The Hygiea or Hygiean family of asteroids is a grouping of dark, carbonaceous C-type and B-type asteroids in outer asteroid belt, the largest member of which is 10 Hygiea. About 1% of all known asteroids in the asteroid belt belong to this family.
By far the largest member is 10 Hygiea, a 400 km diameter C-type asteroid that is the fourth largest in the belt. The remaining members are much smaller so Hygiea contains about 94–98% of the mass in the family (depending on the exact criteria for inclusion). The two next largest members are 333 Badenia, and 538 Friederike, both just over 70 km in diameter. After that, the remaining members have diameters of less than 30 km.
The Hygiea family is thought to be of the cratering type, implying that it was formed as a result of a giant impact that excavated the much smaller family members from Hygiea (Zappala 1995, Farinella 1996). However, the two 70-kilometer-diameter bodies are still surprisingly large to have been excavated in an impact that did not disrupt the parent body (compare e.g. to the Vesta family, which contains no members above around 10 km in diameter). They may be interlopers (see below) despite having a similar spectral type to Hygiea, because dark carbonaceous asteroids dominate the outer asteroid belt.
There are some indications that this family is relatively quite old (Tanga 1999)[clarification needed].
Location and size
A HCM numerical analysis by (Zappala 1995) found a 'core' group of family members, whose proper orbital elements lie in the approximate ranges
The 1995 analysis by Zappalà found 103 core members, whereas a search of a recent proper element database (AstDys)for 96944 minor planets in 2005 yielded 1043 objects lying within the rectangular-shaped region defined by the first table above. This would give about 1% of all asteroids in the asteroid belt.
This family contains quite a large number of identified interlopers. The following have been identified in a spectral survey (Mothé-Diniz 2001), and also by inspection of the PDS asteroid taxonomy data set for S- and D-type members: 100 Hekate, 108 Hecuba, 1109 Tata, 1209 Pumma, and 1599 Giomus.
In fact, some of the other asteroids of the C spectral type are probably interlopers as well, due to the prevalence of this spectral type in the region. Possible candidates include 333 Badenia and 538 Friederike, based on their unusually large size for cratering family members.
52 Europa, a very large 300 km diameter asteroid orbits nearby with a proper inclination of 6.37°, and was sometimes considered part of the Hygiea family in the past, but it is an unrelated asteroid. A better sampling of asteroids in the area in recent years has clearly shown that it orbits well beyond the Hygiea family clump.
- V. Zappalà, Ph. Bendjoya, A. Cellino, P. Farinella and C. Froeschlé, Asteroid Families: Search of a 12,487-Asteroid Sample Using Two Different Clustering Techniques, Icarus, Volume 116, Issue 2 (August 1995), pages 291-314
- P. Farinella, D.R. Davia and F. Marzari, Asteroid Families, Old and Young, ASP Conference Series, Vol. 107, p. 45 (1996).
- T. Mothé-Diniz et al. Rotationally Resolved Spectra of 10 Hygiea and a Spectroscopic Study of the Hygiea Family, Icarus, Vol. 152, p. 117 (2001).
- P. Tanga et al. On the Size Distribution of Asteroid Families: The Role of Geometry, Icarus, Vol. 141, p. 65 (1999).
- AstDys site. Proper elements for 96944 numbered minor planets.