Asteroid family
An asteroid family is a population of asteroids that share similar proper orbital elements, such as semi-major axis, eccentricity, and orbital inclination. The members of the families are thought to be fragments of past asteroid collisions. An asteroid family is a more specific term than asteroid group, whose members, while sharing some broad orbital characteristics, may be otherwise unrelated to each other.
Image:Asteroid proper elements i vs e.png|thumb|300px|Plot of proper inclination vs. eccentricity for numbered asteroids
Large prominent families contain several hundred recognized asteroids. Small, compact families may have only about ten identified members. About 33% to 35% of asteroids in the main belt are family members. There are about 20 to 30 reliably recognized families, with several tens of less certain groupings. Most asteroid families are found in the main asteroid belt, although several family-like groups such as the Pallas family, Hungaria family, and the Phocaea family lie at smaller semi-major axis or larger inclination than the main belt.
One family has been identified associated with the dwarf planet. Some studies have tried to find evidence of collisional families among the trojan asteroids, but at present the evidence is inconclusive.
History
The Japanese astronomer Kiyotsugu Hirayama pioneered the estimation of proper elements for asteroids, and first identified several of the most prominent families in 1918. Kiyotsugu Hirayama initially identified the Koronis, Eos, and Themis families, and later recognized also the Flora and Maria families. In his honor, asteroid families are sometimes called Hirayama families. This particularly applies to the five prominent groupings discovered by him.Origin and evolution
The families are thought to form as a result of collisions between asteroids. In many or most cases the parent body was shattered, but there are also several families which resulted from a large cratering event which did not disrupt the parent body. Such cratering families typically consist of a single large body and a swarm of asteroids that are much smaller. Some families have complex internal structures which are not satisfactorily explained at the moment, but may be due to several collisions in the same region at different times.Due to the method of origin, all the members have closely matching compositions for most families. Notable exceptions are those families which formed from a large differentiated parent body.
Asteroid families are thought to have lifetimes of the order of a billion years, depending on various factors. This is significantly shorter than the Solar System's age, so few if any are relics of the early Solar System. Decay of families occurs both because of slow dissipation of the orbits due to perturbations from Jupiter or other large bodies, and because of collisions between asteroids which grind them down to small bodies. Such small asteroids then become subject to perturbations such as the Yarkovsky effect that can push them towards orbital resonances with Jupiter over time. Once there, they are relatively rapidly ejected from the asteroid belt. Tentative age estimates have been obtained for some families, ranging from hundreds of millions of years to less than several million years as for the compact Karin family. Old families are thought to contain few small members, and this is the basis of the age determinations.
It is supposed that many very old families have lost all the smaller and medium-sized members, leaving only a few of the largest intact. A suggested example of such old family remains are the 9 Metis and 113 Amalthea asteroid pair. Further evidence for a large number of past families comes from analysis of chemical ratios in iron meteorites. These show that there must have once been at least 50 to 100 parent bodies large enough to be differentiated, that have since been shattered to expose their cores and produce the actual meteorites.
Identification
Strictly speaking, families and their membership are identified by analysing the proper orbital elements rather than the current osculating orbital elements, which regularly fluctuate on timescales of tens of thousands of years. The proper elements are related constants of motion that remain almost constant for at least tens of millions of years, and perhaps longer.Membership
When the orbital elements of main belt asteroids are plotted, a number of distinct concentrations are seen against the rather uniform distribution of non-family background asteroids. These concentrations are the asteroid families. Interlopers are asteroids classified as family members based on their so-called proper orbital elements but having spectroscopic properties distinct from the bulk of the family, suggesting that they, contrary to the true family members, did not originate from the same parent body that once fragmented upon a collisional impact.Family types
As previously mentioned, families caused by an impact that did not disrupt the parent body but only ejected fragments are called cratering families. Other terminology has been used to distinguish various types of groups which are less distinct or less statistically certain from the most prominent "nominal families".The term cluster is also used to describe a small asteroid family, such as the Karin cluster. Clumps are groupings which have relatively few members but are clearly distinct from the background. Clans are groupings which merge very gradually into the background density and/or have a complex internal structure making it difficult to decide whether they are one complex group or several unrelated overlapping groups. Tribes are groups that are less certain to be statistically significant against the background either because of small density or large uncertainty in the orbital parameters of the members.
Hierarchical clustering method
Present day computer-assisted searches have identified more than a hundred asteroid families. The most prominent algorithms have been the hierarchical clustering method, which looks for groupings with small nearest-neighbour distances in orbital element space, and wavelet analysis, which builds a density-of-asteroids map in orbital element space, and looks for density peaks.The boundaries of the families are somewhat vague because at the edges they blend into the background density of asteroids in the main belt. For this reason the number of members even among discovered asteroids is usually only known approximately, and membership is uncertain for asteroids near the edges.
