astro.wikisort.org - Asteroid3267 Glo, provisional designation 1981 AA, is an eccentric Phocaean asteroid and sizable Mars-crosser from the inner regions of the asteroid belt, approximately 6.4 kilometers (4.0 miles) in diameter. It was discovered on 3 January 1981, by American astronomer Edward Bowell at Lowell's Anderson Mesa Station in Flagstaff, Arizona.[1] It was later named after American astronomer Eleanor Helin.[2]
3267 Glo|
Discovered by | E. Bowell |
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Discovery site | Anderson Mesa Stn. |
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Discovery date | 3 January 1981 |
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MPC designation | (3267) Glo |
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Named after | Eleanor F. Helin (American astronomer)[2] |
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Alternative designations | 1981 AA |
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Minor planet category | Mars-crosser[1][3] Phocaea[4][5] |
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Epoch 23 March 2018 (JD 2458200.5) |
Uncertainty parameter 0 |
Observation arc | 36.49 yr (13,329 d) |
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Aphelion | 3.0178 AU |
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Perihelion | 1.6424 AU |
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Semi-major axis | 2.3301 AU |
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Eccentricity | 0.2951 |
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Orbital period (sidereal) | 3.56 yr (1,299 d) |
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Mean anomaly | 196.67° |
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Mean motion | 0° 16m 37.56s / day |
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Inclination | 24.021° |
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Longitude of ascending node | 110.47° |
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Argument of perihelion | 307.73° |
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Mean diameter | 6.45±1.44 km[6] 7.58±0.76 km[7] 13.56±1.1 km[8] 13.59 km (derived)[4] |
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Synodic rotation period | 6.8782±0.0011 h[4][lower-alpha 1] |
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Geometric albedo | 0.0607±0.011[8] 0.0725 (derived)[4] 0.233±0.047[7] 0.26±0.12[6] |
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Spectral type | LS[9] · S (derived)[4] |
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Absolute magnitude (H) | 12.8[3][4][7] · 12.86±0.14[9] 13.19[6] |
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Orbit and classification
Glo is an eccentric member of the Phocaea family (701),[5] that orbits the Sun in the inner asteroid belt at a distance of 1.6–3.0 AU once every 3 years and 7 months (1,299 days; semi-major axis of 2.33 AU). Its orbit has an eccentricity of 0.30 and an inclination of 24° with respect to the ecliptic.[3]
The body's observation arc begins with its official discovery observation at Anderson Mesa in January 1981.[1]
Physical characteristics
The asteroid has been characterized as an L- and S-type asteroid by Pan-STARRS large-scale survey.[9]
Spectral type
PanSTARRS' photometric survey, has characterized Glo as a LS-type asteroid, a transitional spectral type between the common S-type and rather rare L-type asteroids,[9] which have very different albedos, from as low as 0.039 to as high as 0.383.[10]
Rotation period
A rotational lightcurve of Glo was obtained from photometric observations by Czech astronomer Petr Pravec at Ondřejov Observatory in January 2006. Lightcurve analysis gave a well-defined rotation period of 6.8782 hours with a brightness variation of 0.33 magnitude (U=3).[4]
Diameter and albedo
According to the surveys carried out by the Infrared Astronomical Satellite IRAS, and NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Glo measures 6.45 and 13.56 kilometers in diameter and its surface has an albedo of 0.061 and 0.26, respectively.[6][8] The Collaborative Asteroid Lightcurve Link agrees with IRAS and derives a similar albedo of 0.0725 and a diameter of 13.59 kilometers with an absolute magnitude of 12.8.[4][lower-alpha 1]
Naming
This minor planet was named in honor of Eleanor "Glo" Helin (1932–2009), who was a planetary scientist at JPL and a prolific discoverer of minor planets.[2] The official naming citation was published by the Minor Planet Center on 13 February 1987 (M.P.C. 11641).[11]
Notes
- Lightcurve plot of 3267 Glo giving a rotation period of 6.8782 hours with an amplitude of 0.0329 magnitude, taken from unpublished data of the Ondrejov Asteroid Photometry Project. Summary figures at the LCDB.
References
- "3267 Glo (1981 AA)". Minor Planet Center. Retrieved 14 April 2018.
- Schmadel, Lutz D. (2007). "(3267) Glo". Dictionary of Minor Planet Names – (3267) Glo. Springer Berlin Heidelberg. p. 272. doi:10.1007/978-3-540-29925-7_3268. ISBN 978-3-540-00238-3.
- "JPL Small-Body Database Browser: 3267 Glo (1981 AA)" (2017-07-02 last obs.). Jet Propulsion Laboratory. Retrieved 14 April 2018.
- "LCDB Data for (3267) Glo". Asteroid Lightcurve Database (LCDB). Retrieved 9 March 2017.
- "Asteroid 3267 Glo – Nesvorny HCM Asteroid Families V3.0". Small Bodies Data Ferret. Retrieved 26 October 2019.
- 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.
- Alí-Lagoa, V.; Delbo', M. (July 2017). "Sizes and albedos of Mars-crossing asteroids from WISE/NEOWISE data". Astronomy and Astrophysics. 603: 8. arXiv:1705.10263. Bibcode:2017A&A...603A..55A. doi:10.1051/0004-6361/201629917.
- Tedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004). "IRAS Minor Planet Survey V6.0". NASA Planetary Data System. 12: IRAS-A-FPA-3-RDR-IMPS-V6.0. Bibcode:2004PDSS...12.....T. Retrieved 22 October 2019.
- 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.
- "JPL Small-Body Database Search Engine: "spectral type = L (SMASSII)"". JPL Solar System Dynamics. Retrieved 28 April 2017.
- "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 9 March 2017.
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На других языках
[de] (3267) Glo
(3267) Glo ist ein Asteroid des Hauptgürtels, der am 3. Januar 1981 vom amerikanischen Astronomen Edward L. G. Bowell an der Anderson Mesa Station (IAU-Code 688) des Lowell-Observatoriums in Coconino County entdeckt wurde.
- [en] 3267 Glo
[ru] (3267) Гло
(3267) Гло (лат. Glo) — астероид, относящийся к группе астероидов пересекающих орбиту Марса. Он был открыт 3 января 1981 года американским астрономом Эдвардом Боуэллом в обсерватории Андерсон-Меса и назван в честь американской женщины-астронома Элеанор Хелин.[1]
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