57424 Caelumnoctu

Last updated
57424 Caelumnoctu
Orbit of 57424 Caelumnoctu.gif
Orbital diagram of Caelumnoctu
Discovery  [1] [2]
Discovered by LINEAR
Discovery site Lincoln Lab's ETS
Discovery date16 September 2001
Designations
(57424) Caelumnoctu
Named after
 The Sky at Night   [2]
(BBC astronomy programme)
2001 SP22 ·1982 BV4
main-belt  ·(outer)
Eos   [3]
Orbital characteristics   [1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc 35.76 yr (13,061 days)
Aphelion 3.3243 AU
Perihelion 2.7495 AU
3.0369 AU
Eccentricity 0.0946
5.29 yr (1,933 days)
334.96°
0° 11m 10.32s / day
Inclination 9.6708°
353.32°
45.951°
Physical characteristics
Dimensions6.876±0.356 km [4]
0.113±0.019 [4]
13.7 [1]

    57424 Caelumnoctu (provisional designation 2001 SP22) is an Eoan asteroid from the outer regions of the asteroid belt, approximately 7 kilometers in diameter. It was discovered on 16 September 2001, by astronomers of the Lincoln Near-Earth Asteroid Research at Lincoln Laboratory's Experimental Test Site near Socorro, New Mexico. The asteroid was named for the BBC television programme The Sky at Night . [2]

    Contents

    Orbit and classification

    Caelumnoctu is a member the Eos family ( 606 ), [3] the largest asteroid family in the outer main belt consisting of nearly 10,000 asteroids. [5] : 23 

    It orbits the Sun at a distance of 2.7–3.3  AU once every 5 years and 3 months (1,933 days; semi-major axis of 3.04 AU). Its orbit has an eccentricity of 0.09 and an inclination of 10° with respect to the ecliptic. [1]

    The body's observation arc begins with its first identification as 1982 BV4 at Kiso Observatory in January 1982, more than 19 years prior to its official discovery observation at Socorro. [2]

    Physical characteristics

    The body's spectral type is unknown. [1] Its albedo, however, corresponds to the K-type asteroids of which the Eos family predominantly consists. [5] : 23 

    Diameter and albedo

    According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Caelumnoctu measures 6.876 kilometers in diameter and its surface has an albedo of 0.113. [4]

    Rotation period

    As of 2017, no rotational lightcurve of Caelumnoctu has been obtained from photometric observations. The body's rotation period, poles and shape remain unknown. [1] [6]

    Naming

    This minor planet was named "Caelumnoctu" (Latin for The Sky at Night) in honour of the BBC television programme which celebrated its 50th anniversary in 2007. The number "57424" refers to the date of the first broadcast, 24 April 1957. [2]

    The official naming citation was published by the Minor Planet Center on 2 April 2007 ( M.P.C. 59387). [7]

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    <span class="mw-page-title-main">4001 Ptolemaeus</span>

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    <span class="mw-page-title-main">2111 Tselina</span> Stony asteroid in the outer asteroid belt

    2111 Tselina is a stony Eos asteroid from the outer regions of the asteroid belt. It was discovered on 13 June 1969, by Soviet astronomer Tamara Smirnova at Crimean Astrophysical Observatory in Nauchnij, on the Crimean peninsula. The S-type asteroid has a rotation period of 6.6 hours and measures approximately 23 kilometers in diameter. It was later named after the Soviet Virgin Lands Campaign.

    2752 Wu Chien-Shiung, provisional designation 1965 SP, is an Eoan asteroid from the outer regions of the asteroid belt, approximately 16 kilometers in diameter. It was discovered on 20 September 1965, by astronomers at Purple Mountain Observatory in Nanking, China. The asteroid has a long rotation period of 36.3 hours. It was named for Chinese-American nuclear physicist Chien-Shiung Wu.

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    23327 Luchernandez (provisional designation 2001 BE31) is a Florian asteroid from the inner regions of the asteroid belt, approximately 2 kilometers in diameter. It was discovered on 20 January 2001, by astronomers of the LINEAR program at the Lincoln Laboratory's Experimental Test Site near Socorro, New Mexico, United States. The asteroid was named for ISEF awardee Lucero Hernandez.

    <span class="mw-page-title-main">7835 Myroncope</span>

    7835 Myroncope is an asteroid of the Mitidika family from the central region of the asteroid belt. It was discovered on 16 June 1993, by American astronomer Timothy Spahr at the Catalina Station in Arizona, United States. The assumed S-type asteroid has a rotation period of 7.4 hours and measures approximately 10 kilometers in diameter. It was named in memory of American sports announcer Myron Cope (1929–2008).

    <span class="mw-page-title-main">5357 Sekiguchi</span> Asteroid

    5357 Sekiguchi is an Eos asteroid from the outer region of the asteroid belt, approximately 15 kilometers in diameter. It was discovered on 2 March 1992, by Japanese amateur astronomers Tetsuya Fujii and Kazuro Watanabe at the Kitami Observatory in eastern Hokkaidō, Japan. The asteroid was later named after Japanese astronomer Tomohiko Sekiguch.

    References

    1. 1 2 3 4 5 6 "JPL Small-Body Database Browser: 57424 Caelumnoctu (2001 SP22)" (2017-10-30 last obs.). Jet Propulsion Laboratory . Retrieved 23 November 2017.
    2. 1 2 3 4 5 "57424 Caelumnoctu (2001 SP22)". Minor Planet Center . Retrieved 23 November 2017.
    3. 1 2 "Asteroid 57424 Caelumnoctu – Nesvorny HCM Asteroid Families V3.0". Small Bodies Data Ferret. Retrieved 27 October 2019.
    4. 1 2 3 Masiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Dailey, J.; et al. (November 2011). "Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters". The Astrophysical Journal. 741 (2): 20. arXiv: 1109.4096 . Bibcode:2011ApJ...741...68M. doi:10.1088/0004-637X/741/2/68.
    5. 1 2 Nesvorný, D.; Broz, M.; Carruba, V. (December 2014). "Identification and Dynamical Properties of Asteroid Families". Asteroids IV. pp. 297–321. arXiv: 1502.01628 . Bibcode:2015aste.book..297N. doi:10.2458/azu_uapress_9780816532131-ch016. ISBN   9780816532131.
    6. ↑ "LCDB Data for (57424) Caelumnoctu (not in the LCDB)". Asteroid Lightcurve Database (LCDB). Retrieved 23 November 2017.
    7. ↑ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 23 November 2017.
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