HD 10307

HD 10307: HD 10307 A/B
Observation data
Epoch J2000.0 Equinox J2000.0

Constellation Andromeda

Right ascension 01^h 41^m 47.1^s

Declination +42° 36' 48.1"

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: 791.35 mas/yr
Dec.: -180.16 mas/yr

Parallax (π) 79.09 ± 0.83 mas

Distance 41.2 ± 0.4 ly
(12.6 ± 0.1 pc)

Absolute magnitude (M_V) 4.30/11.9

Details

Mass 0.97/0.29 M_☉

Radius 1.20/? R_☉

Surface gravity (log g) 4.35/?

Luminosity 1.44/0.0013 L_☉

Temperature 5881 ± 4.0 ^[1]/? K

Metallicity 96% Sun

Rotation ?/?

Age 7.0 × 10⁹^[2] years

Orbit

Companion HR 483 B

Period (P) 19.5 yr

Semimajor axis (a) 0.58"

Eccentricity (e) 0.43

Inclination (i) 103°

Database references

SIMBAD data

ARICNS data

Other designations

BD+41 328, GJ 67, HD 10307, HIP 7918, HR 483, LHS 1284, NStars 0141+4236, SAO 37434, YPC 350

HD 10307 (aka 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.

Contents

1 System

2 Possibility of planets and life

3 METI message to HD 10307

4 References

5 External links

System

HR 483 is a binary star located 41.2 ly away, in Andromeda. The pair 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, and larger than the Sun. 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.^[3]

References

^ 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. http://www.aanda.org/articles/aa/full/2003/46/aa3944/aa3944.html.

^ 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. Bibcode 2008ApJ...687.1264M. doi:10.1086/591785.

^ (Russian) http://www.cplire.ru/rus/ra&sr/VAK-2004.html

External links

High proper-motion Star

GJ 67B

Image HD 10307

ARICNS: 00144 (A)

ARICNS: 00145 (B)

NStars: 0141+4236

SolStation: HR 483 / HD 10307 AB

Space.com: Top 10 List of Habitable Stars to Guide Search

Spectra HD 10307

v · ← «Bright» star systems within 40–50 light-years →

Star systems within 40–50 light-years from Earth with brightest member's absolute magnitude of +8.5 or brighter.

Giant
star

A III

Alpha Ophiuchi «Rasalhague» (46.7 ± 0.6 ly; 1 star)

G III

Capella (42.2 ± 0.5 ly; 4 stars)

A
(White)

IV

Alpha Cephei «Alderamin» (48.8 ± 0.4 ly; 1 star)

V

Iota Ursae Majoris «Talitha Borealis» (47.7 ± 0.6 ly; 4 stars)

F
(Yellow-
white)

IV

Beta Trianguli Australis (40.2 ± 0.3 ly; 2 stars)‡ • Theta Ursae Majoris «Alhaud» (44.0 ± 0.4 ly; 3 stars) • Delta Aquilae «Denebokab» (50.1 ± 0.6 ly; 3 stars)‡

V

36 Ursae Majoris (41.9 ± 0.4 ly; 2 stars) • Upsilon Andromedae (43.9 ± 0.4 ly; 2 stars, 4 planets: planet b • planet c • planet d • planet e) • 10 Tauri (44.8 ± 0.5 ly; 2 stars) • Iota Piscium (45.0 ± 0.5 ly; 1 star) • Alpha Fornacis «Dalim» (46.0 ± 0.4 ly; 2 stars) • Theta Boötis «Asellus Primus» (47.5 ± 0.4 ly; 2 stars) • Psi Capricorni «Yue» (47.9 ± 0.6 ly; 1 star) • Alpha Corvi «Alchiba» (48.2 ± 0.5 ly; 1 star) • Eta Leporis (49.1 ± 0.5 ly; 1 star) • Nu Phoenicis (49.1 ± 0.5 ly; 1 star) • Sigma Boötis «Hemelein Secunda» (50.4 ± 0.6 ly; 2 stars)‡

G
(Yellow)

