| Discovery [1] | |
|---|---|
| Discovered by | C. S. Shoemaker E. M. Shoemaker |
| Discovery site | Palomar Obs. |
| Discovery date | 25 September 1987 |
| Designations | |
| (4450) Pan | |
| Pronunciation | /ˈpæn/[2] |
Named after | Pan (Greek deity)[3] |
| 1987 SY · 1937 CA | |
| NEO · Apollo · PHA [1][4] | |
| Orbital characteristics [1] | |
| Epoch 4 September 2017 (JD 2458000.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 78.85 yr (28,799 days) |
| Earliest precovery date | 6 February 1937 |
| Aphelion | 2.2884 AU |
| Perihelion | 0.5962 AU |
| 1.4423 AU | |
| Eccentricity | 0.5866 |
| 1.73 yr (633 days) | |
| 152.71° | |
| 0° 34m 8.4s / day | |
| Inclination | 5.5196° |
| 311.84° | |
| 291.79° | |
| Earth MOID | 0.0287 AU · 11.2 LD |
| Physical characteristics | |
| 1.0±0.2km[5] 1.13 km (calculated)[6] | |
| 3.51±0.02 h[7] 56.48±0.02h[8] 60±12h[a] | |
| 0.20 (assumed)[6] | |
| S [6] | |
| 17.1[1][6] · 17.43±0.07[5] | |
4450 Pan (prov. designation: 1987 SY) is a highly eccentric asteroid and contact binary, classified as a potentially hazardous asteroid and near-Earth object of the Apollo group, approximately 1.1 kilometers in diameter. It was discovered on 25 September 1987, by American astronomers Eugene and Carolyn ShoemakeratPalomar Observatory in California, United States.[4] It was named after Pan from Greek mythology.[3]
This minor planet was named after Pan, the Greek god of nature, shepherds of flocks and wild animals.[3] In art, he was represented as a horned half-man, half goat. Pan was worshiped by the citizens of Athens, after he had inspired panic in the hearts of their Persians enemies in the Battle of Marathon (also see 4356 Marathon). The modern word "panic" origins from this myth. The name Pan has also been given to Saturn XVIII, one of the moons of Saturn.[3] The official naming citation was published by the Minor Planet Center on 30 January 1991 (M.P.C. 17657).[9]
Pan orbits the Sun in the inner main-belt at a distance of 0.6–2.3 AU once every 1 years and 9 months (633 days). Its orbit has an eccentricity of 0.59 and an inclination of 6° with respect to the ecliptic.[1]
As an Apollo asteroid, it is an Earth-crosser and has a minimum orbit intersection distance with Earth of 0.0287 AU (4,290,000 km), which corresponds to 11.2 lunar distances. Due to its extremely eccentric orbit, it is also a Venus- and Mars-crosser and approaches Mercury within 20 Gm.
It was first observed as 1937 CAatHeidelberg Observatory in 1937. The body's observation arc begins at Palomar with its official discovery observation.[4]
Pan is an assumed stony S-type asteroid.[6]
Pan is a contact binary, composed of two lobes in mutual contact, held together only by their weak gravitational attraction, and typically show a dumbbell-like shape (also see 4769 Castalia).[10] A large number of near-Earth objects are thought to be contact binaries.[11]
The Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 1.1 kilometers,[6] while photometric observations by Italian Albino Carbognani at Saint-Barthelemy Observatory (B04) gave a diameter of 1.0±0.2 kilometers.[5]
In September 2013, a rotational lightcurveofPan was obtained from photometric observations by American astronomer Brian Warner at his Palmer Divide Station (716) in Colorado. It gave a long rotation periodof56.48±0.02 hours with a brightness variation of 0.64 in magnitude (U=3).[8]
The results supersedes two previous observations by Petr PravecatSilvano Casulli that gave a period of 60±12 and 3.51±0.02 hours, respectively (U=2/1).[a][7]
