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Star in the constellation Auriga
Omicron Aurigae is an astrometric binary star system in the northern constellation of Auriga. Its name is a Bayer designation that is Latinized from ο
Omicron_Aurigae
Quasar in the constellation Auriga
constellation Auriga not far in the sky from the 5th magnitude star Omicron Aurigae. The "distance" of a far away galaxy depends on the distance measurement
3C_147
Star naming system
both constellations: Alpha Andromedae = Delta Pegasi, Beta Tauri = Gamma Aurigae, and Nu Boötis = Psi Herculis. (He catalogued Fomalhaut only once, as Alpha
Bayer_designation
Common proper motion binary star in the constellation Ursa Minor
Bibcode:2006ApJ...643.1160L, doi:10.1086/503183, S2CID 119520529. The Electronic Sky University of Florida Astronomy Department HR 1971 Image Omicron Aurigae
Pi1_Ursae_Minoris
reassigned to Scorpius – Star Tales – Norma Also designated Gamma Aurigae (γ Aur, γ Aurigae) by Bayer, after Ptolemy – Bayer’s Uranometria and Bayer letters
Table of stars with Bayer designations
Table_of_stars_with_Bayer_designations
Cloud Galaxy 1.88 Alpha Trianguli Australis (Atria) Star 1.90 1.89 Beta Aurigae (Menkalinan) Binary star system 1.918 Alpha Pavonis (Peacock) Binary star
List of brightest natural objects in the sky
List_of_brightest_natural_objects_in_the_sky
Triple star system in the constellation Cygnus
distance of approximately 1,120 light years. The Bayer designation ο (omicron) has been variously applied to two or three of the stars 30, 31, and 32
31_Cygni
Aquarius B5 III 5.43 V357 Carinae 450 ± 20 Carina B2IV-V +3.41 - 3.44 Iota Aurigae (Hassaleh) 450 ± 20 Auriga K3 II–III 2.69 28 Monocerotis 450 ± 20 Monoceros
List of star systems within 450–500 light-years
List_of_star_systems_within_450–500_light-years
Part of Latin grammar
poēta, poētae m. ('poet'), agricola, agricolae m. ('farmer'), auriga, aurigae m. ('auriga, charioteer'), pīrāta, pīrātae m. ('pirate') and nauta, nautae
Latin_declension
2 DAZ B L8-L9 Gaia-4 241 K Has one confirmed exoplanet (Gaia-4 b). Eta Aurigae (Haedus) 243 ± 4 Auriga B3 V 3.18 39 Ceti (AY Ceti) A 244 ± 2 Cetus G5IIIe
List of star systems within 200–250 light-years
List_of_star_systems_within_200–250_light-years
Kaʿab Dhiy l-ʿInān the Shoulder of the Rein-holder كعب ذي العنان Iota Aurigae also named Hassaleh Kaffaljidhma al-Kaff al-Jadhmā' the Cut-short Hand
List_of_Arabic_star_names
Type of star
Gamma Pegasi (Algenib) 2.84 B2IV 113 Zeta Pegasi (Homam) 3.41 B8V 0.96 63 Omicron Velorum 3.63 B3IV 2.80 151 Iota Herculis (Tianbang) 3.80 B3IV 3.49 139
Slowly_pulsating_B-type_star
95 Part of Coma Star Cluster. K2-155 267 K7 Has 3 exoplanets. 14 Aurigae (KW Aurigae) A 269 ± 4 Auriga A9IV + ? 5.01 B F5V C M3V: D WDA K2-384 270 M0V
List of star systems within 250–300 light-years
List_of_star_systems_within_250–300_light-years
Constellation in the northern celestial hemisphere
"Properties of main-sequence eclipsing binaries - Into the G stars with HS Aurigae, FL Lyrae, and EW Orionis". The Astronomical Journal. 91: 383. Bibcode:1986AJ
Lyra
American astronomer
realized that there were many undiscovered ones. He soon found that Beta Aurigae and Delta Orionis were eclipsing binaries. Further discoveries followed
Joel_Stebbins
Red supergiant star in the constellation Orion
supernovae, and there is strong evidence that OB stars μ Columbae, AE Aurigae, and 53 Arietis all originated from such explosions in Ori OB1 2.2, 2.7
Betelgeuse
Zodiac constellation straddling the celestial equator
constellation of Auriga. As a result, it also bears the designation Gamma Aurigae. Zeta Tauri (the proper name is Tianguan) is an eclipsing binary star that
Taurus_(constellation)
813s +19° 17′ 37.88″ A0Vnp λ Boo or A0IV-V(n)kB8 3.86 B A2IVpSiSrCr Theta Aurigae (Mahasim) A 166 ± 1 Auriga 05h 59m 43.27012s +37° 12′ 45.3047″ A0pSi 2
List of star systems within 150–200 light-years
List_of_star_systems_within_150–200_light-years
List of stars with high proper motion
Librae 0.387 +48.85 PM; RM 38 Aurigae 0.178 +35.90 PM; RM 39 Arietis Lilii Borea 0.195 −15.73 Name; PM; RM 39 Aurigae 0.153 +29.31 PM; RM 40 Eridani
List of stars with large proper motion
List_of_stars_with_large_proper_motion
Overview of the events of 2022 in science
neurons. The CDC confirms the Omicron variant causes less severe disease than previously dominant variants. The novel Omicron subtype 'BA.2' did not initially
January–March_2022_in_science
is effective against all SARS-CoV-2 variants known to date, including Omicron. A study presents a mechanism by which the hypothesized potential dark-energy-explaining
2022_in_science
Canopus (fourth time) +480,000 +990,000 +480,000 −0.40 346 310 −0.72 Beta Aurigae (Menkalinan) +990,000 +1,150,000 +1,190,000 −0.40 28.5 82.1 1.9 Delta Scuti
Historical_brightest_stars
Star whose brightness fluctuates, as seen from Earth
Herbig Ae/Be stars, are the more massive form. The fourth are the RW Aurigae irregular variables that have similar properties but lack nearby nebulosity
Variable_star
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