Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

89 Julia

From Wikipedia, the free encyclopedia
Main-belt asteroid

89 Julia
VLT-SPHERE image of Julia. The large crater Nonza, half the diameter of the asteroid, is centered on the upper left quadrant.
Discovery
Discovered byÉdouard Stephan
Discovery date6 August 1866
Designations
(89) Julia
Pronunciation/ˈliə/[1]
Named after
Julia of Corsica
Main belt
AdjectivesJulian/ˈliən/
Orbital characteristics[2]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc149.68 yr (54672 d)
Aphelion3.0202 AU (451.82 Gm)
Perihelion2.08017 AU (311.189 Gm)
2.55016 AU (381.499 Gm)
Eccentricity0.18430
4.07yr (1487.5d)
255.367°
0° 14m 31.272s / day
Inclination16.128°
311.563°
45.461°
Physical characteristics
Dimensions(89±2)×(80±1)×(62±3) km[3]
140±km[3][4]
151±3 km[2]
148±8 km[5]
Flattening0.30[a]
Mass(4.3±3.2)×1018 kg[4]
(4.3±3.6)×1018 kg[3]
(6.7±1.8)×1018 kg[5]
3.0±2.2 g/cm3[4]
3.0±2.6 g/cm3[3]
4.0±1.3 g/cm3[5]
11.388336±0.000001 h (0.4745 day)[3]
0.216 (calculated)[4]
0.1764±0.007[2]
0.176[6]
S
8.74 to 12.61[7]
6.37[2]
0.18" to 0.052"

89 Julia is a largemain-beltasteroid that was discovered by French astronomerÉdouard Stephan on 6 August 1866. This was first of his two asteroid discoveries; the other was91 Aegina. 89 Julia is believed to be named after SaintJulia of Corsica. Astellaroccultation by Julia was observed on 20 December 1985.

The spectrum of 89 Julia shows the signature ofsilicate rich minerals with possible indications of an abundant calcicclinopyroxene component. It is classified as anS-type asteroid. The asteroid has an estimated diameter of151.4±3.1 km.[8]Photometry from the Oakley Observatory during 2006 produced alightcurve that indicated asidereal rotation period of11.38±0.01 with anamplitude of0.20±0.02 in magnitude.[9]

Nonza crater and Julian family

[edit]

89 Julia is the parent body of the eponymousJulia family of asteroids. Observations of 89 Julia by theVLT's SPHERE instrument identified a 'highly probable' crater 70–80 km in diameter and4.1±1.7 km deep in the southern hemisphere as the only visible possible source of the family.[10] The crater was named Nonza by the discoverers, referring to thecommune on the island of Corsica where Saint Julia was born.[11] The excavated volume is on the order of 5,000 to15000 km3. It is hypothesized an impact 30 to 120 million years ago by another body approximately 8 kilometers in diameter may have created the collisional family.

Notes

[edit]
  1. ^Flattening derived from the maximum aspect ratio (c/a):f=1ca{\displaystyle f=1-{\frac {c}{a}}}, where (c/a) =0.70±0.03.[4]

References

[edit]
  1. ^Noah Webster (1884)A Practical Dictionary of the English Language
  2. ^abcdYeomans, Donald K.,"89 Julia",JPL Small-Body Database Browser,NASA Jet Propulsion Laboratory, retrieved13 May 2016.
  3. ^abcdeVernazza et al. (August 2018) The impact crater at the origin of the Julia family detected with VLT/SPHERE?,Astronomy and Astrophysics 618, DOI: 10.1051/0004-6361/201833477
  4. ^abcdeP. Vernazza et al. (2021) VLT/SPHERE imaging survey of the largest main-belt asteroids: Final results and synthesis.Astronomy & Astrophysics 54, A56
  5. ^abcCarry, B. (December 2012), "Density of asteroids",Planetary and Space Science,73 (1):98–118,arXiv:1203.4336,Bibcode:2012P&SS...73...98C,doi:10.1016/j.pss.2012.03.009. See Table 1.
  6. ^Asteroid Data SetsArchived 2009-12-17 at theWayback Machine
  7. ^"AstDys (89) Julia Ephemerides". Department of Mathematics, University of Pisa, Italy. Retrieved27 June 2010.
  8. ^Birlan, Mirel; Barucci, Maria Antonietta; Vernazza, Pierre; Fulchignoni, Marcello; Binzel, Richard P.; Bus, Schelte J.; et al. (June 2004). "Near-IR spectroscopy of asteroids 21 Lutetia, 89 Julia, 140 Siwa, 2181 Fogelin and 5480 (1989YK8), potential targets for the Rosetta mission; remote observations campaign on IRTF".New Astronomy.9 (5):343–351.arXiv:astro-ph/0312638.Bibcode:2004NewA....9..343B.doi:10.1016/j.newast.2003.12.005.
  9. ^Ditteon, Richard; Hawkins, Scot (September 2007), "Asteroid Lightcurve Analysis at the Oakley Observatory - October-November 2006",The Minor Planet Bulletin,34 (3):59–64,Bibcode:2007MPBu...34...59D,ISSN 1052-8091.
  10. ^Vernazza, P.; Broz, M.; Drouard, A."Astronomy & Astrophysics (A&A)".www.aanda.org. Retrieved20 December 2019.
  11. ^Vernazza, P."ESO/VLT/SPHERE Survey of D>100km Asteroids : First Results"(PDF).USRA. Retrieved20 December 2019.

External links

[edit]
Minor planets
Asteroid
Distant minor planet
Comets
Other
Authority control databasesEdit this at Wikidata
Retrieved from "https://en.wikipedia.org/w/index.php?title=89_Julia&oldid=1294080633"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2025 Movatter.jp