From Wikipedia, the free encyclopedia
HD 1032
Observation data
Epoch J2000.0       Equinox J2000.0 ( ICRS)
Constellation Octans
Right ascension 00h 13m 19.6219s [1]
Declination −84° 59′ 38.3178″ [1]
Apparent magnitude (V) 5.77 [2]
Characteristics
Evolutionary stage AGB [3]
Spectral type M0/1 III [4]
U−B color index +2.10 [2]
B−V color index +1.72 [2]
Variable type suspected [5]
Astrometry
Radial velocity (Rv)4±0.4 [6] km/s
Proper motion (μ) RA: +11.046  mas/ yr [1]
Dec.: +17.696  mas/ yr [1]
Parallax (π)3.8517 ± 0.0501  mas [1]
Distance850 ± 10  ly
(260 ± 3  pc)
Absolute magnitude (MV)−1.57 [7]
Details
Mass1.11 [8]  M
Radius95.54 [9]  R
Luminosity1,461 [10]  L
Surface gravity (log g)0.69 [8]  cgs
Temperature3,838±122 [11]  K
Metallicity [Fe/H]−0.08 [8]  dex
Other designations
2 G. Octantis [12], CPD−85°2, FK5 3972, GC 257, HD 1032, HIP 1074, HR 47, SAO 258217 [13]
Database references
SIMBAD data

HD 1032 (HR 47) is a solitary [14] star in the southern circumpolar constellation Octans. It is faintly visible to the naked eye with an apparent magnitude of 5.77 [2] and is estimated to be 850 light years away from the Solar System based on parallax measure. [1] However, it is receding with a heliocentric radial velocity of km/s.

HD 1032 is an asymptotic giant branch [3] star with a stellar classification of M0/1 III [4] — intermediate between a M0 and M1 giant star. It has 111% the mass of the Sun [8] and an enlarged radius of 95.54  R [9] as a result of its evolved state. It radiates at 1,461 times the luminosity of the Sun [10] from its photosphere at an effective temperature of 3,838  K, [11] giving a red hue. HD 1032 is slightly metal deficient with an iron abundance 83% that of the Sun. [8]

This is a suspected variable star that fluctuates between magnitudes 5.82 and 5.88 in the Hipparcos passband. [5]

