2025 DB51

Summary

2025 DB51 is a centaur^[1].

Key Facts

• 2025 DB51's instance of is recorded as centaur^[2].
• 2025 DB51's instance of is recorded as trans-Neptunian object^[3].
• 2025 DB51's instance of is recorded as asteroid^[4].
• 2025 DB51's minor planet group is recorded as trans-Neptunian object^[5].
• 2025 DB51's parent astronomical body is recorded as Sun^[6].
• 2025 DB51's JPL Small-Body Database SPK-ID is recorded as 54524119^[7].
• 2025 DB51's orbital eccentricity is recorded as {'unit': '1', 'amount': '+0.9726596910862013'}^[8].
• 2025 DB51's absolute magnitude is recorded as {'unit': '1', 'amount': '+10.32'}^[9].
• 2025 DB51's orbital inclination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+104.7426563787977'}^[10].
• 2025 DB51's orbital period is recorded as {'unit': 'http://www.wikidata.org/entity/Q573', 'amount': '+4081090.808614914'}^[11].
• 2025 DB51's longitude of ascending node is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+357.1598195343583'}^[12].
• 2025 DB51's semi-major axis of an orbit is recorded as {'unit': 'http://www.wikidata.org/entity/Q1811', 'amount': '+499.7873055929526'}^[13].
• 2025 DB51's apoapsis is recorded as {'unit': 'http://www.wikidata.org/entity/Q1811', 'amount': '+985.9102718597989'}^[14].
• 2025 DB51's periapsis is recorded as {'unit': 'http://www.wikidata.org/entity/Q1811', 'amount': '+13.66433932610643'}^[15].
• 2025 DB51's argument of periapsis is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+109.0168998996368'}^[16].
• 2025 DB51's mean anomaly is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+0.1234766846221598'}^[17].
• 2025 DB51's epoch is recorded as November 21, 2025^[18].
• 2025 DB51's time of periapsis is recorded as {'unit': 'http://www.wikidata.org/entity/Q14267', 'amount': '+2459600.723436973'}^[19].