1045 Michela

1045 Michela
Keşif[1]
KeşfedenG. van Biesbroeck
Keşif yeriYerkes Gözlemevi
Keşif tarihi19 Kasım 1924
Adlandırmalar
MPC belirtmesi(1045) Michela
Adın kaynağı
Micheline van Biesbroeck[2]
(kaşifin kızı)
Alternatif adlandırma
1924 TR · 1953 VB2
1964 XJ · 1976 AL
Asteroit kuşağı[1][3] · ()
Massalia[4]
Yörünge özellikleri[3]
Dönem 23 Mart 2018 (JG 2458200,5)
Belirsizlik parametresi 0
Gözlem yayı63,64 yıl (23,246 gün)
Günöte2,7348 AB
Günberi1,9811 AB
2,3580 AB
Dış merkezlik0,1598
3,62 yıl (1.323 gün)
259.96°
0° 16d 19.92s / gün
Eğiklik0,2648°
267,71°
166,97°
Fiziksel özellikler
SMASS = S[3]
13,0[3]
Ortalama çap
6,104±0,265 km[5]
0,328±0,077[5]

1045 Michela, geçici ismi 1924 TR, asteroit kuşağının iç bölgelerinden, yaklaşık 6 kilometre (3,7 mi) kilometre çapında taşlı bir Massalia asteroitidir. 19 Kasım 1924'te Belçikalı-Amerikalı astronom George Van Biesbroeck tarafından Williams Bay, Wisconsin, ABD'deki Yerkes Gözlemevi'nde keşfedilmiştir.[1] S-tipi asteroit, kaşifin kızı Micheline van Biesbroeck'in adını almıştır.[2]

Yörünge ve sınıflandırma

Michela, Massalia ailesinin (404) bir üyesidir, taşlı asteroitlerden oluşan çok büyük bir iç kuşak asteroit ailesidir.[6] İç ana kuşağında Güneş'in yörüngesinde 2,0–2,7 AB uzaklıkta; her 3 yıl ve 7 ayda bir (1.323 gün; 2,36 AB yarı büyük ekseni vardır). Yörüngesi, ekliptik ile ilgili olarak 0,16'lık bir eksantrikliğe ve 0 °'lik bir eğime sahiptir.[3]

Asteroidin gözlem yayı, Kasım 1953'te Goethe Link Gözlemevinde 1953 VB2 olarak gözlemlenmesiyle veya resmi keşif gözleminden 29 yıl sonra başlar.[1]

Fiziksel özellikler

SMASS sınıflandırmasında, Michela, Massalian asteroitleri için genel spektral tip olan yaygın, taşlı S tipi bir asteroittir.[6]:23

Çapı ve albedosu

NASA'nın Geniş Alan Kızılötesi Araştırma Gezgini'nin NEOWISE misyonu tarafından gerçekleştirilen araştırmaya göre, Michela 6,104 kilometre çapında ve yüzeyinin albedo değeri 0,328'dir.[5]

Rotasyon periyodu

2018 itibarıyla, fotometrik gözlemlerden Michela'nın dönme ışık eğrisi elde edilmemiştir. Gövdenin dönme periyodu, kutupları ve şekli bilinmemektedir.[3]

İsimlendirme

Bu küçük gezegen, adını kaşif George Van Biesbroeck'in kızı Micheline van Biesbroeck'ten almıştır. Resmi isimlendirme, 1955'te Paul Herget tarafından Küçük Gezegenlerin İsimleri'nde belirtilmiştir (H 99).[2]

Kaynakça

  1. ^ a b c d "1045 Michela (1924 TR)". Minor Planet Center. 3 Mart 2016 tarihinde kaynağından arşivlendi. Erişim tarihi: 20 Mart 2018. 
  2. ^ a b c Schmadel, Lutz D. (2007). "(1045) Michela". Dictionary of Minor Planet Names – (1045) Michela. Springer Berlin Heidelberg. s. 89. doi:10.1007/978-3-540-29925-7_1046. ISBN 978-3-540-00238-3. 
  3. ^ a b c d e f "JPL Small-Body Database Browser: 1045 Michela (1924 TR)" (2017-07-04 last obs.). Jet Propulsion Laboratory. 30 Ocak 2020 tarihinde kaynağından arşivlendi. Erişim tarihi: 20 Mart 2018. 
  4. ^ "Asteroid 1045 Michela – Nesvorny HCM Asteroid Families V3.0". Small Bodies Data Ferret. 3 Ekim 2020 tarihinde kaynağından arşivlendi. Erişim tarihi: 24 Ekim 2019. 
  5. ^ a b c Masiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Dailey, J.; Eisenhardt, P. R. M.; McMillan, R. S.; Spahr, T. B.; Skrutskie, M. F.; Tholen, D.; Walker, R. G.; Wright, E. L.; DeBaun, E.; Elsbury, D.; Gautier, T., IV; Gomillion, S.; Wilkins, A. (November 2011). "Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters". The Astrophysical Journal. 741 (2): 20. arXiv:1109.4096 $2. Bibcode:2011ApJ...741...68M. doi:10.1088/0004-637X/741/2/68. 9 Aralık 2019 tarihinde kaynağından arşivlendi. Erişim tarihi: 20 Mart 2018. 
  6. ^ a b Nesvorný, D.; Broz, M.; Carruba, V. (December 2014). Identification and Dynamical Properties of Asteroid Families. Asteroids IV. ss. 297-321. arXiv:1502.01628 $2. Bibcode:2015aste.book..297N. doi:10.2458/azu_uapress_9780816532131-ch016. ISBN 9780816532131. 

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