| Minorplanet: | yes |
| 736 Harvard | |
| Background: |
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| Discovery Ref: |   |
| Discovered: | 16 November 1912 |
| Mpc Name: | (736) Harvard |
| Alt Names: | A912 WC1937 FC 1947 HB1912 PZ |
| Named After: | Harvard University  |
| Mp Category: |
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| Orbit Ref: |   |
| Epoch: | 31 May 2020 (JD 2459000.5) |
| Uncertainty: | 0 |
| Observation Arc: | 106.85 yr (39,027 d) |
| Perihelion: | 1.8382 AU |
| Semimajor: | 2.2018 AU |
| Eccentricity: | 0.1651 |
| Period: | 3.27 yr (1,193 d) |
| Mean Motion: | / day |
| Inclination: | 4.3767° |
| Asc Node: | 135.91° |
| Arg Peri: | 200.51° |
| Mean Diameter: | |
| Albedo: | |
| Spectral Type: |
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| Abs Magnitude: |
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736 Harvard (prov. designation: or) is a stony background asteroid from the inner regions of the asteroid belt, approximately 17km (11miles) in diameter. It was discovered on 16 November 1912, by American astronomer Joel Hastings Metcalf at the Winchester Observatory . The bright S-type asteroid has a rotation period of 6.7 hours. It was named after Harvard University in Cambridge, Massachusetts.
Located in the orbital region of the Flora family, Harvard is a non-family asteroid of the main belt's background population when applying the hierarchical clustering method to its proper orbital elements. It orbits the Sun in the inner asteroid belt at a distance of 1.8–2.6 AU once every 3 years and 3 months (1,193 days; semi-major axis of 2.2 AU). Its orbit has an eccentricity of 0.17 and an inclination of 4° with respect to the ecliptic. The body's observation arc begins at Heidelberg Observatory on 9 December 1912, or three weeks after its official discovery observation by Metcalf at Winchester.
This minor planet was named in honor of the prestigious Harvard University in Cambridge, Massachusetts, United States. The was also mentioned in The Names of the Minor Planets by Paul Herget in 1955 .
In the Tholen classification, Harvard is a common, stony S-type asteroid.
In 1970s, a rotational lightcurve of Harvard was obtained from photometric observations by Ed Tedesco. Lightcurve analysis gave a well-defined rotation period of hours with a brightness variation of magnitude .
According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer (WISE), and the Japanese Akari satellite, Harvard measures, and kilometers in diameter and its surface has an albedo of, and, respectively. The Collaborative Asteroid Lightcurve Link derives an albedo of 0.2051 and a diameter of 16.89 kilometers based on an absolute magnitude of 11.2. An asteroid occultation observed on 25 May 2003, gave a best-fit ellipse dimension of with a low quality rating of 1. These timed observations are taken when the asteroid passes in front of a distant star.
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