| Minorplanet: | yes |
| 1870 Glaukos | |
| Background: |
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| Discovered: | 24 March 1971 |
| Mpc Name: | (1870) Glaukos |
| Alt Names: | 1971 FE1976 SM |
| Adjective: | Glaukian |
| Pronounced: | [1] |
| Named After: | Glaucus |
| Mp Category: | Jupiter trojan |
| Epoch: | 23 March 2018 (JD 2458200.5) |
| Uncertainty: | 0 |
| Observation Arc: | 62.50 yr (22,827 d) |
| Perihelion: | 5.0765 AU |
| Semimajor: | 5.2460 AU |
| Eccentricity: | 0.0323 |
| Period: | 12.02 yr (4,389 d) |
| Mean Motion: | / day |
| Inclination: | 6.5763° |
| Asc Node: | 176.30° |
| Arg Peri: | 129.91° |
| Jupiter Moid: | 0.1272 AU |
| Tisserand: | 2.9860 |
| Abs Magnitude: | 10.5 10.6 |
1870 Glaukos is a mid-sized Jupiter trojan from the Trojan camp, approximately 47km (29miles) in diameter. Discovered during the first Palomar–Leiden Trojan survey in 1971, it was later named for Glaucus from Greek mythology. The dark D-type asteroid has a rotation period of 6.0 hours.
Glaukos was discovered on 24 March 1971, by Dutch astronomer couple Ingrid and Cornelis van Houten at Leiden, on photographic plates taken by astronomer Tom Gehrels at the Californian Palomar Observatory in California. The body's observation arc begins with a precovery of its first recorded observation at Palomar in November 1955, or more than 15 years prior to its official discovery observation.
This discovery was made in the context of a larger survey of faint Trojans. The trio of Dutch and Dutch–American astronomers also collaborated on the productive Palomar–Leiden survey in the 1960s, using the same procedure as for this (smaller) survey: Tom Gehrels used Palomar's Samuel Oschin telescope (also known as the 48-inch Schmidt Telescope), and shipped the photographic plates to Cornelis and Ingrid van Houten at Leiden Observatory where astrometry was carried out.
More than 7000 Jupiter trojans have already been discovered.
Glaukos is a dark Jovian asteroid in a 1:1 orbital resonance with Jupiter. It is located in the trailing Trojan camp at the Gas Giant's Lagrangian point, 60° behind its orbit . It is also a non-family asteroid of the Jovian background population. It orbits the Sun at a distance of 5.1–5.4 AU once every 12.02 years (4,389 days; semi-major axis of 5.25 AU). Its orbit has an eccentricity of 0.03 and an inclination of 7° with respect to the ecliptic.
Glaukos has been characterized as a dark D-type asteroid by PanSTARRS photometric survey as well as in the SDSS-based taxonomy. It is the most common spectral type among the Jupiter trojans.
In 2012 and 2013, three rotational lightcurves of Glaukos in the R- and S-band were obtained by astronomers at the Palomar Transient Factory in California. Lightcurve analysis gave a rotation period of 5.979, 5.980 and 5.989 hours with an amplitude between 0.27 and 0.37 magnitude .
In October 2013, photometric observations by American astronomer Robert Stephens at the Center for Solar System Studies gave the so-far best rated lightcurve, with a period of hours and a brightness variation of 0.42 magnitude .
According to the survey carried out by NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Glaukos measures 47.65 kilometers in diameter, and its surface has an albedo of 0.049, while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for a carbonaceous asteroid of 0.057 and calculates a diameter of 42.23 kilometers with an absolute magnitude of 10.6.
This minor planet was named after Glaucus (Glaukos) from Greek mythology. In Homer's Iliad, he was captain in the Lycian contingent during the Trojan War. and was killed by Ajax, after whom the Jovian asteroid 1404 Ajax is named. The official was published by the Minor Planet Center on 1 June 1975 .