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Comet Elst–Pizarro is a body that displays characteristics of both asteroids and comets,[11] and is the prototype of active asteroids. Its orbit keeps it within the asteroid belt, yet it displayed a dust tail like a comet while near perihelion in 1996, 2001, and 2007.

7968 Elst–Pizarro
133P/Elst–Pizarro
7968 Elst–Pizarro imaged at La Silla Observatory in August 1996. The narrow tail is visible.
Discovery
Discovered by1979 OW7:
M. R. S. Hawkins
R. H. McNaught,[1] S. J. Bus[2]
1996 N2:
Eric W. Elst, Guido Pizarro
Discovery date24 July 1979 (1979 OW7) [3]
14 July 1996 (1996 N2)
Designations
MPC designation
(7968) Elst–Pizarro
Alternative designations
P/1996 N2
1979 OW7
Minor planet category
Main-belt comet[4][5]
Main-belt asteroid[6]
Themis/ Beagle family [4]
Orbital characteristics[6]
Epoch 13 January 2016 (JD 2457400.5)
Uncertainty parameter 0
Observation arc13350 days (36.55 yr)
Aphelion3.66751 AU (548.652 Gm) (Q)
Perihelion2.6524 AU (396.79 Gm) (q)
Semi-major axis
3.1600 AU (472.73 Gm) (a)
Eccentricity0.16062 (e)
Orbital period (sidereal)
5.62 yr (2051.7 d)
Average orbital speed
16.64 km/s
Mean anomaly
187.70° (M)
Mean motion
0° 10m 31.656s / day (n)
Inclination1.3873° (i)
Longitude of ascending node
160.14° (Ω)
Argument of perihelion
131.97° (ω)
Jupiter MOID1.51427 AU (226.532 Gm)
TJupiter3.185
Physical characteristics
Dimensions3.8±0.6 km[7]
3.9+0.4
−0.3 km[8]
Mean density
1.3(?) g/cm3[9]
Synodic rotation period
3.471 h (0.1446 d)[6]
Geometric albedo
0.074±0.013R
Temperature160 K[9]
Apparent magnitude
17.24 to 20.71
Absolute magnitude (H)
15.7[6]
15.3R (2004) [9]
15.49R (2010) [10]

    Elst–Pizarro was reported in 1979 as minor planet 1979 OW7, with its image on a photographic plate being completely stellar in appearance. Its orbit remains entirely within the orbits of Mars and Jupiter, with eccentricity 0.165, typical of a minor planet in the asteroid belt. However, the images taken by Eric W. Elst and Guido Pizarro in 1996, when it was near perihelion, clearly show a cometary tail. Since this is not normal behaviour for asteroids, it is suspected that Elst–Pizarro has a different, probably icy, composition. The cometary nature of Elst–Pizarro was first discovered when a linear dust feature was observed with the ESO 1-metre Schmidt telescope at La Silla Observatory on 7 August 1996.[9][12]

    Subsequently, around the next perihelion in November 2001, the cometary activity appeared again, and persisted for 5 months.[9] It again came to perihelion on 8 February 2013.[6] The outgassing was found to happen only on small part of the surface measuring less than 600m in effective diameter, likely being the relatively recent (younger than 100 million years) impact crater.[8]

    At present, seven other objects that are cross-listed as both comets and asteroids: 2060 Chiron (95P/Chiron), 4015 Wilson–Harrington (107P/Wilson–Harrington), 60558 Echeclus (174P/Echeclus), 118401 LINEAR (176P/LINEAR), (323137) 2003 BM80 (282P/2003 BM80), (300163) 2006 VW139 (288P/2006 VW139), (457175) 2008 GO98 (362P/2008 GO98),[13] and (248370) 2005 QN173 (433P/2005 QN173).[14] As a dual status object, astrometric observations of 7968 Elst–Pizarro should be reported under the minor planet designation.[13]


    Exploration


    Castalia is a proposed mission concept for a robotic spacecraft to explore Pizarro and make the first in situ measurements of water in the asteroid belt, and thus, help solve the mystery of the origin of Earth's water.[15] The lead is Colin Snodgrass, from The Open University in the UK. Castalia was proposed in 2015 and 2016 to the European Space Agency within the Cosmic Vision programme missions M4 and M5, but it was not selected. The team continues to mature the mission concept and science objectives.[15] Because of the construction time required and orbital dynamics, a launch date of October 2028 was proposed.[15]

    Castalia mission scientists are now considering instrument contributions for the Chinese ZhengHe comet exploration mission, which will conduct detailed remote sensing and in-situ measurements at Elst–Pizarro in 2032[16] following a proposed launch in 2025.[17]