Additionally, some interlopers from the heterogeneous background asteroid population are expected even in the central regions of a family. Since the true family members caused by the collision are expected to have similar compositions, most such interlopers can in principle be recognised by spectral properties which do not match those of the bulk of family members. A prominent example is 1 Ceres, the largest asteroid, which is an interloper in the family once named after it.
Spectral characteristics can also be used to determine the membership of asteroids in the outer regions of a family, as has been used e.g. for the Vesta family, whose members have an unusual composition.
List
Prominent families
Among the many asteroid families, the following families are the most prominent ones in the asteroid belt. For the complete list, see below.- The Eos family
- The Eunomia family is a family of S-type asteroids. It is the most prominent family in the intermediate asteroid belt and the 6th-largest family with approximately 1.4% of all main belt asteroids.
- The Flora family is the 3rd-largest family. Broad in extent, it has no clear boundary and gradually fades into the surrounding background population. Several distinct groupings within the family, possibly created by later, secondary collisions. It has also been described as an asteroid clan.
- The Hungaria family
- The Hygiea family
- The [|Koronis family]
- The Nysa family. Alternatively named Hertha family after 135 Hertha.
- The Themis family
- The Vesta family
All families
| FIN | Family | Lbl | # of Members | Loc. | Taxonomy | mean- albedo | mean a | mean e | mean i | Parent bodyNotes | Cat | LoMP |
| 001 | Hilda family | HIL | 18 | rim | C | 0.04 | 3.965 | 0.174 | 8.92 | 153 Hilda; adj. Hildian; within the larger dynamical group with the same name. | cat | |
| 002 | Schubart family | SHU | 531 | rim | C | 0.03 | 3.966 | 0.191 | 2.92 | 1911 Schubart | cat | |
| 003 | Hungaria family | H | 1870 | close | E | 0.35 | 1.944 | 0.078 | 20.87 | 434 Hungaria; located within the dynamical group of the same name. | cat | |
| 004 | Hektor family | HEK | 16 | trojan | – | – | 5.204 | 0.054 | 19.02 | 624 Hektor | cat | |
| 005 | Eurybates family | ERY | 197 | trojan | CP | 0.06 | 5.204 | 0.044 | 7.42 | 3548 Eurybates | cat | |
| 006 | Thronium family | 006 | 15 | trojan | – | 0.06 | 5.204 | 0.049 | 31.75 | 9799 Thronium | — | |
| 007 | James Bond family | 007 | 1 | A | ASP | – | 2.474 | 0.129 | 6.32 | 9007 James Bond | — | |
| 008 | Arkesilaos family | ARK | 37 | trojan | – | – | 5.204 | 0.029 | 8.89 | 20961 Arkesilaos | cat | |
| 009 | Ennomos family | ENM | 30 | trojan | – | 0.06 | 5.204 | 0.041 | 26.79 | 4709 Ennomos | cat | |
| 010 | Shaulladany family | 010 | 13 | trojan | – | 0.09 | 5.204 | 0.041 | 24.23 | 247341 Shaulladany | — | |
| 401 | Vesta family | V | 10612 | A | V | 0.35 | 2.362 | 0.099 | 6.36 | 4 Vesta | cat | |
| 402 | Flora family | FLO | 13786 | A | S | 0.30 | 2.201 | 0.144 | 5.34 | 8 Flora, also named after 43 Ariadne; typical asteroid clan. Not a legitimate asteroid family according to Carruba and Milani, instead, the Florian core region is labelled Belgica family and Duponta family, respectively. | cat | |
| 403 | Baptistina family | BAP | 176 | A | X | 0.16 | 2.264 | 0.149 | 6.00 | 298 Baptistina, merges with the Belgica family at 100 m/s according to Carruba | cat | |
