&A...411..559K. doi:10.1051/0004-6361:20031378.
↑ Mamajek, Eric E.; Hillenbrand, Lynne A. (November 2008). "Improved Age Estimation for Solar-Type Dwarfs Using Activity-Rotation Diagnostics". The Astrophysical Journal. 687 (2): 1264–1293. arXiv:0807.1686. Bibcode:2008ApJ...687.1264M. doi:10.1086/591785.
↑ (Russian) http://www.cplire.ru/rus/ra&sr/VAK-2004.html

External links

Wikimedia Commons has media related to Canes Venatici.

Andromeda constellation

Stars (list)

Bayer	α (Alpheratz) β (Mirach) γ (Almach) δ ε ζ η θ ι κ λ μ ν ξ (Adhil) ο π ρ σ τ υ (Titawin) φ χ ψ ω

Flamsteed	2 3 4 5 6 7 8 9 10 11 12 13 14 (Veritate) 15 18 22 23 26 28 32 36 39 41 44 45 47 49 51 55 56 58 59 60 62 63 64 65 66 6 Per

Variable	R S T U W X Y Z RR RS RT RU RV RW RX RY SS ST SU SW TU TW VX WZ XX XZ AB AC AD AE AF AR BM BX CC CG CN DS DX EG ET EU FF GO GP GR GY HN KK KX KZ LL LN LP LQ OP OS OU PX PY QR QX V385 V455 V529

HR	1 8 17 36 40 44 52 53 56 71 75 78 79 104 110 122 134 152 156 157 178 205 249 272 275 282 283 289 355 372 376 379 396 409 415 452 483 495 504 518 521 551 552 556 619 647 653 671 673 679 687 746 748 756 768 769 8744 8801 8837 8857 8875 8884 8925 8927 8941 8950 8955 8962 8973 8977 8986 9011 9053 9057 9074 9086 9105 9107

HD	800 8673 11884 13931 14633 15082 16175 217731 218365 218393 218915 222155

Other	ADS 48 Groombridge 34 (GX/GQ) HAT-P-6 HAT-P-16 HAT-P-19 HAT-P-28 HAT-P-32 M31V J004437.99+412923.6 NGC 44 PSR B2303+46 PSR J0218+4232 Ross 248 (HH) WASP-1 WISE 0146+4234

Star clusters

Association	NGC 206

Open	NGC 752 NGC 956 NGC 7686

Globular	Mayall II

Nebulae

Planetary	M 1-1 NGC 7662

Galaxies

Messier	31 32 110

NGC	5 11 13 19 20 27 29 39 43 48 49 51 67 67A 68 69 70 71 72 72A 74 76 79 80 81 83 85 86 90 93 94 96 97 108 109 112 140 149 160 169 181 183 184 214 218 226 228 229 233 243 252 258 260 262 266 280 304 317 389 393 404 425 431 477 512 513 528 529 531 536 537 542 551 561 562 573 590 591 605 620 662 668 679 687 700 703 704 705 708 709 710 712 714 717 721 732 746 753 759 797 801 812 818 828 834 841 845 846 891 898 906 909 910 911 912 913 914 920 923 933 937 946 980 982 995 996 999 1000 7440 7445 7446 7449 7618 7640 7707 7831 7836

Other	Andromeda I Andromeda III Andromeda IV Andromeda V Andromeda VIII Andromeda IX Andromeda X Andromeda XI Andromeda XII Andromeda XXI B2 0206+35 3C 13 3C 46 3C 65 3C 66A 3C 66B IRAS 23365+3604 QSO B0133+476

Galaxy
clusters

Other

GRB 050824
SN 1885A

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