C/2014 UN₂₇₁ (Bernardinelli-Bernstein)
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C/2014 UN₂₇₁ (Bernardinelli-Bernstein)
Summary
C/2014 UN₂₇₁ (Bernardinelli-Bernstein) is a non-periodic comet[1]. C/2014 UN₂₇₁ (Bernardinelli-Bernstein) ranks in the top 10% of non_periodic_comet entities by monthly Wikipedia readership (94 views/month).[2]
Key Facts
- C/2014 UN₂₇₁ (Bernardinelli-Bernstein) is credited with the discovery of Pedro H. Bernardinelli[3].
- C/2014 UN₂₇₁ (Bernardinelli-Bernstein) is credited with the discovery of Gary Bernstein[4].
- C/2014 UN₂₇₁ (Bernardinelli-Bernstein)'s image is recorded as Comet Bernardinelli-Bernstein annotated - noirlab2119b.jpg[5].
- C/2014 UN₂₇₁ (Bernardinelli-Bernstein)'s instance of is recorded as non-periodic comet[6].
- C/2014 UN₂₇₁ (Bernardinelli-Bernstein)'s site of astronomical discovery is recorded as The Dark Energy Survey[7].
- C/2014 UN₂₇₁ (Bernardinelli-Bernstein)'s Commons category is recorded as C/2014 UN271 (Bernardinelli-Bernstein)[8].
- C/2014 UN₂₇₁ (Bernardinelli-Bernstein)'s parent astronomical body is recorded as Sun[9].
- C/2014 UN₂₇₁ (Bernardinelli-Bernstein)'s provisional designation is recorded as C/2014 UN271[10].
- C/2014 UN₂₇₁ (Bernardinelli-Bernstein)'s type of orbit is recorded as Oort cloud[11].
- C/2014 UN₂₇₁ (Bernardinelli-Bernstein)'s time of discovery or invention is recorded as +2014-10-20T00:00:00Z[12].
- C/2014 UN₂₇₁ (Bernardinelli-Bernstein)'s JPL Small-Body Database SPK-ID is recorded as 1003787[13].
- C/2014 UN₂₇₁ (Bernardinelli-Bernstein)'s orbital eccentricity is recorded as {'amount': '+0.9981093984445126'}[14].
- C/2014 UN₂₇₁ (Bernardinelli-Bernstein)'s official name is recorded as {'lang': 'mul', 'text': 'C/2014 UN271 (Bernardinelli-Bernstein)'}[15].
- C/2014 UN₂₇₁ (Bernardinelli-Bernstein)'s absolute magnitude is recorded as {'amount': '+7.96'}[16].
- C/2014 UN₂₇₁ (Bernardinelli-Bernstein)'s absolute magnitude is recorded as {'amount': '+6.0'}[17].
- C/2014 UN₂₇₁ (Bernardinelli-Bernstein)'s orbital inclination is recorded as {'unit': 'Q28390', 'amount': '+95.53688914567009'}[18].
- C/2014 UN₂₇₁ (Bernardinelli-Bernstein)'s orbital period is recorded as {'unit': 'Q573', 'amount': '+160754263.7385913'}[19].
- C/2014 UN₂₇₁ (Bernardinelli-Bernstein)'s longitude of ascending node is recorded as {'unit': 'Q28390', 'amount': '+190.0645451845533'}[20].
- C/2014 UN₂₇₁ (Bernardinelli-Bernstein)'s semi-major axis of an orbit is recorded as {'unit': 'Q1811', 'amount': '+5785.968290561134'}[21].
- C/2014 UN₂₇₁ (Bernardinelli-Bernstein)'s apoapsis is recorded as {'unit': 'Q1811', 'amount': '+11560.99762047213'}[22].
- C/2014 UN₂₇₁ (Bernardinelli-Bernstein)'s periapsis is recorded as {'unit': 'Q1811', 'amount': '+10.93896065013548'}[23].
- C/2014 UN₂₇₁ (Bernardinelli-Bernstein)'s argument of periapsis is recorded as {'unit': 'Q28390', 'amount': '+326.3780380646967'}[24].
- C/2014 UN₂₇₁ (Bernardinelli-Bernstein)'s mean anomaly is recorded as {'unit': 'Q28390', 'amount': '+359.989824116409'}[25].
- C/2014 UN₂₇₁ (Bernardinelli-Bernstein)'s diameter is recorded as {'unit': 'Q828224', 'amount': '+137'}[26].
- C/2014 UN₂₇₁ (Bernardinelli-Bernstein)'s Google Knowledge Graph ID is recorded as /g/11rgg89jxm[27].
Body
Works and Contributions
Credited discoveries include Pedro H. Bernardinelli[3], an astronomer[28], b. 1994[29], specialised in dark energy[30] and Gary Bernstein[4], an astronomer[31], specialised in dark energy[32].
Why It Matters
C/2014 UN₂₇₁ (Bernardinelli-Bernstein) ranks in the top 10% of non_periodic_comet entities by monthly Wikipedia readership (94 views/month).[2] C/2014 UN₂₇₁ (Bernardinelli-Bernstein) has Wikipedia articles in 14 language editions, a strong signal of global cultural recognition.[33] C/2014 UN₂₇₁ (Bernardinelli-Bernstein) is known by 23 alternative names across languages and contexts.[34]