Skip to content
Surf Wiki
Save to docs
general/eunomia-asteroids

From Surf Wiki (app.surf) — the open knowledge base

2181 Fogelin

Asteroid


Asteroid

FieldValue
minorplanetyes
name2181 Fogelin
background#D6D6D6
image002181-asteroid shape model (2181) Fogelin.png
captionShape model of *Fogelin* from its lightcurve
discovery_ref
discovererK. Reinmuth
discovery_siteHeidelberg Obs.
discovered28 December 1942
mpc_name(2181) Fogelin
alt_names1942 YA
named_afterEric S. Fogelin
(MPC staff member)
mp_categorymain-belt(middle)
Eunomia
orbit_ref
epoch23 March 2018 (JD 2458200.5)
uncertainty0
observation_arc75.08 yr (27,422 d)
aphelion2.8986 AU
perihelion2.2836 AU
semimajor2.5911 AU
eccentricity0.1187
period4.17 yr (1,523 d)
mean_anomaly354.25°
mean_motion/ day
inclination13.007°
asc_node17.286°
arg_peri116.18°
mean_diameter
(calculated)
rotation
albedo
0.21 (assumed)
spectral_typeS (assumed)
abs_magnitude12.012.10

(MPC staff member) Eunomia

(calculated) 0.21 (assumed)

2181 Fogelin (prov. designation: ) is an Eunomia asteroid from the central regions of the asteroid belt, approximately 11 km in diameter. It was discovered on 28 December 1942, by Germany astronomer Karl Reinmuth at the Heidelberg Observatory in southwest Germany. In 1980, it was named for Eric S. Fogelin an assistant at the Minor Planet Center. The likely elongated S-type asteroid has a rotation period of 14.07 hours.

Orbit and classification

Fogelin is a member of the Eunomia family (502), a prominent family of stony asteroid and the largest one in the intermediate main belt with more than 5,000 known members. It orbits the Sun in the central main-belt at a distance of 2.3–2.9 AU once every 4 years and 2 months (1,523 days; semi-major axis of 2.59 AU). Its orbit has an eccentricity of 0.12 and an inclination of 13° with respect to the ecliptic. The body's observation arc begins at Heidelberg with its official discovery observation in December 1942.

Naming

This minor planet was named by Brian Marsden and Conrad Bardwell of the Minor Planet Center, after their assistant, Eric S. Fogelin. During 1979–1980, he was preparing the center's computerized data and helped publishing the Minor Planet Circulars. The official naming citation was published by the Minor Planet Center on 1 August 1980 (M.P.C. 5451).

Physical characteristics

Fogelin is an assumed S-type asteroid, in line with the overall spectral type seen among Eunomian asteroids. Near-IR spectroscopy at the NASA Infrared Telescope Facility with the SpeX instrument showed that the asteroid contains mafic minerals, which are rich in magnesium and iron.

Rotation period

In March 2010, a rotational lightcurve of Fogelin was obtained from photometric observations by Richard Durkee at the Shed of Science Observatory in the United States. Lightcurve analysis gave a well-defined rotation period of 14.07 hours with a brightness amplitude of 0.57 magnitude, indicative of an elongated shape ().

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, Fogelin measures between 10.067 and 11.29 kilometers in diameter and its surface has an albedo between 0.200 and 0.252. The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.21 – derived from 15 Eunomia, the family's parent body and namesake – and calculates a diameter of 11.55 kilometers based on an absolute magnitude of 12.0.

References

Info: Wikipedia Source

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.

Want to explore this topic further?

Ask Mako anything about 2181 Fogelin — get instant answers, deeper analysis, and related topics.

Research with Mako

Free with your Surf account

Content sourced from Wikipedia, available under CC BY-SA 4.0.

This 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