596 Scheila

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596 Scheila
596 Scheila, 5 minute exposure, Dec. 12, 2010.jpg
596 Scheila outbursting as seen in a 5 min photo with a 24" telescope
Discovery [1]
Discovered by August Kopff
Discovery site Heidelberg Observatory
Discovery date21 February 1906
Designations
(596) Scheila
Pronunciation /ˈʃiːlə/
Named after
 Sheila
main-belt [1]
main-belt comet [2]
Orbital characteristics   [1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc 111.19 yr (40,611 days)
Aphelion 3.4062 AU
Perihelion 2.4490 AU
2.9276 AU
Eccentricity 0.1635
5.01 yr (1,830 days)
21.266°
0° 11m 48.48s / day
Inclination 14.661°
70.606°
175.16°
Physical characteristics
56.67±1.15 km (IRAS)
Mean density
2.0 g/cm3(assumed) [3]
2.5 g/cm3(assumed) [4]
Equatorial escape velocity
60 m/s (calculated) [3]
75 m/s (calculated) [4]
15.8480  h (0.66033  d) [1]
0.0379±0.002 [1]
PCD (Tholen) [1]
T (SMASSII) [1]
11.67 to 15.32
8.90 [1]

    596 Scheila is a main-belt asteroid [1] and main-belt comet [2] orbiting the Sun. It was discovered on 21 February 1906 by August Kopff from Heidelberg. [1] Kopff named the asteroid after a female English student with whom he was acquainted. [5]

    Contents

    Overview

    Scheila imaged by the Hubble Space Telescope on 7 December 2010, with visible features marked. 596 Scheila Hubble annotated.jpg
    Scheila imaged by the Hubble Space Telescope on 7 December 2010, with visible features marked.
    Scheila imaged by Neil Gehrels Swift Observatory's ultraviolet-optical telescope on 15 December 2010 596 Scheila Swift.jpg
    Scheila imaged by Neil Gehrels Swift Observatory's ultraviolet-optical telescope on 15 December 2010

    On 11 December 2010, Steve Larson of the Catalina Sky Survey detected a comet-like appearance to asteroid Scheila: it displayed a "coma" of about magnitude 13.5. [6] Inspection of archival Catalina Sky Survey observations showed the activity was triggered between 11 November 2010 and 3 December. [7] Imaging with the 2-meter Faulkes Telescope North revealed a linear tail in the anti-sunward direction and an orbital tail, indicative of larger slower particles. [8]

    When first detected it was unknown what drove the ejecta plumes. Scheila's gravity is too large for electrostatics to launch dust. [2] Cometary outgassing could not be ruled out until detailed spectroscopic observations indicated the absence of gas in Scheila's plumes. [4] Observations by the Hubble Space Telescope and the Neil Gehrels Swift Observatory's ultraviolet-optical telescope make it most likely that Scheila was impacted at ~5 km/s by a previously unknown asteroid ~35 meters in diameter. [3] [4] Each asteroid the size of Scheila might be hit by an impactor 10–100 meters in diameter approximately every 1000 years, so with 200 asteroids of this size or bigger in the asteroid belt, we can observe a collision as often as every 5 years. [4]

    As a consequence of the 2010 impact, the surface spectrum of Scheila changed, from a moderately red T-type spectrum to a more reddish D-type spectrum, showing how "fresh" material weathers over time in space. This is similar to laboratory experiments done on the Tagish Lake meteorite. [9]

    Scheila last came to perihelion on 2022 May 26. [1]

    See also

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    References

    1. 1 2 3 4 5 6 7 8 9 10 11 "JPL Small-Body Database Browser: 596 Scheila (1906 UA)" (2010-11-14 last obs). Retrieved 7 May 2016.
    2. 1 2 3 David C. Jewitt. "Main Belt Comets". UCLA, Department of Earth and Space Sciences. Retrieved 15 December 2010.
    3. 1 2 3 Jewitt, David; Weaver, H.; Mutcher, M.; Larson, S.; Agarwal, J. (2011). "Hubble Space Telescope Observations of Main Belt Comet (596) Scheila". Astrophysical Journal Letters. 733 (1): L4. arXiv: 1103.5456 . Bibcode:2011ApJ...733L...4J. doi:10.1088/2041-8205/733/1/l4. S2CID   50809352.
    4. 1 2 3 4 5 Bodewits, Dennis; Kelley, M. S.; Li, J. -Y.; Landsman, W. B.; Besse, S.; A'Hearn, M. F. (2011). "Collisional Excavation of Asteroid (596) Scheila". Astrophysical Journal Letters. 733 (1): L3. arXiv: 1104.5227 . Bibcode:2011ApJ...733L...3B. doi:10.1088/2041-8205/733/1/L3. S2CID   54187826.
    5. ↑ Schmadel, Lutz D. (2003). Dictionary of Minor Planet Names. Springer Science & Business Media. p. 61. ISBN   978-3-540-00238-3.
    6. ↑ Ernesto Guido & Giovanni Sostero (12 December 2010). "Comet-like appearance of (596) Scheila". Remanzacco Observatory in Italy (blog). Archived from the original on 7 January 2011. Retrieved 12 December 2010.
    7. ↑ Mike Simonsen (12 December 2010). "A Comet Masquerading as an Asteroid". Simostronomy (blog). Retrieved 12 December 2010.
    8. ↑ Richard Miles's posting on Yahoo minor planet mailing list (MPML)
    9. ↑ Hasegawa, Sunao; Marsset, Michaël; Demeo, Francesca E.; Bus, Schelte J.; Ishiguro, Masateru; Kuroda, Daisuke; Binzel, Richard P.; Hanuš, Josef; Nakamura, Akiko M.; Yang, Bin; Vernazza, Pierre (2022). "The Appearance of a "Fresh" Surface on 596 Scheila as a Consequence of the 2010 Impact Event". The Astrophysical Journal Letters. 924 (1): L9. arXiv: 2112.04672 . Bibcode:2022ApJ...924L...9H. doi: 10.3847/2041-8213/ac415a . S2CID   245005881.
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