5806 Archieroy

Last updated

5806 Archieroy
Discovery  [1]
Discovered by E. Bowell
Discovery site Lowell Obs.
Discovery date11 January 1986
Designations
(5806) Archieroy
Named after
 Archie Roy
(astrophysicist) [2]
1986 AG1 ·1987 QQ9
main-belt  ·(inner)  [1]
Hungaria   [3] [4]
Orbital characteristics   [1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc 62.83 yr (22,948 days)
Aphelion 2.0347 AU
Perihelion 1.8908 AU
1.9628 AU
Eccentricity 0.0367
2.75 yr (1,004 days)
257.13°
0° 21m 30.24s / day
Inclination 20.816°
300.87°
97.285°
Physical characteristics
Dimensions5.75±1.02 km [5]
6.34±1.34 km [6]
6.38 km (calculated) [4]
6.785±0.224 km [7]
12.16±0.01 h [8]
12.1602±0.0005 h [9]
12.163±0.001 h [10]
12.187±0.003 h [11]
0.19±0.10 [6]
0.291±0.063 [7]
0.3 (assumed) [4]
0.37±0.18 [5]
E   [4]  · V   [12]
12.80 [7]  ·12.9 [1] [4] [5]  ·13.53 [6]

    5806 Archieroy, provisional designation 1986 AG1, is a stony Hungaria asteroid from the inner regions of the asteroid belt, approximately 6 kilometers in diameter. It was discovered on 11 January 1986, by American astronomer Edward Bowell at Lowell's Anderson Mesa Station near Flagstaff, Arizona. [3] It is named after Scottish astrophysicist Archie Roy. [2]

    Contents

    Classification and orbit

    The bright E-type asteroid, alternatively classified as a V-type, is a member of the Hungaria family, which form the innermost dense concentration of asteroids in the Solar System. It orbits the Sun in the inner main-belt at a distance of 1.9–2.0  AU once every 2 years and 9 months (1,004 days). Its orbit has an eccentricity of 0.04 and an inclination of 21° with respect to the ecliptic. [1] A first precovery was taken at Palomar Observatory in 1954, extending the asteroid's observation arc by 32 years prior to its official discovery observation at Anderson Mesa. [3]

    Lightcurve

    Between 2004 and 2015, several rotational lightcurves of Archieroy have been obtained from photometric observations by American astronomers Brian Warner at his Palmer Divide Observatory, Colorado, and Robert Stephens at the Center for Solar System Studies, California. Lightcurve analysis [lower-alpha 1] gave a well-defined rotation period between 12.16 and 12.187 hours with a high brightness variation of 0.34 to 0.47 magnitude ( U=3-/3/3/3 ). [8] [9] [10] [11]

    Diameter and albedo

    According to the survey carried out by NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Archieroy measures between 5.75 and 6.78 kilometers in diameter, and its surface has an albedo between 0.19 and 0.37, [5] [6] [7] while the Collaborative Asteroid Lightcurve Link assumes an albedo of 0.30 – a compromise value between 0.4 and 0.2, corresponding to the Hungaria asteroids both as family and orbital group – and calculates a diameter of 6.38 kilometers, with an absolute magnitude of 12.9. [4]

    Naming

    This minor planet was named after Scottish astrophysicist and celestial mechanician Archie Roy (1924–2012), who was a Fellow of the Royal Society of Edinburgh, the Royal Astronomical Society, and the British Interplanetary Society, as well as the president of the Society for Psychical Research and professor at Glasgow University. His research included the restricted and general three-body problems, high-order Taylor series and the long-term stability of and the orbital resonances in the Solar System. He has also authored and published several textbooks and novels. [2] The approved naming citation was published by the Minor Planet Center on 19 October 1994 ( M.P.C. 24123). [13]

    Notes

    1. ↑ lightcurve plots by Brian Warner and Robert Stephens of (5806) Archieroy

    Related Research Articles

    1509 Esclangona, provisional designation 1938 YG, is a rare-type Hungaria asteroid and binary system from the inner regions of the asteroid belt, approximately 8 kilometers in diameter. It is named after French astronomer Ernest Esclangon.

    1019 Strackea, provisional designation 1924 QN, is a stony Hungaria asteroid of the inner asteroid belt, approximately 8 kilometers in diameter. It was discovered on 3 March 1924, by astronomer Karl Reinmuth at Heidelberg Observatory in southwest Germany. It is named for German astronomer Gustav Stracke.

    3309 Brorfelde, provisional designation 1982 BH, is a nearly spheroidal, binary Hungaria asteroid from the inner regions of the asteroid belt, approximately 4 kilometers in diameter. It was discovered on 28 January 1982, by Danish astronomers Kaare Jensen and Karl Augustesen at the Brorfelde Observatory near Holbæk, Denmark. It was named for the discovering observatory and the village where it is located.