IV

Beta Aquilae «Alshain» (44.7 ± 0.5 ly; 2 stars) • b (31) Aquilae (49.4 ± 0.6 ly; 3 stars)

V

Rho¹ (55) Cancri (40.9 ± 0.4 ly; 2 stars, 5 planets: planet e • planet b • planet c • planet f • planet d) • HR 483 (41.2 ± 0.4 ly; 2 stars) • Lambda Aurigae «Al Hurr» (41.2 ± 0.5 ly; 2 stars) • HR 683 (41.4 ± 0.4 ly; 1 star) • i (44) Boötis (41.6 ± 0.3 ly; 3 stars) • HR 6094 (42.0 ± 0.5 ly; 2 stars, 1 planet: planet b) • HR 6998 (42.4 ± 0.5 ly; 1 star) • 58 Eridani (43.4 ± 0.5 ly; 1 star) • HR 8501 (44.4 ± 0.4 ly; 2 stars) • 18 Scorpii (45.7 ± 0.6 ly; 1 star) • 47 Ursae Majoris (45.9 ± 0.4 ly; 1 star, 3 planets: planet b • planet c • planet d) • 26 Draconis (45.9 ± 0.3 ly; 3 stars) • Pi¹ Ursae Majoris (46.6 ± 0.5 ly; 1 star) • 72 Herculis (46.9 ± 0.4 ly; 1 star) • Nu² Lupi (47.5 ± 0.5 ly; 1 star, 3 planets: planet b • planet c • planet d) • HR 7898 (47.8 ± 0.6 ly; 1 star) • Psi Serpentis (47.9 ± 0.6 ly; 2 stars) • HR 3862 (48.5 ± 0.5 ly; 1 star) • 20 Leonis Minoris «Cor» (48.6 ± 0.6 ly; 1 star) • HD 176051 (48.9 ± 0.4 ly; 2 stars, 1 planet: planet b) • Mu Arae (49.8 ± 0.6 ly; 1 star, 4 planets: planet d • planet e • planet b • planet c)‡ • 51 Pegasi (50.1 ± 0.6 ly; 1 star, 1 planet: planet b «Bellerophon»)‡ • HR 2007 (50.8 ± 0.9 ly; 1 star, 1 planet: planet b)‡

K
(Orange)

IV

HR 4587 (42.1 ± 0.4 ly; 1 star) • Gamma Cephei «Errai» (45.0 ± 0.3 ly; 2 stars, 1 planet: planet b) • Eta Cephei «Al Agemim» (46.8 ± 0.3 ly; 1 star)

V

HR 3384 (39.7 ± 0.3 ly; 1 star)‡ • HR 1925 (39.9 ± 0.4 ly; 1 star)‡ • Gliese 435 (40.8 ± 0.5 ly; 1 star) • HR 3259 (41.0 ± 0.4 ly; 1 star, 3 planets: planet b • planet c • planet d) • Gliese 349 (41.4 ± 0.6 ly; 1 star) • HR 6518 (41.7 ± 0.3 ly; 1 star) • HD 40307 (41.8 ± 0.3 ly; 1 star, 3 planets: planet b • planet c • planet d) • Gliese 428 (42.0 ± 1.0 ly; 2 stars) • Gliese 707 (42.3 ± 0.7 ly; 1 star) • Gliese 204 (42.3 ± 0.5 ly; 1 star) • Gliese 167 (42.7 ± 0.3 ly; 1 star) • Gliese 425 (42.9 ± 1.0 ly; 2 stars) • Gliese 716 (43.1 ± 0.5 ly; 1 star) • Gliese 174 (44.0 ± 0.8 ly; 1 star) • Gliese 656 (44.6 ± 0.6 ly; 1 star) • Gliese 5 (44.7 ± 0.5 ly; 2 stars) • AB Doradus (48.7 ± 0.4 ly; 2 stars)

In left column are stellar classes of primary members of star systems. ‡Distance error margin extends out of declared distance interval. Italic are systems possibly located within declared distance interval, but probably not.

