63 Ausonia

63 Ausonia
Keşif [1][2]
KeşfedenA. de Gasparis
Keşif yeriCapodimonte Göz.
Keşif tarihi10 Şubat 1861
Adlandırmalar
MPC belirtmesi(63) Ausonia
Telaffuz/ɔːˈsoʊniə/[3]
Adın kaynağı
Ausonia [4]
(İtalya'nın eski adı)
Alternatif adlandırma
1947 NA · 1948 WT
Asteroit kuşağı · (iç)
Vesta [5][6]
SıfatlarAusonian /ɔːˈsoʊniən/[7]
Yörünge özellikleri [1]
Dönem 4 Eylül 2017 (JG 2458000.5)
Belirsizlik parametresi 0
Gözlem yayı156.34 yıl (57,104 gün)
Günöte2.6993 AB
Günberi2.0910 AU
2.3951 AU
Dış merkezlik0.1270
340.16°
0° 15d 57.24s / gün
Eğiklik5.7763°
337.75°
295.78°
Fiziksel özellikler
Tholen = S [1]
SMASS = Sa [1]
S [5][8]
B–V = 0.916[1]
U–B = 0.500[1]
7.55[9][10][11][1][5][12][13]
Boyutlarc/a = 0,45±0,02[14]
Ortalama çap
93±3 km[14] 87,5±1,1 km[9]
90±18 km[15]
94,4±7,2 km[16]
103,0±2,8 km[10]
103,14±2,4 km[11]
Kütle(1,2±0,2)×1018 kg[14]
(1,53±0,15)×1018 kg[16]
Ortalama yoğunluk
2,96±0,61 g/cm3[14]
3,46±0,86 g/cm3[16]
9,282±0,003 h[17]
9,29 h[18]
9,293±0,001 h[19]
9,294 h[20]
9,29757 h[21]
9,29758 h[22]
9,29759 h[15][23]
9,29766 h[24]
9,298 h[25]
9,299 h[26]
0.195 (calculated)[14]
0,125±0,016[13]
0,1586±0,008[11]
0,1591±0,0277[10]
0,232±0,008[9]
0,25±0,18[12]
  Wikimedia Commons'ta ilgili ortam

Ausonia (küçük gezegen tanımı: 63 Ausonia), asteroit kuşağının iç bölgesinden, yaklaşık 100 kilometre (60 mil) çapında, taşlı bir Vestian asteroididir. İtalyan gök bilimci Annibale de Gasparis tarafından 10 Şubat 1861'de İtalya'nın Napoli kentindeki Capodimonte Astronomik Gözlemevi'nden keşfedildi. Asteroit için ilk isim seçimi İtalya'dan sonra "Italia" idi, ancak bu, İtalyan bölgesi için eski bir klasik isim olan Ausonia olarak değiştirildi.

Ausonia'nın Işık eğrisi tabanlı 3B modeli

Yörünge ve sınıflandırma

Ausonia, Vesta ailesinin bir üyesidir. Vestian asteroitlerinin kümülatif ökritlere (HED göktaşları) benzer bir bileşimi vardır ve Vesta'nın kabuğunun derinliklerinde, muhtemelen Güney kutbuna yakın güney yarımkürede büyük bir çarpışma krateri olan Rheasilvia kraterinden kaynaklandığı düşünülmektedir. bir yarı-felaket çarpışmasının. Vesta, Ceres'ten sonra ana kuşağın ikinci en büyük ve ikinci en büyük gövdesidir.[27][28]

İç asteroit kuşağında 2,1–2,7 uzaklıkta Güneş'in yörüngesinde döner. AB her 3 yıl 9 ayda bir (1.354 gün; yarı ana eksen 2.40) AÜ). Yörüngesi ekliptiğe göre 0.13 eksantrikliğe ve 6 °'lik bir eğime sahiptir.

Fiziksel özellikler

Tholen sınıflandırmasında, Ausonia taşlı bir S-tipi asteroitken, SMASS sınıflandırmasında, S-tipinden nadir görülen A-tipi asteroide geçiş yapan bir S-alt tipidir. Vücudun taşlı yapısı 2017 yılında yapılan polarimetrik gözlemlerle de doğrulanmıştır. Işık eğrisine dayanarak, küçük bir ay önerildi, ancak asla onaylanmadı.[29]

Kızılötesi Astronomik Uydu IRAS, Japon Akari uydusu ve NASA'nın Geniş Alan Kızılötesi Araştırma Kaşifi'nin NEOWISE misyonu tarafından yapılan araştırmalara göre, Ausonia'nın çapı 87.47 ile 116.044 kilometre arasında ve yüzeyi 0.125 ile 0.25 arasında bir yansıtabiliriğe sahip. İşbirlikçi Asteroit Işık Eğrisi Bağlantısı, 7,55 mutlak kadire dayalı olarak 0,2082'lik bir yansıtabilirlik ve 90 kilometrelik bir çap elde ediyor.