    4031 Mueller, provisional designation 1985 CL, is a Hungaria asteroid from the inner regions of the asteroid belt, approximately 4 kilometers in diameter. It was discovered on 12 February 1985, by American astronomer Carolyn Shoemaker at Palomar Observatory, California, and named after astronomer Jean Mueller.

    3225 Hoag, provisional designation 1982 QQ, is a dynamical Hungaria asteroid from the innermost regions of the asteroid belt, approximately 5.5 kilometers in diameter. It was discovered on 20 August 1982, by American astronomer couple Carolyn and Eugene Shoemaker at the Palomar Observatory in California. The stony S/L-type asteroid has a short rotation period of 2.37 hours. It was named for American astronomer Arthur Hoag.

    6296 Cleveland, provisional designation 1988 NC, is a Hungaria asteroid from the innermost regions of the asteroid belt, approximately 3.5 kilometers in diameter. It was discovered on 12 July 1988, by American astronomer Eleanor Helin at the Palomar Observatory in California. The presumed E-type asteroid has a long rotation period of 30.8 hours and possibly an elongated shape. It was named for the city of Cleveland in the U.S. state of Ohio.

    3854 George, provisional designation: 1983 EA, is a stony Hungaria asteroid and Mars-crosser from the innermost regions of the asteroid belt, approximately 3.5 kilometers in diameter. It was discovered on 13 March 1983, by American astronomer couple Carolyn and Eugene Shoemaker at the Palomar Observatory in California. The unlikely synchronous binary system has a rotation period of 3.3 hours. It was named after the discoverer's father-in-law, George Shoemaker.

    7187 Isobe, provisional designation 1992 BW, is a likely binary Hungaria asteroid from the inner regions of the asteroid belt, approximately 5 kilometers in diameter. It was discovered on 30 January 1992, by American astronomer Eleanor Helin at Palomar Observatory in California, United States. It is named after Japanese astronomer Syuzo Isobe.

    3353 Jarvis, or by its provisional designation, 1981 YC, is a carbonaceous Hungaria asteroid, slow rotator and suspected tumbler from the inner regions of the asteroid belt, approximately 10 kilometers in diameter.

    1176 Lucidor, provisional designation 1930 VE, is a carbonaceous background asteroid from the central region of the asteroid belt, approximately 30 kilometers in diameter. It was discovered by Eugène Delporte in 1930, who named it after a friend.

    5641 McCleese, provisional designation 1990 DJ, is a rare-type Hungaria asteroid and slow rotator, classified as Mars-crosser from the innermost regions of the asteroid belt, approximately 4 kilometers in diameter.

    <span class="mw-page-title-main">3169 Ostro</span>

    3169 Ostro, provisional designation 1981 LA, is a Hungaria family asteroid from the innermost regions of the asteroid belt, approximately 5 kilometers in diameter.

    3873 Roddy, provisional designation 1984 WB, is a stony Hungarian asteroid, Mars-crosser and suspected binary system, from the innermost regions of the asteroid belt, approximately 7 kilometers in diameter. It was discovered on 21 November 1984, by American astronomer Carolyn Shoemaker at the Palomar Observatory in California, United States. It was named after American astrogeologist David Roddy.

    2074 Shoemaker, provisional designation 1974 UA, is a stony Hungaria asteroid, Mars-crosser and suspected synchronous binary system from the innermost regions of the asteroid belt, approximately 4 kilometers in diameter. It was discovered on 17 October 1974, by astronomer Eleanor Helin at the Palomar Observatory. She named it after American astronomer Eugene Shoemaker.

    2047 Smetana, provisional designation 1971 UA1, is a bright Hungaria asteroid and synchronous binary system from the innermost regions of the asteroid belt, approximately 3.5 kilometers in diameter. It was discovered on 26 October 1971, by Czech astronomer Luboš Kohoutek at Bergedorf Observatory in Hamburg, Germany. The asteroid was named after Czech composer Bedřich Smetana. Its sub-kilometer sized minor-planet moon was discovered in 2012.

    3401 Vanphilos, provisional designation 1981 PA, is a stony, eccentric asteroid and sizeable Mars-crosser, approximately 7 kilometers in diameter. It was discovered on 1 August 1981, by and at Harvard's Oak Ridge Observatory in Massachusetts, United States.

    <span class="mw-page-title-main">1600 Vyssotsky</span>

    1600 Vyssotsky, provisional designation 1947 UC, is a rare-type Hungaria asteroid and suspected interloper from the inner regions of the asteroid belt, approximately 7 kilometers in diameter. It was discovered on 22 October 1947, by American astronomer Carl Wirtanen at Lick Observatory in California, United States. It was named after astronomer Alexander Vyssotsky.

    (6382) 1988 EL, is a stony Hungaria asteroid from the inner regions of the asteroid belt, approximately 5 kilometers in diameter. It was discovered on 14 March 1988, by American astronomer Jeffrey Alu at the U.S. Palomar Observatory, California.

