11755 Paczynski
| Discovery | |
|---|---|
| Discovered by | C. J. van Houten, I. van Houten-Groeneveld and T. Gehrels |
| Discovery site | Palomar Observatory |
| Discovery date | 24 September 1960 |
| Designations | |
| MPC designation | 11755 |
Named after | Bohdan Paczyński |
| 2691 P-L | |
| Orbital characteristics[1] | |
| Epoch 13 January 2016 (JD 2457400.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 22198 days (60.77 yr) |
| Aphelion | 2.7490988 AU (411.25933 Gm) |
| Perihelion | 2.0191137 AU (302.05511 Gm) |
| 2.384106 AU (356.6572 Gm) | |
| Eccentricity | 0.1530941 |
| 3.68 yr (1344.6 d) | |
| 141.82520° | |
| 0° 16m 3.869s / day | |
| Inclination | 2.823397° |
| 32.69826° | |
| 192.36603° | |
| Earth MOID | 1.00938 AU (151.001 Gm) |
| Jupiter MOID | 2.2298 AU (333.57 Gm) |
| Jupiter Tisserand parameter | 3.519 |
| Physical characteristics | |
| 14.7 | |
|
| |
11755 Paczynski (2691 P-L) is a main-belt asteroid discovered on September 24, 1960, by C. J. van Houten and I. van Houten-Groeneveld on Palomar Schmidt plates taken by T. Gehrels.
Polish-born astrophysicist Bohdan Paczyński (b. 1940), at Princeton University since 1982, is known for his theoretical work on gamma ray bursters---he was an early proponent of their being at cosmological distances---and for leading searches for gravitational lensing by low-mass stars and substellar objects.[2]
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