Misplaced Pages

325 Heidelberga

Article snapshot taken from Wikipedia with creative commons attribution-sharealike license. Give it a read and then ask your questions in the chat. We can research this topic together.
Main-belt asteroid

325 Heidelberga
Orbital diagram
Discovery
Discovered byMax Wolf
Discovery date4 March 1892
Designations
MPC designation(325) Heidelberga
Pronunciation/ˌhaɪdəlˈbɜːrɡə/
Named afterHeidelberg
Minor planet categoryMain belt
AdjectivesHeidelergian /ˌhaɪdəlˈbɜːrdʒiən, -ɡiən/
Orbital characteristics
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc117.86 yr (43050 d)
Aphelion3.7223 AU (556.85 Gm)
Perihelion2.69998 AU (403.911 Gm)
Semi-major axis3.21115 AU (480.381 Gm)
Eccentricity0.15919
Orbital period (sidereal)5.75 yr (2101.8 d)
Mean anomaly7.2090°
Mean motion0° 10 16.608 / day
Inclination8.5545°
Longitude of ascending node344.881°
Argument of perihelion68.563°
Physical characteristics
Dimensions75.72±1.7 km
Synodic rotation period6.737 h (0.2807 d)
Geometric albedo0.1068±0.005
Absolute magnitude (H)8.65

325 Heidelberga is a large main belt asteroid that was discovered by German astronomer Max Wolf on 4 March 1892 in Heidelberg. It is orbiting the Sun at a distance of 3.21 AU with an eccentricity (oval shape) of 0.159. The orbital plane is inclined at an angle of 8.55° to the ecliptic.

Based upon its spectrum, 325 Heidelberga is classified as an M-type asteroid. No absorption features have been detected with certainty, indicating it most likely has a nickel-iron or enstatite chondrite composition. A weak feature in the near infrared spectrum indicates the presence of low-iron orthopyroxene on the asteroid surface.

References

  1. ^ Yeomans, Donald K., "325 Heidelberga", JPL Small-Body Database Browser, NASA Jet Propulsion Laboratory, retrieved 11 May 2016.
  2. Hardersen, Paul S.; Gaffey, Michael J.; Abell, Paul A. (January 1983), "Near-IR spectral evidence for the presence of iron-poor orthopyroxenes on the surfaces of six M-type asteroids", Icarus, vol. 175, no. 1, pp. 141–158, Bibcode:2005Icar..175..141H, doi:10.1016/j.icarus.2004.10.017.
  3. Takir, D.; Hardersen, P. S.; Gaffey, M. J. (March 2008), "The Near-Infrared Spectroscopy of Two M-Class Main Belt Asteroids, 77 Frigga and 325 Heidelberga", 39th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXIX), held March 10–14, 2008 in League City, Texas. LPI Contribution No. 1391, p. 1084, Bibcode:2008LPI....39.1084T

External links

Minor planets navigator
Small Solar System bodies
Minor planets
Asteroid
Distant minor planet
Comets
Other


Stub icon

This article about an asteroid native to the asteroid belt is a stub. You can help Misplaced Pages by expanding it.

Categories: