From Surf Wiki (app.surf) — the open knowledge base
1532 Inari
Main-belt asteroid discovered on 1938-09-16 by Yrjö Väisälä at Turku
Main-belt asteroid discovered on 1938-09-16 by Yrjö Väisälä at Turku
| Field | Value |
|---|---|
| minorplanet | yes |
| name | 1532 Inari |
| background | #D6D6D6 |
| discovery_ref | |
| discoverer | Y. Väisälä |
| discovery_site | Turku Obs. |
| discovered | 16 September 1938 |
| mpc_name | (1532) Inari |
| alt_names | 1938 SM1933 SZ |
| 1935 BJ | |
| named_after | Lake Inari (Finnish lake) |
| mp_category | main-belt(outer) |
| Eos | |
| orbit_ref | |
| epoch | 4 September 2017 (JD 2458000.5) |
| uncertainty | 0 |
| observation_arc | 80.74 yr (29,492 days) |
| aphelion | 3.1618 AU |
| perihelion | 2.8486 AU |
| semimajor | 3.0052 AU |
| eccentricity | 0.0521 |
| period | 5.21 yr (1,903 days) |
| mean_anomaly | 325.80° |
| mean_motion | / day |
| inclination | 8.7769° |
| asc_node | 330.63° |
| arg_peri | 122.85° |
| dimensions | km |
| km | |
| 28.38 km (derived) | |
| km | |
| km | |
| rotation | h |
| albedo | |
| 0.1049 (derived) | |
| spectral_type | Tholen S |
| B–V 0.840 | |
| U–B 0.360 | |
| abs_magnitude | 10.810.8611.50 |
1935 BJ Eos km 28.38 km (derived) km km
0.1049 (derived) B–V 0.840 U–B 0.360
1532 Inari (provisional designation ****) is a stony Eoan asteroid from the outer regions of the asteroid belt, approximately 28 kilometers in diameter. Discovered by Yrjö Väisälä at Turku Observatory in 1938, it was later named for Lake Inari in northern Finland.
Discovery
Inari was discovered on 16 September 1938, by Finnish astronomer Yrjö Väisälä at the Iso-Heikkilä Observatory near Turku, Finland. The asteroid was first identified as at Simeiz Observatory in September 1933, and its observation arc begins at Nice Observatory in April 1936, more than two years prior to its official discovery observation at Turku.
Orbit and classification
Inari is a member the Eos family (606), one of the asteroid belt's largest families with nearly 10,000 known asteroids. It orbits the Sun in the outer main belt at a distance of 2.8–3.2 AU once every 5 years and 3 months (1,903 days). Its orbit has an eccentricity of 0.05 and an inclination of 9° with respect to the ecliptic.
Physical characteristics
In the Tholen classification, Saimaa is a featureless stony S-type asteroid. The overall spectral type for members of the Eos family is that of a K-type.
Rotation period
In January 2008, a fragmentary rotational lightcurve of Inari was obtained from photometric observations by French amateur astronomer René Roy. Lightcurve analysis gave a longer-than-average rotation period of 25 hours with a low brightness amplitude of 0.09 magnitude (). As of 2017, no secure period has been obtained.
Diameter and albedo
According to the surveys carried out by the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Inari measures between 24.439 and 30.39 kilometers in diameter and its surface has an albedo between 0.060 and 0.087. The Collaborative Asteroid Lightcurve Link derives an albedo of 0.1049 and a diameter of 28.38 kilometers based on an absolute magnitude of 10.8.
Naming
This minor planet was named after Lake Inari (Inarijärvi), located north of the Arctic Circle in Lapland, Finland. Lake Inari is the country's third-largest lake and one of the largest lakes in Europe.
The official was published by the Minor Planet Center on 20 February 1976 (M.P.C. 3929).
References
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 1532 Inari — 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