From Surf Wiki (app.surf) — the open knowledge base
9994 Grotius
Rafita asteroid
Rafita asteroid
| Field | Value |
|---|---|
| minorplanet | yes |
| name | 9994 Grotius |
| background | #D6D6D6 |
| image | AnimatedOrbitOf9994Grotius.gif |
| caption | |
| discovery_ref | |
| discovered | 24 September 1960 |
| discoverer | C. J. van Houten |
| I. van Houten-G. | |
| T. Gehrels | |
| discovery_site | Palomar Obs. |
| mpc_name | (9994) Grotius |
| alt_names | 4028 P-L |
| pronounced | |
| named_after | Hugo Grotius |
| (Dutch jurist) | |
| mp_category | main-belt(middle) |
| Rafita | |
| orbit_ref | |
| epoch | 4 September 2017 (JD 2458000.5) |
| uncertainty | 0 |
| observation_arc | 55.59 yr (20,306 days) |
| aphelion | 3.0391 AU |
| perihelion | 2.1307 AU |
| semimajor | 2.5849 AU |
| eccentricity | 0.1757 |
| period | 4.16 yr (1,518 days) |
| mean_anomaly | 204.01° |
| mean_motion | / day |
| inclination | 7.1806° |
| asc_node | 207.15° |
| arg_peri | 224.33° |
| dimensions | 3.38 km (calculated) |
| km | |
| rotation | h |
| albedo | 0.20 (assumed) |
| spectral_type | S |
| abs_magnitude | 14.2 (R)14.314.72 |
I. van Houten-G. T. Gehrels (Dutch jurist) Rafita km
9994 Grotius , provisional designation , is a stony Rafita asteroid from the middle regions of the asteroid belt, approximately 3.5 kilometers in diameter. It was discovered during the Palomar–Leiden survey in 1960, and named after Dutch jurist Hugo Grotius.
Discovery
Grotius was discovered on 24 September 1960, by the Dutch astronomers Ingrid and Cornelis van Houten, on photographic plates taken by Dutch–American astronomer Tom Gehrels at Palomar Observatory in California, United States.
Survey designation
The survey designation "P-L" stands for Palomar–Leiden, named after Palomar Observatory and Leiden Observatory, which collaborated on the fruitful Palomar–Leiden survey in the 1960s. Gehrels used Palomar's Samuel Oschin telescope (also known as the 48-inch Schmidt Telescope), and shipped the photographic plates to Ingrid and Cornelis van Houten at Leiden Observatory where astrometry was carried out. The trio are credited with the discovery of several thousand minor planets.
Orbit and classification
Grotius orbits the Sun in the central main-belt at a distance of 2.1–3.0 AU once every 4 years and 2 months (1,518 days). Its orbit has an eccentricity of 0.18 and an inclination of 7° with respect to the ecliptic. The body's observation arc begins with its official discovery observation at Palomar.
Rotation period
In August 2010, a rotational lightcurve of Grotius was obtained from photometric observations in the R-band at the Palomar Transient Factory in California. Lightcurve analysis gave a rotation period of 9.2189 hours with a brightness variation of 0.27 magnitude ().
Diameter and albedo
According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Grotius measures 3.746 kilometers in diameter and its surface has an albedo of 0.263. The Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 3.38 kilometers based on an absolute magnitude of 14.72.
Naming
This minor planet was named for Dutch jurist Hugo Grotius (1583–1645), who laid the foundations for international law, based on natural law. He was a child prodigy and entered Leiden University when he was just eleven years old. The approved naming citation was published by the Minor Planet Center on 11 November 2000 (M.P.C. 41571).
References
References
- Noah Webster (1884) ''A Practical Dictionary of the English Language''
This article was imported from Wikipedia and is available under the Creative Commons Attribution-ShareAlike 4.0 License. Content has been adapted to SurfDoc format. Original contributors can be found on the article history page.
Ask Mako anything about 9994 Grotius — get instant answers, deeper analysis, and related topics.
Research with MakoFree with your Surf account
Create a free account to save articles, ask Mako questions, and organize your research.
Sign up freeThis content may have been generated or modified by AI. CloudSurf Software LLC is not responsible for the accuracy, completeness, or reliability of AI-generated content. Always verify important information from primary sources.
Report