    References


    1. "MPEC 1996-R07 : COMET P/1996 N2 (ELST-PIZARRO)". IAU-Minor Planet Center. 12 September 1996.
    2. "IAUC 6473". IAU-Central Bureau for Astronomical Telegrams. 12 September 1996.
    3. "IAUC 6457". IAU-Central Bureau for Astronomical Telegrams. 21 August 1996.
    4. Henry H. Hsieh (May 2010). "Main Belt Comets". Hawaii. Archived from the original on 2011-08-06. Retrieved 2010-12-15. (older 2010 site) Archived August 10, 2009, at the Wayback Machine
    5. David Jewitt. "Main Belt Comets". UCLA, Department of Earth and Space Sciences. Retrieved 2010-12-15.
    6. "JPL Small-Body Database Browser: 7968 Elst–Pizarro (1996 N2)" (2012-06-06 last obs). Archived from the original on 9 August 2012. Retrieved 13 April 2016. from the original on 2012-08-08
    7. Hsieh, Henry H.; Jewitt, David C.; Fernández, Yanga R. (2009). "Albedos of Main-Belt Comets 133P/Elst–Pizarro and 176P/LINEAR". The Astrophysical Journal Letters. 694 (2): L111–L114. arXiv:0902.3682. Bibcode:2009ApJ...694L.111H. doi:10.1088/0004-637X/694/2/L111. S2CID 17438376.
    8. Liang Liang Yu; Hsia, Chih-Hao; Ip, Wing-Huen (2020). "Low-activity Main-belt Comet 133P/Elst-Pizarro: New Constraints on Its Albedo, Temperature, and Active Mechanism from a Thermophysical Perspective". The Astronomical Journal. 159 (2): 66. arXiv:1912.06266. Bibcode:2020AJ....159...66Y. doi:10.3847/1538-3881/ab61f7. S2CID 209370820.
    9. Hsieh, Henry H.; Jewitt, David C.; Fernández, Yanga R. (2004). "The Strange Case of 133P/Elst–Pizzarro: A Comet Among the Asteroids". The Astronomical Journal. 127 (5): 2997–3017. Bibcode:2004AJ....127.2997H. CiteSeerX 10.1.1.362.9950. doi:10.1086/383208.
    10. Hsieh, Henry H.; Jewitt, David C.; Lacerda, Pedro; Lowry, Stephen C.; Snodgrass, Colin (2010). "The return of activity in main-belt comet 133P/Elst–Pizarro". Monthly Notices of the Royal Astronomical Society. 403 (1): 363–377. arXiv:0911.5522. Bibcode:2010MNRAS.403..363H. doi:10.1111/j.1365-2966.2009.16120.x. S2CID 118438991.
    11. "Main-Belt Comets May Have Been Source Of Earths Water". Space Daily. 23 March 2006.
    12. "Strange Comet Discovered at ESO". ESO. 16 September 1996.
    13. "Dual-Status Objects". Minor Planet Center. 2008-03-06. Retrieved 2018-02-13.
    14. M.P.C. 133823
    15. Snodgrass, C.; Jones, G.H.; Boehnhardt, H.; Gibbings, A.; Homeister, M.; Andre, N.; Beck, P.; Bentley, M.S.; Bertini, I.; Bowles, N.; Capria, M.T.; Carr, C.; Ceriotti, M.; Coates, A.J.; Della Corte, V.; Donaldson Hanna, K.L.; Fitzsimmons, A.; Gutiérrez, P.J.; Hainaut, O.R.; Herique, A.; Hilchenbach, M.; Hsieh, H.H.; Jehin, E.; Karatekin, O.; Kofman, W.; Lara, L.M.; Laudan, K.; Licandro, J.; Lowry, S.C.; et al. (2018). "The Castalia mission to Main Belt Comet 133P/Elst-Pizarro". Advances in Space Research. 62 (8): 1947–1976. arXiv:1709.03405. Bibcode:2018AdSpR..62.1947S. doi:10.1016/j.asr.2017.09.011. S2CID 55821241.
    16. Snodgrass, Colin (October 2018). "Exploring the next frontier: the Main Belt Comets – Chinese MBC mission" (PDF). University of Edinburgh. p. 20. Retrieved 20 June 2019.
    17. Jones, Andrew (30 June 2021). "China outlines space plans to 2025". SpaceNews. Retrieved 30 June 2021.


    Numbered comets
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    На других языках

    [de] (7968) Elst-Pizarro

    Elst-Pizarro ist der Prototyp einer Klasse der Kometen, deren Bahn vollständig im Hauptgürtel liegt und nicht von der eines Asteroiden unterschieden werden kann, die aber auch eine Koma oder – wie Elst-Pizarro – im Perihel sogar einen Schweif ausbilden. Das Objekt hat deshalb auch die Doppelbenennung 133P/Elst-Pizarro und (7968) Elst-Pizarro.
    - [en] 7968 Elst–Pizarro

    [ru] (7968) Эльст — Писарро

    (7968) Эльст — Писарро (лат. Elst-Pizarro) — это астероид главного пояса, также известный как комета 133P/Эльста — Писарро[8][9]. Объект был открыт 14 июля 1996 года бельгийским астрономом Эриком Эльстом на фотопластине, полученной Гвидо Писарро с помощью 1,0-метрового телескопа обсерватории Ла-Силья[10][11]. И, первоначально, был описан как комета 18,3 m звёздной величины и небольшим узким хвостом, простирающимся на 1 ' угловую минуту в юго-западном направлении. Но на найденных архивных снимках, полученных ещё 24 и 25 июля 1979 года M. R. S. Hawkins, Робертом Макнотом и Шелте Басом, он выглядел как звёздоподобный объект 19,5 m и был идентифицирован как малая планета с временным обозначением 1979 OW7[12]. Несмотря на официальный двойной статус, по правилам МАС, все подобные объекты в базах данных, фактически, проходят как астероиды.


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