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

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

515 Athalia

Minor planet (asteroid)


Minor planet (asteroid)

FieldValue
minorplanetyes
name515 Athalia
background#D6D6D6
discovery_ref
discovererM. F. Wolf
discovery_siteHeidelberg Obs.
discovered20 September 1903
mpc_name(515) Athalia
alt_names1903 ME1931 TQ
1937 WO1937 WQ
1937 WR1937 YH
1953 TD
1977 CF
pronounced
named_afterAthaliah
(ancient queen consort)
mp_categorymain-belt(outer)
Themis
orbit_ref
epoch4 September 2017 (JD 2458000.5)
uncertainty0
observation_arc113.79 yr (41,562 days)
aphelion3.6671 AU
perihelion2.5797 AU
semimajor3.1234 AU
eccentricity0.1741
period5.52 yr (2,016 days)
mean_anomaly178.72°
mean_motion/ day
inclination2.0376°
asc_node121.11°
arg_peri300.16°
dimensionskm
km
38.22 km (SIMPS)
km
km
km
km
km
rotationh
albedo
0.0390 (SIMPS)
spectral_typeTholen no classification possible
SMASS Cb
B–V 0.875
U–B 0.415
abs_magnitude10.610.8911.23

1937 WO1937 WQ 1937 WR1937 YH 1953 TD 1977 CF (ancient queen consort) Themis km 38.22 km (SIMPS) km km km km km

0.0390 (SIMPS)

SMASS Cb B–V 0.875 U–B 0.415

515 Athalia, provisional designation , is a carbonaceous Themistian asteroid from the outer regions of the asteroid belt, approximately 40 kilometers in diameter. It was discovered on 20 September 1903, by German astronomer Max Wolf at the Heidelberg Observatory in southwest Germany. The asteroid was named after the ancient Judahite queen Athaliah.

Orbit and classification

Athalia is a Themistian asteroid that belongs to the Themis family (602), a very large family of carbonaceous asteroids, named after 24 Themis. It orbits the Sun in the outer main belt at a distance of 2.6–3.7 AU once every 5 years and 6 months (2,016 days). Its orbit has an eccentricity of 0.17 and an inclination of 2°. The body's observation arc begins at Heidelberg with its official discovery observation in 1903.

Physical characteristics

Spectral type

In the SMASS classification, the asteroid is a Cb-subtype, that transitions between the carbonaceous C-type to the B-type asteroids. In the Tholen classification, no type could be assigned to Athalia since its spectrum was inconsistent as it resembled that of an S-type asteroid, while its albedo was far too low for that spectral type.

Rotation period

In October 2015, a rotational lightcurve of Athalia was obtained from photometric observations by American astronomer Frederick Pilcher at the Organ Mesa Observatory (G50) in New Mexico, United States. Lightcurve analysis gave a well-defined rotation period of 10.636 hours with a brightness amplitude of 0.22 magnitude ().

Diameter and albedo

According to the surveys carried out by the Japanese Akari satellite, the Spitzer Space Telescope and the Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Athalia measures about 40 kilometers in diameter and its surface has an albedo of about 0.03 to 0.04.

The Collaborative Asteroid Lightcurve Link adopts the results obtained by the Infrared Astronomical Satellite IRAS, that is, an albedo of 0.039 and a diameter of 38.22 kilometers based on an absolute magnitude of 11.23.

Naming

This minor planet was named after Athaliah (Athalia), the daughter of King Ahab and Queen Jezebel of Israel. The murderous queen of the ancient Kingdom of Judah was the only woman to ever rule the Hebrew kingdoms. The official naming citation was mentioned in The Names of the Minor Planets by Paul Herget in 1955 (H 55).

References

References

  1. 'Athaliah' in Noah Webster (1884) ''A Practical Dictionary of the English Language''
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 515 Athalia — 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