Categories:
Andromeda constellation
Binary stars
Henry Draper Catalogue objects
HIP objects
M-type main sequence stars
G-type main sequence stars
Main sequence star stubs
Multiple star stubs

HD 10307 A/B
Observation data Epoch J2000.0 Equinox J2000.0
Constellation	Andromeda
Right ascension	01^h 41^m 47.1^s
Declination	+42° 36' 48.1"
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: 791.35 mas/yr Dec.: -180.16 mas/yr
Parallax (π)	79.09 ± 0.83 mas
Distance	41.2 ± 0.4 ly (12.6 ± 0.1 pc)
Absolute magnitude (M_V)	4.30/11.9

Details

Mass	0.97/0.29 M_☉
Radius	1.20/? R_☉
Surface gravity (log g)	4.35/?
Luminosity	1.44/0.0013 L_☉
Temperature	5881 ± 4.0 ^[1]/? K
Metallicity	96% Sun
Rotation	?/?
Age	7.0 × 10⁹^[2] years

Orbit
Companion	HR 483 B
Period (P)	19.5 yr
Semimajor axis (a)	0.58"
Eccentricity (e)	0.43
Inclination (i)	103°
Database references
SIMBAD	data
ARICNS	data
Other designations
BD+41 328, GJ 67, HD 10307, HIP 7918, HR 483, LHS 1284, NStars 0141+4236, SAO 37434, YPC 350

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(10307) 1990 QX1 — is a main belt minor planet. It was discovered by Henry E. Holt at the Palomar Observatory in San Diego County, California, on August 22, 1990.[1] See also List of minor planets: 10001–11000 References ^ JPL Small Body Database Browser … Wikipedia
10307 — Staten Island, Ny (Miscellaneous » ZIP Codes) … Abbreviations dictionary
HD 10307 — Звезда Наблюдательные данные (Эпоха J2000,0) Прямое восхождение … Википедия
HD 10307 — A/B Constelación Andrómeda Ascensión recta α 01h 41min 47,14s Declinación δ +42º 36’ 48,1’’ Distancia … Wikipedia Español
HD 10307 — Données d observation (Époque J2000.0) Ascension droite 01h 41m 47.1s Déclinaison 42° 36′ 48.1″ Constellation Andromède Magnitude apparente 4,95 / … Wikipédia en Français
ISO 10307-1:1993 — изд.1 C TC 28 Нефтепродукты. Общий осадок в топочных мазутах. Часть 1. Определение способом высокотемпературной очистки Изменения и дополнения: – ISO 10307 1:1993/Cor.1:1997 (изд.1 TC 28) раздел 75.160.20 … Стандарты Международной организации по стандартизации (ИСО)
ГОСТ Р ИСО 10307-1-2009 — 12 с. (3) Нефтепродукты. Определение содержания общего осадка в остаточных жидких топливах. Часть 1. Метод горячей фильтрации раздел 75.080 … Указатель национальных стандартов 2013
ГОСТ Р ИСО 10307-1-2009: Нефтепродукты. Определение содержания общего осадка в остаточных жидких топливах. Часть 1. Метод горячей фильтрации — Терминология ГОСТ Р ИСО 10307 1 2009: Нефтепродукты. Определение содержания общего осадка в остаточных жидких топливах. Часть 1. Метод горячей фильтрации оригинал документа: 3.1 общий осадок: Сумма нерастворимых органических и неорганических… … Словарь-справочник терминов нормативно-технической документации
ISO 10307-2:1993 — изд.1 C TC 28 Нефтепродукты. Общий осадок в топоных мазутах. Часть 2. Определение с использованием стандартных процедур старения раздел 75.160.20 … Стандарты Международной организации по стандартизации (ИСО)
Поток Наличности — А. Сумма полученных или выплаченных наличных денег. Б. Разность между суммами поступлений и выплат денежных средств компании за определенный период времени. Словарь бизнес терминов. Академик.ру. 2001 … Словарь бизнес-терминов

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HD 10307

Contents

System

Possibility of planets and life

METI message to HD 10307

References

External links

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HD 10307

Contents

System

Possibility of planets and life

METI message to HD 10307

References

External links

Look at other dictionaries:

Share the article and excerpts

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