Epsilon Delphini

Epsilon Delphini (ε Delphini, abbreviated Eps Del, ε Del), officially named Aldulfin /ælˈdʌlfən/, is a solitary, blue-white hued star in the northern constellation of Delphinus. It is visible to the naked eye with an apparent visual magnitude of 4.03. Based upon an annual parallax shift of 9.87 mas as seen from the Earth, the system is located about 330 light-years from the Sun. At Epsilon Delphini's distance, the visual magnitude is diminished by an extinction factor of 0.11 due to interstellar dust. The star is moving closer to the Sun with a radial velocity of −19 km/s.

ε Delphini
Location of ε Delphini (circled)
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Delphinus
Right ascension 20h 33m 12.77192s
Declination +11° 18 11.7412
Apparent magnitude (V) 4.03 (3.95−4.05)
Characteristics
Spectral type B6 III
U−B color index −0.46
B−V color index −0.13
Variable type suspected
Astrometry
Radial velocity (Rv)−19.4±0.7 km/s
Proper motion (μ) RA: +11.96 mas/yr
Dec.: −28.97 mas/yr
Parallax (π)9.87 ± 0.21 mas
Distance330 ± 7 ly
(101 ± 2 pc)
Absolute magnitude (MV)−0.06
Details
Radius4.6 R
Luminosity676 L
Surface gravity (log g)3.71±0.09 cgs
Temperature13,614±15 K
Metallicity [Fe/H]+0.08±0.10 dex
Rotational velocity (v sin i)52±4 km/s
Age220 Myr
Other designations
Aldulfin, ε Del, 2 Del, BD+10° 4321, FK5 768, HD 195810, HIP 101421, HR 7852, SAO 106230
Database references
SIMBADdata

This is a B-type giant star with a stellar classification of B6 III. It has 4.6 times the Sun's radius and is radiating 676 times the solar luminosity from its photosphere at an effective temperature of 13,614 K. The star may be slightly variable, occasionally brightening to magnitude 3.95. It is spinning with a projected rotational velocity of 52 km/s.

This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.