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6726 Suthers
Main-belt asteroid
Main-belt asteroid
| Field | Value |
|---|---|
| minorplanet | yes |
| name | 6726 Suthers |
| background | #D6D6D6 |
| discovery_ref | |
| discovered | 5 August 1991 |
| discoverer | H. E. Holt |
| discovery_site | Palomar Obs. |
| mpc_name | (6726) Suthers |
| alt_names | 1991 PS |
| named_after | Paul Sutherland |
| (author and journalist) | |
| mp_category | main-belt(inner) |
| background | |
| orbit_ref | |
| epoch | 4 September 2017 (JD 2458000.5) |
| uncertainty | 0 |
| observation_arc | 63.66 yr (23,250 days) |
| aphelion | 2.5004 AU |
| perihelion | 2.0740 AU |
| semimajor | 2.2872 AU |
| eccentricity | 0.0932 |
| period | 3.46 yr (1,263 days) |
| mean_anomaly | 96.351° |
| mean_motion | / day |
| inclination | 4.2993° |
| asc_node | 277.71° |
| arg_peri | 146.31° |
| dimensions | |
| albedo | |
| abs_magnitude | 13.9 |
(author and journalist) background
6726 Suthers, provisional designation **, is a background asteroid from the inner regions of the asteroid belt, approximately 3.5 km in diameter. It was discovered on 5 August 1991, by American astronomer Henry E. Holt at Palomar Observatory in San Diego County, California. The asteroid was named after author Paul Sutherland.
Orbit and classification
Suthers is a non-family asteroid from the main belt's background population. It orbits the Sun in the inner main-belt at a distance of 2.1–2.5 AU once every 3 years and 6 months (1,263 days). Its orbit has an eccentricity of 0.09 and an inclination of 4° with respect to the ecliptic.
Naming
In 2012, this minor planet was officially named after Paul Sutherland, author and journalist, who has actively supported the UK-based Society for Popular Astronomy for many years, and who is known as "Suthers" to friends and colleagues. He is author of Where Did Pluto Go? and responsible for bringing many astronomical stories to a wider public.
Physical characteristics
According to the survey carried out by NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Suthers measures 3.455 kilometers in diameter and its surface has an albedo of 0.207.
References
|archive-url = https://web.archive.org/web/20170312032210/http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2006726 |url-status = dead |archive-date = 12 March 2017 |access-date = 21 June 2017}}
|access-date = 9 March 2017}}
|display-authors = 6 |access-date= 9 March 2017}}
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