| Minorplanet: | yes |
| 1687 Glarona | |
| Background: |
|
| Discovered: | 19 September 1965 |
| Mpc Name: | (1687) Glarona |
| Alt Names: | 1965 SC1926 UA 1942 PD 1945 EA1948 QN 1954 TB 1959 PG 1960 XD1965 UX A909 UAA915 XC |
| Epoch: | 4 September 2017 (JD 2458000.5) |
| Uncertainty: | 0 |
| Observation Arc: | 107.45 yr (39,245 days) |
| Perihelion: | 2.6004 AU |
| Semimajor: | 3.1576 AU |
| Eccentricity: | 0.1765 |
| Period: | 5.61 yr (2,049 days) |
| Mean Motion: | / day |
| Inclination: | 2.6367° |
| Asc Node: | 93.570° |
| Arg Peri: | 316.57° |
| Dimensions: | km km km km |
| Rotation: | h h |
| Albedo: | |
| Spectral Type: | S B–V = 0.670 U–B = 0.380 |
| Abs Magnitude: | 10.25 |
1687 Glarona (prov. designation:) is a stony Themis asteroid approximately 34 kilometers in diameter from the outer region of the asteroid belt. It was discovered by Swiss astronomer Paul Wild at Zimmerwald Observatory near Bern, Switzerland, on 19 September 1965. It was later named after the Swiss Canton of Glarus.
The asteroid is a member of the Themis family, one of the larger groups in the outer main-belt. It orbits the Sun at a distance of 2.6–3.7 AU once every 5 years and 7 months (2,049 days). Its orbit has an eccentricity of 0.18 and an inclination of 3° with respect to the ecliptic. The first precovery was taken at Heidelberg Observatory in 1909, extending the asteroid's observation arc by 56 years prior to its discovery.
The minor planet was named for of the discoverer's home valley, the Swiss Canton of Glarus and its capital Glarus. Paul Wild (1925–2014) was a prolific discoverer almost 100 asteroids, and is well known for his discovery of comet Wild 2, which was visited by NASA's Stardust mission. The official was published by the Minor Planet Center on 1 October 1969 .
A rotational lightcurve obtained in the 1970s gave a well-defined rotation period of 6.3 hours with a brightness amplitude of 0.75 in magnitude . In March 2016, a second period was published based on data from the Lowell Photometric Database (LPD). Using lightcurve inversion and convex shape models, as well as distributed computing power and the help of individual volunteers, a period of hours could be obtained for this asteroid from the LPD's sparse-in-time photometry data .
According to the space-based surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite, and NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, the asteroid measures between 31.5 and 42.0 kilometers in diameter and its surface has an albedo in the range of 0.0795 to 0.141.
The Collaborative Asteroid Lightcurve Link (CALL) gives preference to the results obtained by IRAS with an albedo of 0.1219 and a diameter of 33.93 kilometers. CALL also classifies the Themistian asteroid as a stony S-class body, which are otherwise known to have low albedos, showing spectra of carbonaceous C-type bodies (also see Carbonaceous chondrites).