Q15202665

Summary

Q15202665 is an asteroid^[1].

Key Facts

• Q15202665 is credited with the discovery of Cornelis Johannes van Houten^[2].
• Q15202665 is credited with the discovery of Ingrid van Houten-Groeneveld^[3].
• Q15202665 is credited with the discovery of Tom Gehrels^[4].
• Q15202665's instance of is recorded as asteroid^[5].
• Q15202665's site of astronomical discovery is recorded as Palomar Observatory^[6].
• Q15202665's follows is recorded as Q15202664^[7].
• Q15202665's followed by is recorded as Q15202667^[8].
• Q15202665's minor planet group is recorded as asteroid belt^[9].
• Q15202665's parent astronomical body is recorded as Sun^[10].
• Q15202665's provisional designation is recorded as 2499 T-3^[11].
• Q15202665's provisional designation is recorded as 2000 FZ70^[12].
• Q15202665's provisional designation is recorded as 1997 SK24^[13].
• Q15202665's time of discovery or invention is recorded as +1977-10-16T00:00:00Z^[14].
• Q15202665's JPL Small-Body Database SPK-ID is recorded as 20079063^[15].
• Q15202665's orbital eccentricity is recorded as {'unit': '1', 'amount': '+0.07283805583064251'}^[16].
• Q15202665's absolute magnitude is recorded as {'unit': '1', 'amount': '+15.41'}^[17].
• Q15202665's orbital inclination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+1.902067923437215'}^[18].
• Q15202665's orbital period is recorded as {'unit': 'http://www.wikidata.org/entity/Q573', 'amount': '+1815.280178264947'}^[19].
• Q15202665's rotation period is recorded as {'unit': 'http://www.wikidata.org/entity/Q25235', 'amount': '+3.32'}^[20].
• Q15202665's longitude of ascending node is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+334.5721670182132'}^[21].
• Q15202665's semi-major axis of an orbit is recorded as {'unit': 'http://www.wikidata.org/entity/Q1811', 'amount': '+2.912260092877523'}^[22].
• Q15202665's apoapsis is recorded as {'unit': 'http://www.wikidata.org/entity/Q1811', 'amount': '+3.124383456115888'}^[23].
• Q15202665's periapsis is recorded as {'unit': 'http://www.wikidata.org/entity/Q1811', 'amount': '+2.700136729639158'}^[24].
• Q15202665's argument of periapsis is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+330.8525809175309'}^[25].
• Q15202665's mean anomaly is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+227.8951208245696'}^[26].

Body

Works and Contributions

Credited discoveries include Cornelis Johannes van Houten^[2], an astronomer^[27], 1920–2002^[28], of Kingdom of the Netherlands^[29], specialised in astronomy^[30]; Ingrid van Houten-Groeneveld^[3], an astronomer^[31], 1921–2015^[32], of Kingdom of the Netherlands^[33], specialised in astronomy^[34]; and Tom Gehrels^[4], an astronomer^[35], 1925–2011^[36], of Kingdom of the Netherlands^[37], awarded the Masursky Award^[38], specialised in astronomy^[39].