Discovery | |
---|---|
Discovered by | E. Bowell |
Discovery site | Anderson Mesa Stn. |
Discovery date | 3 January 1981 |
Designations | |
MPC designation | (3267) Glo |
Named after | Eleanor F. Helin (American astronomer) |
Alternative designations | 1981 AA |
Minor planet category | Mars-crosser Phocaea |
Orbital characteristics | |
Epoch 23 March 2018 (JD 2458200.5) | |
Uncertainty parameter 0 | |
Observation arc | 36.49 yr (13,329 d) |
Aphelion | 3.0178 AU |
Perihelion | 1.6424 AU |
Semi-major axis | 2.3301 AU |
Eccentricity | 0.2951 |
Orbital period (sidereal) | 3.56 yr (1,299 d) |
Mean anomaly | 196.67° |
Mean motion | 0° 16 37.56 / day |
Inclination | 24.021° |
Longitude of ascending node | 110.47° |
Argument of perihelion | 307.73° |
Physical characteristics | |
Mean diameter | 6.45±1.44 km 7.58±0.76 km 13.56±1.1 km 13.59 km (derived) |
Synodic rotation period | 6.8782±0.0011 h |
Geometric albedo | 0.0607±0.011 0.0725 (derived) 0.233±0.047 0.26±0.12 |
Spectral type | LS · S (derived) |
Absolute magnitude (H) | 12.8 · 12.86±0.14 13.19 |
3267 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. It was later named after American astronomer Eleanor Helin.
Orbit and classification
Glo is an eccentric member of the Phocaea family (701), 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.
The body's observation arc begins with its official discovery observation at Anderson Mesa in January 1981.
Physical characteristics
The asteroid has been characterized as an L- and S-type asteroid by Pan-STARRS large-scale survey.
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, which have very different albedos, from as low as 0.039 to as high as 0.383.
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).
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. 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.
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. The official naming citation was published by the Minor Planet Center on 13 February 1987 (M.P.C. 11641).
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. S2CID 119224590.
- ^ 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 2014). "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.
- "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.
External links
- Pravec, P.; Wolf, M.; Sarounova, L. (2006) http://www.asu.cas.cz/~ppravec/neo.htm
- Asteroid Lightcurve Database (LCDB), query form (info Archived 16 December 2017 at the Wayback Machine)
- Dictionary of Minor Planet Names, Google books
- Asteroids and comets rotation curves, CdR – Observatoire de Genève, Raoul Behrend
- Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
- 3267 Glo at AstDyS-2, Asteroids—Dynamic Site
- 3267 Glo at the JPL Small-Body Database
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