    8026 Johnmckay, provisional designation 1991 JA1, is a binary Hungaria asteroid and very slow rotator from the inner regions of the asteroid belt, approximately 2 kilometers in diameter. It was discovered on 8 May 1991, by American astronomer Eleanor Helin at the U.S. Palomar Observatory, California, and later named for NASA test pilot John B. McKay.

    20936 Nemrut Dagi, provisional designation: 4835 T-1, is a stony Hungaria asteroid and Mars-grazer from the innermost regions of the asteroid belt, approximately 3.5 kilometers in diameter. It was discovered on 13 May 1971, by Dutch astronomer couple Ingrid and Cornelis van Houten at Leiden, on photographic plates taken by Dutch–American astronomer Tom Gehrels at Palomar Observatory in California, United States. The asteroid has a rotation period of 3.28 hours, a likely spheroidal shape, and a high albedo typically seen among the enstatite-rich E-type asteroids. In 2012, it was named after the a dormant volcano Nemrut in Turkey.

    References

    1. 1 2 3 4 5 "JPL Small-Body Database Browser: 5806 Archieroy (1986 AG1)" (2017-05-01 last obs.). Jet Propulsion Laboratory . Retrieved 4 July 2017.
    2. 1 2 3 Schmadel, Lutz D. (2007). "(5806) Archieroy". Dictionary of Minor Planet Names – (5806) Archieroy. Springer Berlin Heidelberg. p. 490. doi:10.1007/978-3-540-29925-7_5459. ISBN   978-3-540-00238-3.
    3. 1 2 3 "5806 Archieroy (1986 AG1)". Minor Planet Center. Retrieved 21 March 2017.
    4. 1 2 3 4 5 6 "LCDB Data for (5806) Archieroy". Asteroid Lightcurve Database (LCDB). Retrieved 21 March 2017.
    5. 1 2 3 4 Nugent, C. R.; Mainzer, A.; Masiero, J.; Bauer, J.; Cutri, R. M.; Grav, T.; et al. (December 2015). "NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos". The Astrophysical Journal. 814 (2): 13. arXiv: 1509.02522 . Bibcode:2015ApJ...814..117N. doi:10.1088/0004-637X/814/2/117. S2CID   9341381 . Retrieved 21 March 2017.
    6. 1 2 3 4 Nugent, C. R.; Mainzer, A.; Bauer, J.; Cutri, R. M.; Kramer, E. A.; Grav, T.; et al. (September 2016). "NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos". The Astronomical Journal. 152 (3): 12. arXiv: 1606.08923 . Bibcode:2016AJ....152...63N. doi: 10.3847/0004-6256/152/3/63 .
    7. 1 2 3 4 Masiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Nugent, C.; et al. (November 2012). "Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids". The Astrophysical Journal Letters. 759 (1): 5. arXiv: 1209.5794 . Bibcode:2012ApJ...759L...8M. doi:10.1088/2041-8205/759/1/L8. S2CID   46350317 . Retrieved 21 March 2017.
    8. 1 2 Warner, Brian D. (June 2005). "Asteroid lightcurve analysis at the Palmer Divide Observatory - fall 2004". The Minor Planet Bulletin. 32 (2): 29–32. Bibcode:2005MPBu...32...29W. ISSN   1052-8091 . Retrieved 21 March 2017.
    9. 1 2 Warner, Brian D. (April 2013). "Asteroid Lightcurve Analysis at the Palmer Divide Observatory: 2012 September - 2013 January". The Minor Planet Bulletin. 40 (2): 71–80. Bibcode:2013MPBu...40...71W. ISSN   1052-8091. PMC   7268920 . PMID   32494783.
    10. 1 2 Warner, Brian D. (September 2008). "Asteroid Lightcurve Analysis at the Palmer Divide Observatory: December 2007 - March 2008". The Minor Planet Bulletin. 35 (3): 95–98. Bibcode:2008MPBu...35...95W. ISSN   1052-8091 . Retrieved 21 March 2017.
    11. 1 2 Stephens, Robert D. (April 2016). "Asteroids Observed from CS3: 2015 October - December". The Minor Planet Bulletin. 43 (2): 158–159. Bibcode:2016MPBu...43..158S. ISSN   1052-8091. PMC   7243996 . PMID   32455374 . Retrieved 21 March 2017.
    12. ↑ Fornasier, S.; Migliorini, A.; Dotto, E.; Barucci, M. A. (July 2008). "Visible and near infrared spectroscopic investigation of E-type asteroids, including 2867 Steins, a target of the Rosetta mission". Icarus. 196 (1): 119–134. Bibcode:2008Icar..196..119F. doi:10.1016/j.icarus.2008.02.015. S2CID   122794657 . Retrieved 22 March 2017.
    13. ↑ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 21 March 2017.
    This page is based on this Wikipedia article
    Text is available under the CC BY-SA 4.0 license; additional terms may apply.
    Images, videos and audio are available under their respective licenses.