C Hydrae

C Hydrae
(30 Monocerotis)
Données d'observation
(époque J2000.0)
Ascension droite 08h 25m 39,63201s[1]
Déclinaison −03° 54′ 23,1178″[1]
Constellation Hydre
Magnitude apparente 3,90[2]

Localisation dans la constellation : Hydre

(Voir situation dans la constellation : Hydre)
Caractéristiques
Stade évolutif séquence principale
Type spectral A0Va[3]
Indice U-B −0,02[2]
Indice B-V −0,02[2]
Indice R-I −0,05[2]
Astrométrie
Vitesse radiale +10,00 ± 1,78 km/s[4]
Mouvement propre μα = −66,43 mas/a[1]
μδ = −23,41 mas/a[1]
Parallaxe 26,66 ± 0,19 mas[1]
Distance 122,3 ± 0,9 al
(37,5 ± 0,3 pc)
Magnitude absolue +1,04[5]
Caractéristiques physiques
Luminosité 40,05 L[5]

Désignations

C Hya, 30 Mon, HD 71155, HIP 47307, HR 3314, BD-03°2339, FK5 316, SAO 135896[6]

C Hydrae (en abrégé C Hya) est une étoile de la constellation de l'Hydre. Sa magnitude apparente est de 3,90[2]. Elle porte également la désignation de Flamsteed de 30 Monocerotis (qui la plaçait dans la constellation proche de la Licorne et non dans l'Hydre) et la désignation de HD 71555 dans le catalogue Henry Draper. D'après la mesure de sa parallaxe annuelle par le satellite Hipparcos, l'étoile est située à environ ∼ 122 a.l. (∼ 37,4 pc) de la Terre[1]. Elle s'éloigne du Système solaire à une vitesse radiale de +10 km/s[4].

C Hydrae est une étoile blanche de la séquence principale de type spectral A0Va, comme l'est Véga par exemple[3]. Elle est 40 fois plus lumineuse que le Soleil[5]. Un excès d'infrarouge statistiquement significatif a été détecté venant de l'étoile. Ses caractéristiques indiquent la présence d'un disque de débris à une distance de 2,0 ± 0,1 ua et qui a une température de corps noir de 499 ± 3 K. Il apparaît comparable à la ceinture d'astéroïdes en taille[7].

Références

  1. a b c d e et f (en) F. van Leeuwen, « Validation of the new Hipparcos reduction », Astronomy & Astrophysics, vol. 474, no 2,‎ , p. 653–664 (DOI 10.1051/0004-6361:20078357, Bibcode 2007A&A...474..653V, arXiv 0708.1752)
  2. a b c d et e (en) D. Hoffleit et W. H. Warren, « Bright Star Catalogue, 5e éd. », Catalogue de données en ligne VizieR : V/50. Publié à l'origine dans : 1964BS....C......0H, vol. 5050,‎ (Bibcode 1995yCat.5050....0H)
  3. a et b (en) R. O. Gray et al., « Contributions to the Nearby Stars (NStars) Project: Spectroscopy of Stars Earlier than M0 within 40 Parsecs: The Northern Sample. I. », The Astronomical Journal, vol. 126, no 4,‎ , p. 2048-2059 (DOI 10.1086/378365, Bibcode 2003AJ....126.2048G, arXiv astro-ph/0308182)
  4. a et b (en) N. V. Kharchenko et al., « Astrophysical supplements to the ASCC-2.5: Ia. Radial velocities of ∼55000 stars and mean radial velocities of 516 Galactic open clusters and associations », Astronomische Nachrichten, vol. 328, no 9,‎ , p. 889 (DOI 10.1002/asna.200710776, Bibcode 2007AN....328..889K, arXiv 0705.0878)
  5. a b et c (en) E. Anderson et Ch. Francis, « XHIP: An extended Hipparcos compilation », Astronomy Letters, vol. 38, no 5,‎ , p. 331 (DOI 10.1134/S1063773712050015, Bibcode 2012AstL...38..331A, arXiv 1108.4971)
  6. (en) * 30 Mon -- High Proper Motion Star sur la base de données Simbad du Centre de données astronomiques de Strasbourg.
  7. (en) Margaret M. Moerchen, Charles M. Telesco et Christopher Packham, « High Spatial Resolution Imaging of Thermal Emission from Debris Disks », The Astrophysical Journal, vol. 723, no 2,‎ , p. 1418–1435 (DOI 10.1088/0004-637X/723/2/1418, Bibcode 2010ApJ...723.1418M, arXiv 1011.1410)

Lien externe

  • (en) Bright Star Catalogue, « HR 3314 », sur Alcyone

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