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V Scuti

V Scuti
Observationsdata
Epok: J2000.0
StjärnbildSkölden
Rektascension18t 48m 08,83s
Deklination-12° 07′ 30,73″[1]
Skenbar magnitud ()+9,7-<14,1 (V) [2]
Stjärntyp
SpektraltypM3IIIe[2]
VariabeltypPulserande Mira-variabel (M)[2]
Astrometri
Radialhastighet ()32,0 km/s
Egenrörelse (µ)RA: 17,459±0,287 mas/år
Dek.: -5,744±0,235 mas/år
Parallax ()1,1759±0,2079 mas
Andra beteckningar
2MASS J18480883-1207306[3], ASAS J184809-1207.5[4], GCRV 68635[4], IRAS 18453-1210[4], CSI-12-18443[4], Gaia DR2 4105906138510844800[4] och V Sct

V Scuti är en pulserande variabel av Mira Ceti-typ (M)[2][5] i stjärnbilden Skölden.

Stjärnan varierar mellan visuell magnitud +9,7 och svagare än 14,1 med en period av 0,95498575 dygn eller 22,919658 timmar.[2]

  1. ^ ”Basic data: V* V Sct – Variable Star of Mira Cet type” (på engelska). Centre de Données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=V+Sct&submit=SIMBAD+search. Läst 10 augusti 2019. 
  2. ^ [a b c d e] ”V Sct” (på engelska). The International Variable Star Index. AAVSO – American Association of Variable Star Observers. http://www.aavso.org/vsx/index.php?view=detail.top&oid=34121. Läst 10 augusti 2019. 
  3. ^ SIMBAD Astronomical Database, läs online, läst: 10 augusti 2019.[källa från Wikidata]
  4. ^ [a b c d e] SIMBAD Astronomical Database.[källa från Wikidata]
  5. ^ Otero, S. A.; Watson, C.; Wils, P.. ”Variable Star Type Designations in the VSX” (på engelska). AAVSOs webbsajt. AAVSO (American Association of Variable Star Observers). http://www.aavso.org/vsx/index.php?view=about.vartypes. Läst 10 augusti 2019. 
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V Scuti
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