References

  1. ^ a b c d e Brown, A. G. A.; et al. (Gaia collaboration) (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics. 649: A1. arXiv: 2012.01533. Bibcode: 2021A&A...649A...1G. doi: 10.1051/0004-6361/202039657. S2CID  227254300. (Erratum:  doi: 10.1051/0004-6361/202039657e). Gaia EDR3 record for this source at VizieR.
  2. ^ a b c d Ducati, J. R. (2002). "VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system". CDS/ADC Collection of Electronic Catalogues. 2237. Bibcode: 2002yCat.2237....0D.
  3. ^ a b Eggen, Olin J. (July 1992). "Asymptotic giant branch stars near the sun". The Astronomical Journal. 104: 275. Bibcode: 1992AJ....104..275E. doi: 10.1086/116239. ISSN  0004-6256.
  4. ^ a b Houk, N.; Cowley, A. P. (1975). University of Michigan Catalogue of two-dimensional spectral types for the HD stars. Volume I. Declinations -90_ to -53_ƒ0. Bibcode: 1975mcts.book.....H.
  5. ^ a b Samus’, N. N.; Kazarovets, E. V.; Durlevich, O. V.; Kireeva, N. N.; Pastukhova, E. N. (January 2017). "General catalogue of variable stars: Version GCVS 5.1". Astronomy Reports. 61 (1): 80–88. Bibcode: 2017ARep...61...80S. doi: 10.1134/S1063772917010085. ISSN  1063-7729. S2CID  255195566.
  6. ^ Gontcharov, G. A. (November 2006). "Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system". Astronomy Letters. 32 (11): 759–771. arXiv: 1606.08053. Bibcode: 2006AstL...32..759G. doi: 10.1134/S1063773706110065. ISSN  1063-7737. S2CID  119231169.
  7. ^ Anderson, E.; Francis, Ch. (May 2012). "XHIP: An extended hipparcos compilation". Astronomy Letters. 38 (5): 331–346. arXiv: 1108.4971. Bibcode: 2012AstL...38..331A. doi: 10.1134/S1063773712050015. ISSN  1063-7737. S2CID  119257644.
  8. ^ a b c d e Anders, F.; et al. (August 2019). "Photo-astrometric distances, extinctions, and astrophysical parameters for Gaia DR2 stars brighter than G = 18". Astronomy & Astrophysics. 628: A94. arXiv: 1904.11302. Bibcode: 2019A&A...628A..94A. doi: 10.1051/0004-6361/201935765. ISSN  0004-6361.
  9. ^ a b Kervella, Pierre; Arenou, Frédéric; Thévenin, Frédéric (2022). "Stellar and substellar companions from Gaia EDR3". Astronomy & Astrophysics. 657: A7. arXiv: 2109.10912. Bibcode: 2022A&A...657A...7K. doi: 10.1051/0004-6361/202142146. eISSN  1432-0746. ISSN  0004-6361.
  10. ^ a b McDonald, I.; Zijlstra, A. A.; Watson, R. A. (15 June 2017). "Fundamental parameters and infrared excesses of Tycho–Gaia stars". Monthly Notices of the Royal Astronomical Society. 471 (1): 770–791. arXiv: 1706.02208. Bibcode: 2017MNRAS.471..770M. doi: 10.1093/mnras/stx1433. eISSN  1365-2966. ISSN  0035-8711.
  11. ^ a b Stassun, Keivan G.; et al. (9 September 2019). "The Revised TESS Input Catalog and Candidate Target List". The Astronomical Journal. 158 (4): 138. arXiv: 1905.10694. Bibcode: 2019AJ....158..138S. doi: 10.3847/1538-3881/ab3467. ISSN  0004-6256.
  12. ^ Gould, Benjamin Apthorp (1878). "Uranometria Argentina : brillantez y posicion de las estrellas fijas, hasta la septima magnitud, comprendidas dentro de cien grados del polo austral : con atlas". Resultados del Observatorio Nacional Argentino. 1. Bibcode: 1879RNAO....1.....G.
  13. ^ "HR 47". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved July 1, 2022.
  14. ^ Eggleton, P. P.; Tokovinin, A. A. (11 September 2008). "A catalogue of multiplicity among bright stellar systems". Monthly Notices of the Royal Astronomical Society. 389 (2): 869–879. arXiv: 0806.2878. Bibcode: 2008MNRAS.389..869E. doi: 10.1111/j.1365-2966.2008.13596.x. eISSN  1365-2966. ISSN  0035-8711.
From Wikipedia, the free encyclopedia
HD 1032
Observation data
Epoch J2000.0       Equinox J2000.0 ( ICRS)
Constellation Octans
Right ascension 00h 13m 19.6219s [1]
Declination −84° 59′ 38.3178″ [1]
Apparent magnitude (V) 5.77 [2]
Characteristics
Evolutionary stage AGB [3]
Spectral type M0/1 III [4]
U−B color index +2.10 [2]
B−V color index +1.72 [2]
Variable type suspected [5]
Astrometry
Radial velocity (Rv)4±0.4 [6] km/s
Proper motion (μ) RA: +11.046  mas/ yr [1]
Dec.: +17.696  mas/ yr [1]
Parallax (π)3.8517 ± 0.0501  mas [1]
Distance850 ± 10  ly
(260 ± 3  pc)
Absolute magnitude (MV)−1.57 [7]
Details
Mass1.11 [8]  M
Radius95.54 [9]  R
Luminosity1,461 [10]  L
Surface gravity (log g)0.69 [8]  cgs
Temperature3,838±122 [11]  K
Metallicity [Fe/H]−0.08 [8]  dex
Other designations
2 G. Octantis [12], CPD−85°2, FK5 3972, GC 257, HD 1032, HIP 1074, HR 47, SAO 258217 [13]
Database references
SIMBAD data

HD 1032 (HR 47) is a solitary [14] star in the southern circumpolar constellation Octans. It is faintly visible to the naked eye with an apparent magnitude of 5.77 [2] and is estimated to be 850 light years away from the Solar System based on parallax measure. [1] However, it is receding with a heliocentric radial velocity of km/s.

HD 1032 is an asymptotic giant branch [3] star with a stellar classification of M0/1 III [4] — intermediate between a M0 and M1 giant star. It has 111% the mass of the Sun [8] and an enlarged radius of 95.54  R [9] as a result of its evolved state. It radiates at 1,461 times the luminosity of the Sun [10] from its photosphere at an effective temperature of 3,838  K, [11] giving a red hue. HD 1032 is slightly metal deficient with an iron abundance 83% that of the Sun. [8]

This is a suspected variable star that fluctuates between magnitudes 5.82 and 5.88 in the Hipparcos passband. [5]