Ausonia, Hubble FGS kullanan bir çalışmadaydı. İncelenen diğer asteroitler arasında 15 Eunomia, 43 Ariadne, 44 Nysa ve 624 Hektor yer alıyor.[30] 1976'da Ausonia, İtalya'daki Torino Gözlemevi tarafından bir fotometrik çalışmanın konusu oldu. Ausonia'nın bir ışık eğrisi, 1980 yılında La Silla Gözlemevi'ndeki ESO 0,5 metrelik teleskopla elde edildi.[31]

Kaynakça

  1. ^ a b c d e f g "JPL Small-Body Database Browser: 63 Ausonia" (2017-07-05 last obs.). Jet Propulsion Laboratory. 15 Aralık 2019 tarihinde kaynağından arşivlendi. Erişim tarihi: 3 Şubat 2018. 
  2. ^ "63 Ausonia". Minor Planet Center. 3 Şubat 2011 tarihinde kaynağından arşivlendi. Erişim tarihi: 3 Şubat 2018. 
  3. ^ Noah Webster (1884) A Practical Dictionary of the English Language
  4. ^ Schmadel, Lutz D. (2007). Dictionary of Minor Planet Names – (63) Ausonia. Springer Berlin Heidelberg. s. 21. ISBN 978-3-540-00238-3. 25 Aralık 2021 tarihinde kaynağından arşivlendi. Erişim tarihi: 3 Şubat 2018. 
  5. ^ a b c "LCDB Data for (63) Ausonia". Asteroid Lightcurve Database (LCDB). 18 Şubat 2020 tarihinde kaynağından arşivlendi. Erişim tarihi: 3 Şubat 2018. 
  6. ^ "Asteroid 63 Ausonia". Small Bodies Data Ferret. 15 Eylül 2020 tarihinde kaynağından arşivlendi. Erişim tarihi: 24 Ekim 2019. 
  7. ^ "Ausonian." Oxford Dictionary of English 2e, Oxford University Press, 2003.
  8. ^ Belskaya, I. N.; Fornasier, S.; Tozzi, G. P.; Gil-Hutton, R.; Cellino, A.; Antonyuk, K.; Krugly, Yu. N.; Dovgopol, A. N.; Faggi, S. (March 2017). "Refining the asteroid taxonomy by polarimetric observations". Icarus. 284: 30-42. Bibcode:2017Icar..284...30B. doi:10.1016/j.icarus.2016.11.003. hdl:11336/63617. 
  9. ^ a b c Usui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; Ishihara, Daisuke; Kataza, Hirokazu; Takita, Satoshi; Oyabu, Shinki; Ueno, Munetaka; Matsuhara, Hideo; Onaka, Takashi (October 2011). "Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey". Publications of the Astronomical Society of Japan. 63 (5): 1117-1138. Bibcode:2011PASJ...63.1117U. doi:10.1093/pasj/63.5.1117.  (online, AcuA catalog p. 153 25 Mart 2019 tarihinde Wayback Machine sitesinde arşivlendi.)
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  11. ^ a b c Tedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004). "IRAS Minor Planet Survey V6.0". NASA Planetary Data System. 12: IRAS-A-FPA-3-RDR-IMPS-V6.0. Bibcode:2004PDSS...12.....T. 14 Haziran 2018 tarihinde kaynağından arşivlendi. Erişim tarihi: 22 Ekim 2019. 
  12. ^ a b Nugent, C. R.; Mainzer, A.; Masiero, J.; Bauer, J.; Cutri, R. M.; Grav, T.; Kramer, E.; Sonnett, S.; Stevenson, R.; Wright, E. L. (December 2015). "NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos". The Astrophysical Journal. 814 (2): 13. arXiv:1509.02522 $2. Bibcode:2015ApJ...814..117N. doi:10.1088/0004-637X/814/2/117. 
  13. ^ a b Masiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Nugent, C.; Cabrera, M. S. (November 2012). "Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids". The Astrophysical Journal Letters. 759 (1): 5. arXiv:1209.5794 $2. Bibcode:2012ApJ...759L...8M. doi:10.1088/2041-8205/759/1/L8. 
  14. ^ a b c d e P. Vernazza et al. (2021) VLT/SPHERE imaging survey of the largest main-belt asteroids: Final results and synthesis. Astronomy & Astrophysics 54, A56
  15. ^ a b Durech, Josef; Kaasalainen, Mikko; Herald, David; Dunham, David; Timerson, Brad; Hanus, Josef; Frappa, Eric; Talbot, John; Hayamizu, Tsutomu; Warner, Brian D.; Pilcher, Frederick; Galád, Adrián (August 2011). "Combining asteroid models derived by lightcurve inversion with asteroidal occultation silhouettes". Icarus. 214 (2): 652-670. arXiv:1104.4227 $2. Bibcode:2011Icar..214..652D. doi:10.1016/j.icarus.2011.03.016. 
  16. ^ a b c Carry, B. (December 2012), "Density of asteroids", Planetary and Space Science, 73 (1), ss. 98-118, arXiv:1203.4336 $2, Bibcode:2012P&SS...73...98C, doi:10.1016/j.pss.2012.03.009  See Table 1.
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  19. ^ Behrend, Raoul. "Asteroids and comets rotation curves – (63) Ausonia". Geneva Observatory. 3 Aralık 2002 tarihinde kaynağından arşivlendi. Erişim tarihi: 3 Şubat 2018. 
  20. ^ Lupishko, D. F.; Velichko, F. P. (February 1987). "The sense of rotation of asteroids 21, 63, 216, and 349". Kinematika I Fizika Nebesnykh Tel. 3: 57-65.InRussian. Bibcode:1987KFNT....3...57L. ISSN 0233-7665. 
  21. ^ Magnusson, P. (October 1986). "Distribution of spin axes and senses of rotation for 20 large asteroids". Icarus. 68 (1): 1-39. Bibcode:1986Icar...68....1M. doi:10.1016/0019-1035(86)90072-2. ISSN 0019-1035. 
  22. ^ De Angelis, G. (May 1995). "Asteroid spin, pole and shape determinations". Planetary and Space Science. 43 (5): 649-682. Bibcode:1995P&SS...43..649D. doi:10.1016/0032-0633(94)00151-G. 
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