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Charakterystyka. Homam to błękitna gwiazda należąca do typu widmowego B8, sklasyfikowana jako gwiazda ciągu głównego, lecz prawdopodobnie kończy ona już syntezę wodoru w hel w jądrze i jest w rzeczywistości podolbrzymem. Jej temperatura to 11 190 K, ma ona promień równy 4 R ☉ i masę od 3,3 do 3,5 masy Słońca.
Zeta Pegasi or ζ Pegasi, formally named Homam (/ ˈ h oʊ m æ m /), is a single star in the northern constellation of Pegasus. With an apparent visual magnitude of +3.4, [2] this star is bright enough to be seen with the naked eye and is one of the brighter members of Pegasus.
Homam, also designated as ζ Pegasi (zeta Pegasi), is a double main-sequence star in the constellation of Pegasus . Homam visual magnitude is 3.4. Because of its moderate brightness, Homam should be easily visible from locations with dark skies, while it can be barely visible, or not visible at all, from skies affected by light ...
Zeta Pegasi (HR8634) alpha (2000) = 22h 41m 27.64s , delta (2000) = +10d 49' 53.2'' V = 3.40, B-V = -0.09, Spectral type: B8V. Field is 10.0 x 10.0 arcmin. Hamuy et al (1992, 1994) data (16A bins) ftp access to visible wavelength data files for this standard. ESO is the European Organisation for Astronomical Research in the Southern Hemisphere.
Zeta Pegasi – gwiazda w gwiazdozbiorze Pegaza, odległa od Słońca o około 204 lata świetlne.
HOMAM (Zeta Pegasi). The name really belongs to a pair of stars, Zeta and Xi Pegasi (in Pegasus, the Flying Horse), which together to the ancient Arabs became known (translated from an obscure phrase) as the "lucky stars of the hero," presumably of the hero Perseus.The name then devolved specifically to third magnitude (3.40) Zeta Pegasi, leaving poor fourth magnitude Xi Peg (which lies just ...
Zeta Pegasi or ζ Pegasi, formally named Homam ( / ˈhoʊmæm / ), is a single star in the northern constellation of Pegasus. With an apparent visual magnitude of +3.4, this star is bright enough to be seen with the naked eye and is one of the brighter members of Pegasus.
