148 Gallia

148 Gallia
Keşif[1]
KeşfedenP. M. Henry
Keşif yeriParis
Keşif tarihi7 Ağustos 1875
Adlandırmalar
MPC belirtmesi(148) Gallia
Telaffuz/ˈɡæliə/[2]
Adın kaynağı
Γαλλία Gallia (Galya)[3]
Fransa, (Latince)
Alternatif adlandırma
A875 PA
Asteroit kuşağı[1][4] · (orta)
Gallia[5]
Yörünge özellikleri[4]
Dönem 23 Mart 2018 (JG 2.458.200,5)
Belirsizlik parametresi 0
Gözlem yayı138,37 yıl (50.540 gün)
Günöte3,2885 AB
Günberi2,2531 AB
2,7708 AB
Dış merkezlik0,1868
4,61 yıl (1.685 gün)
278,58°
0° 12d 49.32s / gün
Eğiklik25,291°
145,01°
252,79°
Fiziksel özellikler
Tholen = GU[4]
SMASS = S[4][6]
B–V = 0,858[4]
U–B = 0,423[4]
6,97±0,84[7]
7,4[6]
7,4±0,1[8][9]
7,63[4][10][11]
7,67[12]
7,72±0,10[13]
Ortalama çap
80,87±1,04 km[10]
83,45±5,07 km[14]
85,91±23,39 km[12]
97,75±3,7 km[11]
98,09 km (türetilmiş)[6]
Kütle(4,89±1,67)×1018 kg[14]
Ortalama yoğunluk
16,06±6,22 g/cm3[14]
20,6592±0,0007 sa[15]
20,66±0,01 sa[15]
20,664 sa[16]
20,665266 sa[a]
20,666±0,002 sa[17][b]
0,1640±0,013[11]
0,2013 (türetilmiş)[6]
0,21±0,12[12]
0,240±0,008[10]
  Wikimedia Commons'ta ilgili ortam

Gallia (Küçük gezegen tanımı: 148 Gallia), asteroit kuşağının merkez bölgelerinde yer alan, yaklaşık 90 kilometre (56 mil) çapında bir asteroittir.

Keşfi ve adlandırma

7 Ağustos 1875'te Fransız kardeşler Paul Henry ve Prosper Henry kardeşler tarafından Paris'te keşfedildi.[1] Adını Fransa ülkesinin Latince adı Galya'dan almıştır.[3]

Sınıflandırma

Spektrumuna bağlı olarak, sırasıyla Tholen ve SMASS sınıflandırmasında olağandışı bir G-tipi asteroit (GU) ve taşlı bir S-tipi asteroittir.[4][18] 1977-78'de Avrupa Güney Gözlemevi'nde bu asteroidin fotometrik gözlemleri, 0,86098 ± 0,00030 gün (20,6635 ± 0,0072 sa) günlük periyotlu bir ışık eğrisi ve 0,32 büyüklüğünde bir parlaklık değişimi verdiği gözlemlendi.[16][17][b] Ayrıca 200 taşlı asteroitten oluşan küçük bir aile olan Gallia ailesinin (802) bir üyesidir.[19][20]

Notlar

  1. ^ Warner (2011) web: modellenen ışık eğrisi, 20,665266 saatlik bir dönüş periyodu vermiştir. Summary figures for (148) Gallia at the LCDB
  2. ^ a b Lightcurve plot of 148 Gallia, Palmer Divide Observatory, B. D. Warner (2007): rotation period 20,666±0,002 hours with a brightness amplitude of 0,21±0,02 mag. Quality code of 2+. Summary figures at the LCDB

