8595 Dougallii

Summary

8595 Dougallii is an asteroid^[1]. It has Wikipedia articles in 21 language editions, a strong signal of global cultural recognition.^[2]

Key Facts

• 8595 Dougallii is credited with the discovery of Cornelis Johannes van Houten^[3].
• 8595 Dougallii is credited with the discovery of Ingrid van Houten-Groeneveld^[4].
• 8595 Dougallii is credited with the discovery of Tom Gehrels^[5].
• 8595 Dougallii's instance of is recorded as asteroid^[6].
• 8595 Dougallii's site of astronomical discovery is recorded as Palomar Observatory^[7].
• Roseate Tern is named after 8595 Dougallii^[8].
• 8595 Dougallii's follows is recorded as Q426864^[9].
• 8595 Dougallii's followed by is recorded as Q550085^[10].
• 8595 Dougallii's minor planet group is recorded as asteroid belt^[11].
• 8595 Dougallii's parent astronomical body is recorded as Sun^[12].
• 8595 Dougallii's provisional designation is recorded as 1980 FX2^[13].
• 8595 Dougallii's provisional designation is recorded as 3233 T-1^[14].
• 8595 Dougallii's time of discovery or invention is recorded as +1971-03-26T00:00:00Z^[15].
• 8595 Dougallii's Freebase ID is recorded as /m/03y1h07^[16].
• 8595 Dougallii's JPL Small-Body Database SPK-ID is recorded as 20008595^[17].
• 8595 Dougallii's significant event is recorded as naming^[18].
• 8595 Dougallii's orbital eccentricity is recorded as {'unit': '1', 'amount': '+0.13'}^[19].
• 8595 Dougallii's orbital eccentricity is recorded as {'unit': '1', 'amount': '+0.1330655'}^[20].
• 8595 Dougallii's orbital eccentricity is recorded as {'unit': '1', 'amount': '+0.1335570341995653'}^[21].
• 8595 Dougallii's absolute magnitude is recorded as {'unit': '1', 'amount': '+14.2'}^[22].
• 8595 Dougallii's absolute magnitude is recorded as {'unit': '1', 'amount': '+14.36'}^[23].
• 8595 Dougallii's orbital inclination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+7.32535'}^[24].
• 8595 Dougallii's orbital inclination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+7.320606382316551'}^[25].
• 8595 Dougallii's orbital period is recorded as {'unit': 'http://www.wikidata.org/entity/Q577', 'amount': '+4.57'}^[26].
• 8595 Dougallii's orbital period is recorded as {'unit': 'http://www.wikidata.org/entity/Q573', 'amount': '+1667.559227759168'}^[27].

Body

Works and Contributions

Credited discoveries include Cornelis Johannes van Houten^[3], an astronomer^[28], 1920–2002^[29], of Kingdom of the Netherlands^[30], specialised in astronomy^[31]; Ingrid van Houten-Groeneveld^[4], an astronomer^[32], 1921–2015^[33], of Kingdom of the Netherlands^[34], specialised in astronomy^[35]; and Tom Gehrels^[5], an astronomer^[36], 1925–2011^[37], of Kingdom of the Netherlands^[38], awarded the Masursky Award^[39], specialised in astronomy^[40].

Why It Matters

8595 Dougallii has Wikipedia articles in 21 language editions, a strong signal of global cultural recognition.^[2]