74P/Smirnova–Chernykh

Summary

74P/Smirnova–Chernykh is a quasi-Hilda comet^[1]. 74P/Smirnova–Chernykh draws 4 Wikipedia views per month (quasi_hilda_comet category, ranking #1 of 2).^[2]

Key Facts

• 74P/Smirnova–Chernykh is credited with the discovery of Tamara Smirnova^[3].
• 74P/Smirnova–Chernykh is credited with the discovery of Nikolai Chernykh^[4].
• 74P/Smirnova–Chernykh's image is recorded as 74p-2010Jan25-12UT.jpg^[5].
• 74P/Smirnova–Chernykh's instance of is recorded as quasi-Hilda comet^[6].
• 74P/Smirnova–Chernykh's instance of is recorded as periodic comet^[7].
• 74P/Smirnova–Chernykh's instance of is recorded as Encke-type comet^[8].
• 74P/Smirnova–Chernykh's parent astronomical body is recorded as Sun^[9].
• 74P/Smirnova–Chernykh's provisional designation is recorded as 1992 XXI^[10].
• 74P/Smirnova–Chernykh's provisional designation is recorded as 1984 V^[11].
• 74P/Smirnova–Chernykh's provisional designation is recorded as 74P/1975 E2^[12].
• 74P/Smirnova–Chernykh's provisional designation is recorded as 1975 VII^[13].
• 74P/Smirnova–Chernykh's provisional designation is recorded as 74P/1967 EU^[14].
• 74P/Smirnova–Chernykh's provisional designation is recorded as 1967 XV^[15].
• 74P/Smirnova–Chernykh's time of discovery or invention is recorded as +1975-03-04T00:00:00Z^[16].
• 74P/Smirnova–Chernykh's Freebase ID is recorded as /m/0b722b^[17].
• 74P/Smirnova–Chernykh's JPL Small-Body Database SPK-ID is recorded as 1000088^[18].
• 74P/Smirnova–Chernykh's orbital eccentricity is recorded as {'amount': '+0.1477215183767737'}^[19].
• 74P/Smirnova–Chernykh's absolute magnitude is recorded as {'amount': '+6.8'}^[20].
• 74P/Smirnova–Chernykh's orbital inclination is recorded as {'unit': 'Q28390', 'amount': '+6.651038807537222'}^[21].
• 74P/Smirnova–Chernykh's orbital period is recorded as {'unit': 'Q573', 'amount': '+3105.351200937866'}^[22].
• 74P/Smirnova–Chernykh's longitude of ascending node is recorded as {'unit': 'Q28390', 'amount': '+77.08419922220791'}^[23].
• 74P/Smirnova–Chernykh's semi-major axis of an orbit is recorded as {'unit': 'Q1811', 'amount': '+4.165574103436561'}^[24].
• 74P/Smirnova–Chernykh's apoapsis is recorded as {'unit': 'Q1811', 'amount': '+4.780919034907178'}^[25].
• 74P/Smirnova–Chernykh's periapsis is recorded as {'unit': 'Q1811', 'amount': '+3.550229171965944'}^[26].
• 74P/Smirnova–Chernykh's argument of periapsis is recorded as {'unit': 'Q28390', 'amount': '+86.57844422575022'}^[27].

Body

Works and Contributions

Credited discoveries include Tamara Smirnova^[3], an astronomer^[28], 1935–2001^[29], of Soviet Union^[30], specialised in astronomy^[31] and Nikolai Chernykh^[4], an astronomer^[32], 1931–2004^[33], of Soviet Union^[34], specialised in astronomy^[35].

Why It Matters

74P/Smirnova–Chernykh draws 4 Wikipedia views per month (quasi_hilda_comet category, ranking #1 of 2).^[2] 74P/Smirnova–Chernykh has Wikipedia articles in 10 language editions, a strong signal of global cultural recognition.^[36]