Kaynakça

  1. ^ a b c "148 Gallia". Minor Planet Center. 3 Şubat 2011 tarihinde kaynağından arşivlendi. Erişim tarihi: 18 Nisan 2018. 
  2. ^ Noah Webster (1884) A Practical Dictionary of the English Language
  3. ^ a b Schmadel, Lutz D. (2007). "(148) Gallia". Dictionary of Minor Planet Names – (148) Gallia. Springer Berlin Heidelberg. s. 29. doi:10.1007/978-3-540-29925-7_149. ISBN 978-3-540-00238-3. 
  4. ^ a b c d e f g h "JPL Small-Body Database Browser: 148 Gallia" (2017-10-28 last obs.). Jet Propulsion Laboratory. 20 Ağustos 2020 tarihinde kaynağından arşivlendi. Erişim tarihi: 18 Nisan 2018. 
  5. ^ "Asteroid 148 Gallia". Small Bodies Data Ferret. 20 Ağustos 2020 tarihinde kaynağından arşivlendi. Erişim tarihi: 24 Ekim 2019. 
  6. ^ a b c d "LCDB Data for (148) Gallia". Asteroid Lightcurve Database (LCDB). 18 Şubat 2020 tarihinde kaynağından arşivlendi. Erişim tarihi: 18 Nisan 2018. 
  7. ^ Veres, Peter; Jedicke, Robert; Fitzsimmons, Alan; Denneau, Larry; Granvik, Mikael; Bolin, Bryce; Chastel, Serge; Wainscoat, Richard J.; Burgett, William S.; Chambers, Kenneth C.; Flewelling, Heather; Kaiser, Nick; Magnier, Eugen A.; Morgan, Jeff S.; Price, Paul A.; Tonry, John L.; Waters, Christopher (Kasım 2015). "Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results". Icarus. 261: 34-47. arXiv:1506.00762 $2. Bibcode:2015Icar..261...34V. doi:10.1016/j.icarus.2015.08.007. 
  8. ^ Harris, A. W.; Young, J. W.; Dockweiler, Thor; Gibson, J.; Poutanen, M.; Bowell, E. (January 1992). "Asteroid lightcurve observations from 1981". Icarus. 95 (1): 115-147.ResearchsupportedbyLowellObservatoryEndowmentandNASA. Bibcode:1992Icar...95..115H. doi:10.1016/0019-1035(92)90195-D. ISSN 0019-1035. Erişim tarihi: 18 Nisan 2018. 
  9. ^ Pravec, Petr; Harris, Alan W.; Kusnirák, Peter; Galád, Adrián; Hornoch, Kamil (Eylül 2012). "Absolute magnitudes of asteroids and a revision of asteroid albedo estimates from WISE thermal observations". Icarus. 221 (1): 365-387. Bibcode:2012Icar..221..365P. doi:10.1016/j.icarus.2012.07.026. 8 Haziran 2020 tarihinde kaynağından arşivlendi. Erişim tarihi: 18 Nisan 2018. 
  10. ^ 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 (Ekim 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.)
  11. ^ a b c Tedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (Ekim 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 c Nugent, C. R.; Mainzer, A.; Bauer, J.; Cutri, R. M.; Kramer, E. A.; Grav, T.; Masiero, J.; Sonnett, S.; Wright, E. L. (Eylül 2016). "NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos". The Astronomical Journal. 152 (3): 12. arXiv:1606.08923 $2. Bibcode:2016AJ....152...63N. doi:10.3847/0004-6256/152/3/63. 
  13. ^ Warner, Brian D. (Aralık 2007). "Initial Results of a Dedicated H-G Project". The Minor Planet Bulletin. 34 (4): 113-119. Bibcode:2007MPBu...34..113W. ISSN 1052-8091. Erişim tarihi: 18 Nisan 2018. 
  14. ^ 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  Tablo 1'e bakın.
  15. ^ a b Behrend, Raoul. "Asteroids and comets rotation curves – (148) Gallia". Geneva Observatory. 3 Aralık 2002 tarihinde kaynağından arşivlendi. Erişim tarihi: 18 Nisan 2018. 
  16. ^ a b Surdej, A.; Surdej, J. (Eylül 1979). "Photoelectric lightcurves and rotation period of the minor planet 148 Gallia". Astronomy and Astrophysics Supplement Series. 37: 471-474. Bibcode:1979A&AS...37..471S. Erişim tarihi: 18 Nisan 2018. 
  17. ^ a b Warner, Brian D. (December 2007). "Asteroid Lightcurve Analysis at the Palmer Divide Observatory - Mart–Mayıs 2007". The Minor Planet Bulletin. 34 (4): 104-107. Bibcode:2007MPBu...34..104W. ISSN 1052-8091. Erişim tarihi: 18 Nisan 2018. 
  18. ^ Lazzaro, D.; Angeli, C. A.; Carvano, J. M.; Mothé-Diniz, T.; Duffard, R.; Florczak, M. (Kasım 2004). "S 3OS 2: the visible spectroscopic survey of 820 asteroids". Icarus. 172 (1): 179-220. Bibcode:2004Icar..172..179L. doi:10.1016/j.icarus.2004.06.006. Erişim tarihi: 18 Nisan 2018. 
  19. ^ Novakovic, Bojan; Cellino, Alberto; Knezevic, Zoran (Kasım 2011). "Families among high-inclination asteroids". Icarus. 216 (1): 69-81. arXiv:1108.3740 $2. Bibcode:2011Icar..216...69N. doi:10.1016/j.icarus.2011.08.016. 
  20. ^ Nesvorný, D.; Broz, M.; Carruba, V. (Aralık 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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