References

  1. ^ a b c d e Brown, A. G. A.; et al. (Gaia collaboration) (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics. 649: A1. arXiv: 2012.01533. Bibcode: 2021A&A...649A...1G. doi: 10.1051/0004-6361/202039657. S2CID  227254300. (Erratum:  doi: 10.1051/0004-6361/202039657e). Gaia EDR3 record for this source at VizieR.
  2. ^ a b c d Ducati, J. R. (2002). "VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system". CDS/ADC Collection of Electronic Catalogues. 2237. Bibcode: 2002yCat.2237....0D.
  3. ^ a b Eggen, Olin J. (July 1992). "Asymptotic giant branch stars near the sun". The Astronomical Journal. 104: 275. Bibcode: 1992AJ....104..275E. doi: 10.1086/116239. ISSN  0004-6256.
  4. ^ a b Houk, N.; Cowley, A. P. (1975). University of Michigan Catalogue of two-dimensional spectral types for the HD stars. Volume I. Declinations -90_ to -53_ƒ0. Bibcode: 1975mcts.book.....H.
  5. ^ a b Samus’, N. N.; Kazarovets, E. V.; Durlevich, O. V.; Kireeva, N. N.; Pastukhova, E. N. (January 2017). "General catalogue of variable stars: Version GCVS 5.1". Astronomy Reports. 61 (1): 80–88. Bibcode: 2017ARep...61...80S. doi: 10.1134/S1063772917010085. ISSN  1063-7729. S2CID  255195566.
  6. ^ Gontcharov, G. A. (November 2006). "Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system". Astronomy Letters. 32 (11): 759–771. arXiv: 1606.08053. Bibcode: 2006AstL...32..759G. doi: 10.1134/S1063773706110065. ISSN  1063-7737. S2CID  119231169.
  7. ^ Anderson, E.; Francis, Ch. (May 2012). "XHIP: An extended hipparcos compilation". Astronomy Letters. 38 (5): 331–346. arXiv: 1108.4971. Bibcode: 2012AstL...38..331A. doi: 10.1134/S1063773712050015. ISSN  1063-7737. S2CID  119257644.
  8. ^ a b c d e Anders, F.; et al. (August 2019). "Photo-astrometric distances, extinctions, and astrophysical parameters for Gaia DR2 stars brighter than G = 18". Astronomy & Astrophysics. 628: A94. arXiv: 1904.11302. Bibcode: 2019A&A...628A..94A. doi: 10.1051/0004-6361/201935765. ISSN  0004-6361.
  9. ^ a b Kervella, Pierre; Arenou, Frédéric; Thévenin, Frédéric (2022). "Stellar and substellar companions from Gaia EDR3". Astronomy & Astrophysics. 657: A7. arXiv: 2109.10912. Bibcode: 2022A&A...657A...7K. doi: 10.1051/0004-6361/202142146. eISSN  1432-0746. ISSN  0004-6361.
  10. ^ a b McDonald, I.; Zijlstra, A. A.; Watson, R. A. (15 June 2017). "Fundamental parameters and infrared excesses of Tycho–Gaia stars". Monthly Notices of the Royal Astronomical Society. 471 (1): 770–791. arXiv: 1706.02208. Bibcode: 2017MNRAS.471..770M. doi: 10.1093/mnras/stx1433. eISSN  1365-2966. ISSN  0035-8711.
  11. ^ a b Stassun, Keivan G.; et al. (9 September 2019). "The Revised TESS Input Catalog and Candidate Target List". The Astronomical Journal. 158 (4): 138. arXiv: 1905.10694. Bibcode: 2019AJ....158..138S. doi: 10.3847/1538-3881/ab3467. ISSN  0004-6256.
  12. ^ Gould, Benjamin Apthorp (1878). "Uranometria Argentina : brillantez y posicion de las estrellas fijas, hasta la septima magnitud, comprendidas dentro de cien grados del polo austral : con atlas". Resultados del Observatorio Nacional Argentino. 1. Bibcode: 1879RNAO....1.....G.
  13. ^ "HR 47". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved July 1, 2022.
  14. ^ Eggleton, P. P.; Tokovinin, A. A. (11 September 2008). "A catalogue of multiplicity among bright stellar systems". Monthly Notices of the Royal Astronomical Society. 389 (2): 869–879. arXiv: 0806.2878. Bibcode: 2008MNRAS.389..869E. doi: 10.1111/j.1365-2966.2008.13596.x. eISSN  1365-2966. ISSN  0035-8711.

Videos

Youtube | Vimeo | Bing

Websites

Google | Yahoo | Bing

Encyclopedia

Google | Yahoo | Bing

Facebook