From Surf Wiki (app.surf) — the open knowledge base
881 Athene
Stony background asteroid
Stony background asteroid
| Field | Value | |||
|---|---|---|---|---|
| minorplanet | yes | |||
| name | 881 Athene | |||
| background | #D6D6D6 | |||
| image | 000881-asteroid shape model (881) Athene.png | |||
| caption | Modelled shape of Athene from its lightcurve | |||
| discovery_ref | ||||
| discoverer | M. F. Wolf | |||
| discovery_site | Heidelberg Obs. | |||
| discovered | 22 July 1917 | |||
| mpc_name | (881) Athene | |||
| alt_names | A917 OD1917 CL | |||
| pronounced | ||||
| adjective | Athenian | |||
| named_after | Goddess Athena | |||
| (Greek mythology) | ||||
| mp_category | {{plainlist | |||
| * main-belt<ref name | "MPC-object" /(middle) | |||
| * background<ref name | "AstDys-object" /}} | |||
| orbit_ref | ||||
| epoch | 31 May 2020 (JD 2459000.5) | |||
| uncertainty | 0 | |||
| observation_arc | 102.53 yr (37,449 d) | |||
| aphelion | 3.1510 AU | |||
| perihelion | 2.0764 AU | |||
| semimajor | 2.6137 AU | |||
| eccentricity | 0.2056 | |||
| period | 4.23 yr (1,543 d) | |||
| mean_anomaly | 121.30° | |||
| mean_motion | / day | |||
| inclination | 14.191° | |||
| asc_node | 277.03° | |||
| arg_peri | 41.313° | |||
| mean_diameter | {{plainlist | |||
| * {{val | 12.04 | 0.28 | ul | km}} |
| * {{val | 12.153 | 0.101 | u | km}} |
| rotation | }} | |||
| pole_ecliptic_lat | {{plainlist | |||
| * (123.0°, −58.0°) (λ<sub>1</sub>/β<sub>1</sub>)<ref name | "Ferret" / | |||
| * {{nowrap | (337.0°, −47.0°) (λ<sub>2</sub>/β<sub>2</sub>)<ref name | "Ferret" /}}}} | ||
| albedo | {{plainlist | |||
| * <ref name | "Masiero-2014" / | |||
| * <ref name | "AKARI" /}} | |||
| spectral_type | {{plainlist | |||
| * S <ref name | "Lazzaro-2004" / | |||
| * Sl <ref name | "Lazzaro-2004" / | |||
| * L <ref name | "SDSS-Taxonomy" /}} | |||
| abs_magnitude | 11.8 |
(Greek mythology)
- main-belt(middle)
- background}}
- (123.0°, −58.0°) (λ1/β1)
- (337.0°, −47.0°) (λ2/β2)}}
- }}
- S (S3OS2-TH)
- Sl (S3OS2-BB)
- L (SDSS-MOC)}}
881 Athene (prov. designation: or ) is a stony background asteroid from the central region of the asteroid belt. It was discovered on 22 July 1917, by astronomer Max Wolf at the Heidelberg-Königstuhl State Observatory in southwest Germany. The likely elongated S/L-type asteroid has a rotation period of 13.9 hours and measures approximately 12 km in diameter. It was named after Athena, the goddess of wisdom in Greek mythology. According to Astrophysicist Rayme Traub at JHU APL NASA, Europa Clipper will make a pass by Athene in 2027 after passing Earth on its way to Jupiter. Europa Clipper will test its sensors on Athene in preparation for Europa in 2030.
Orbit and classification
Located in or near the orbital region of the Eunomia family, Athene is a non-family asteroid of the main belt's background population when applying the hierarchical clustering method to its proper orbital elements. It orbits the Sun in the central asteroid belt at a distance of 2.1–3.2 AU once every 4 years and 3 months (1,543 days; semi-major axis of 2.61 AU). Its orbit has an eccentricity of 0.21 and an inclination of 14° with respect to the ecliptic. The body's observation arc begins at Uccle Observatory on 8 August 1934, almost 17 years after its official discovery observation at Heidelberg on 22 July 1917.
Naming
This minor planet was named after Athena or "Pallas Athene", the goddess of wisdom in Greek mythology, also known as Minerva in Roman mythology. The was mentioned in The Names of the Minor Planets by Paul Herget in 1955 (H 86). Asteroids 93 Minerva and 2 Pallas are both named after the goddess as well.
Physical characteristics
In the Tholen-like taxonomy of the Small Solar System Objects Spectroscopic Survey (S3OS2), Athene is a common, stony S-type asteroid, while in the SDSS-based taxonomy, it is an L-type asteroid. In the SMASS-like taxonomic variant of the S3OS2, Athene is an Sl-subtype that transitions between the S-and L-type.
Rotation period
In August 2006, a rotational lightcurve of Athene was obtained from photometric observations by Roberto Crippa and Federico Manzini at the Sozzago Astronomical Station , Italy, and by Jean-Gabriel Bosch at the Collonges Observatory , France. Lightcurve analysis gave a rotation period of hours with a high brightness variation of magnitude, indicative of a non-spherical, elongated shape (). In September 2010, French amateur astronomer René Roy measured a similar period of hours and an amplitude of ().
Poles
Two lightcurves, published in 2016, using modeled photometric data from the Lowell Photometric Database (LPD) and other sources, gave a concurring sidereal period of and hours, respectively. Each modeled lightcurve also determined two spin axes of (123.0°, −58.0°) and (337.0°, −47.0°), as well as (115.0°, −77.0°) and (338.0°, −43.0°) in ecliptic coordinates (λ, β).
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 (WISE), Athene measures () and () kilometers in diameter and its surface has an albedo of () and (), respectively. The Collaborative Asteroid Lightcurve Link assumes a standard Eunomian albedo of 0.21 and calculates a diameter of 12.66 kilometers based on an absolute magnitude of 11.8. Alternative mean diameter measurements published by the WISE team include (), () and () with corresponding albedos of (), () and ().
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 881 Athene — 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