4659 Roddenberry

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4659 Roddenberry
Discovery  [1]
Discovered by S. J. Bus
Discovery site Siding Spring Obs.
Discovery date2 March 1981
Designations
(4659) Roddenberry
Named after
 Gene Roddenberry   [1]
(American screenwriter)
1981 EP20 ·1979 SY7
1979 TO1
main-belt   [1] [2]  ·(inner)
Nysa   [3] [4]
Orbital characteristics   [2]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc 41.19 yr (15,044 d)
Aphelion 2.9019 AU
Perihelion 1.8408 AU
2.3714 AU
Eccentricity 0.2237
3.65 yr (1,334 d)
188.19°
0° 16m 11.64s / day
Inclination 2.4668°
19.633°
5.1337°
Physical characteristics
3.56  km (derived) [3]
3.622±0.601 km [5] [6]
12  h (poor) [7]
0.193±0.065 [5] [6]
0.20(assumed) [3]
S (assumed) [3]
14.4 [2]
14.61 [3] [6] [7]
14.78±0.28 [8]

    4659 Roddenberry, provisional designation 1981 EP20, is a Nysian asteroid from the inner regions of the asteroid belt, approximately 3.6 kilometers (2.2 miles) in diameter. It was discovered on 2 March 1981, by American astronomer Schelte Bus at the Siding Spring Observatory in Australia. [1] The likely S-type asteroid has an unsecured rotation period of 12 hours. [3] It was named for American screenwriter Gene Roddenberry. [1]

    Contents

    Orbit and classification

    Roddenberry is a core member of the Nysa family ( 405 ), [3] [4] a very large family of stony asteroids, alternatively known as Herta family. It is part of the Nysa–Polana complex, the largest grouping of asteroids in the main-belt. The complex is typically further divided into subfamilies with different spectral properties. [9] : 23 

    The asteroid orbits the Sun in the inner asteroid belt at a distance of 1.8–2.9  AU once every 3 years and 8 months (1,334 days; semi-major axis of 2.37 AU). Its orbit has an eccentricity of 0.22 and an inclination of 2° with respect to the ecliptic. [2] The body's observation arc begins with a precovery taken at Palomar Observatory in February 1977, or four years prior to its official discovery observation at Siding Spring. [1]

    Physical characteristics

    Roddenberry is an assumed stony S-type asteroid, typical for core members of the Nysa family and in agreement with its high albedo (see below). [3]

    Rotation period

    In the 1990s, a fragmentary rotational lightcurve of Roddenberry was obtained from photometric observations by Richard Binzel. Lightcurve analysis gave a highly uncertain rotation period of 12 hours with a brightness amplitude of 0.14 magnitude ( U=1 ). As of 2018, no secure period has been obtained. [3] [7]

    Diameter and albedo

    According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Roddenberry measures 3.622 kilometers in diameter and its surface has an albedo of 0.193, [5] [6] while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20, and derives a diameter of 3.56 kilometers based on an absolute magnitude of 14.61. [3]

    Naming

    This minor planet was named in memory of famous American screenwriter, producer and futurist, Gene Roddenberry (1921–1991), known for the Star Trek and Star Trek: The Next Generation television series, and for the Star Trek film franchise. [1] The official naming citation was published by the Minor Planet Center on 18 February 1992 ( M.P.C. 19698). [10]

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    References

    1. 1 2 3 4 5 6 7 "4659 Roddenberry (1981 EP20)". Minor Planet Center. Retrieved 17 May 2018.
    2. 1 2 3 4 "JPL Small-Body Database Browser: 4659 Roddenberry (1981 EP20)" (2018-04-21 last obs.). Jet Propulsion Laboratory . Retrieved 17 May 2018.
    3. 1 2 3 4 5 6 7 8 9 10 "LCDB Data for (4659) Roddenberry". Asteroid Lightcurve Database (LCDB). Retrieved 17 May 2018.
    4. 1 2 "Asteroid 4659 Roddenberry". Small Bodies Data Ferret. Retrieved 17 May 2018.
    5. 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. S2CID   118745497.
    6. 1 2 3 4 Mainzer, A.; Grav, T.; Masiero, J.; Hand, E.; Bauer, J.; Tholen, D.; et al. (November 2011). "NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results". The Astrophysical Journal. 741 (2): 25. arXiv: 1109.6407 . Bibcode:2011ApJ...741...90M. doi:10.1088/0004-637X/741/2/90. S2CID   35447010. (catalog)
    7. 1 2 3 Binzel, Richard P.; Xu, Shui; Bus, Schelte J.; Bowell, Edward (September 1992). "Small Main-Belt Asteroid Lightcurve Survey". Icarus. 99 (1): 225–237. Bibcode:1992Icar...99..225B. doi:10.1016/0019-1035(92)90184-9. ISSN   0019-1035.
    8. ↑ Veres, Peter; Jedicke, Robert; Fitzsimmons, Alan; Denneau, Larry; Granvik, Mikael; Bolin, Bryce; et al. (November 2015). "Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results". Icarus. 261: 34–47. arXiv: 1506.00762 . Bibcode:2015Icar..261...34V. doi:10.1016/j.icarus.2015.08.007. S2CID   53493339.
    9. ↑ 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. S2CID   119280014.
    10. ↑ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 17 May 2018.
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