| 404 | Massalia family | MAS | 7820 | A | S | 0.22 | 2.409 | 0.162 | 1.42 | 20 Massalia, adj. Massalian, a-e-i: | cat | |
| 405 | Nysa–Polana complex | NYS | 15983 | A | SFC | 0.28 0.06 | 2.423 | 0.174 | 3.04 | 44 Nysa/142 Polana also known as the Hertha family. Includes the Eulalia family | cat | |
| 406 | Erigone family | ERI | 1776 | A | CX | 0.06 | 2.367 | 0.210 | 4.74 | 163 Erigone, adj. Erigonian. Can be joined with the dynamically different Martes family into a single collisional family. | cat | |
| 407 | Clarissa family | CLA | 236 | A | X | 0.05 | 2.406 | 0.107 | 3.35 | 302 Clarissa | cat | |
| 408 | Sulamitis family | SUL | 193 | A | C | 0.04 | 2.463 | 0.091 | 5.04 | 752 Sulamitis | cat | |
| 409 | Lucienne family | LCI | 142 | A | S | 0.22 | 2.462 | 0.111 | 14.51 | 1892 Lucienne | cat | |
| 410 | Euterpe family | EUT | 474 | A | S | 0.26 | 2.347 | 0.187 | 0.72 | 27 Euterpe | cat | |
| 411 | Datura family | DAT | 6 | A | S | 0.21 | 2.235 | 0.156 | 5.21 | 1270 Datura; Recently formed family with members:,,, and | cat | |
| 412 | Lucascavin family | LCA | 3 | A | S | – | 2.281 | 0.127 | 5.20 | 21509 Lucascavin; members:, | cat | |
| 413 | Klio family | KLI | 330 | A | C | 0.07 | 2.362 | 0.193 | 9.38 | 84 Klio | cat | |
| 414 | Chimaera family | CIM | 108 | A | CX | 0.06 | 2.460 | 0.155 | 14.65 | 623 Chimaera | cat | |
| 415 | Chaldaea family | CHL | 132 | A | C | 0.07 | 2.376 | 0.236 | 11.60 | 313 Chaldaea; alt. named after 1715 Salli by Masiero | cat | |
| 416 | Svea family | SVE | 48 | A | CX | 0.06 | 2.476 | 0.088 | 16.09 | 329 Svea | cat | |
| 417 | unnamed family | 417 | 9 | A | – | – | 2.465 | 0.153 | 3.93 | — | ||
| 701 | Phocaea family | PHO | 1248 | A | S | 0.22 | 2.400 | 0.228 | 23.41 | 25 Phocaea | cat | |
| 501 | Juno family | JUN | 1693 | B | S | 0.25 | 2.669 | 0.232 | 13.34 | 3 Juno | cat | |
| 502 | Eunomia family | EUN | 9856 | B | S | 0.19 | 2.644 | 0.148 | 13.08 | 15 Eunomia | cat | |
| 504 | Nemesis family | NEM | 1302 | C | C | 0.05 | 2.750 | 0.088 | 5.18 | 128 Nemesis '; also named after 58 Concordia ' and 3827 Zdeněkhorský. Formerly Liberatrix family by Zappalà and Cellino | cat | |
| 505 | Adeona family | ADE | 2070 | B | C | 0.07 | 2.673 | 0.169 | 11.71 | 145 Adeona | cat | |
| 506 | Maria family | MAR | 2958 | B | S | 0.25 | 2.554 | 0.101 | 15.02 | 170 Maria; alternatively named after 472 Roma. | cat | |
| 507 | Padua family | PAD | 1087 | C | X | 0.10 | 2.747 | 0.035 | 5.09 | 363 Padua; also known as Lydia family110 Lydiaadj. Paduan; Lydian | cat | |
| 508 | Aeolia family | AEO | 529 | C | X | 0.17 | 2.742 | 0.168 | 3.49 | 396 Aeolia | cat | |
| 509 | Chloris family | CLO | 120 | C | C | 0.06 | 2.727 | 0.255 | 9.23 | 410 Chloris, adj. Chloridian | cat | |
| 510 | Misa family | MIS | 647 | B | C | 0.03 | 2.658 | 0.178 | 2.26 | 569 Misa, adj. Misian | cat | |
| 511 | Brangäne family | BRG | 325 | B | S | 0.10 | 2.587 | 0.179 | 9.64 | 606 Brangäne | cat | |
| 512 | Dora family | DOR | 1742 | C | C | 0.05 | 2.797 | 0.198 | 7.83 | 668 Dora, adj. Dorian | cat | |
| 513 | Merxia family | MRX | 1263 | C | S | 0.23 | 2.745 | 0.133 | 4.85 | 808 Merxia, adj. Merxian | cat | |
| 514 | Agnia family | AGN | 3336 | C | S | 0.18 | 2.783 | 0.066 | 3.58 | 847 Agnia | cat | |
| 515 | Astrid family | AST | 548 | C | C | 0.08 | 2.788 | 0.048 | 0.66 | 1128 Astrid, adj. Astridian | cat | |
| 516 | Gefion family | GEF | 2428 | C | S | 0.20 | 2.784 | 0.129 | 9.01 | 1272 Gefion, adj. Gefionian; a-e-i: ; also known as Ceres family ' after 1 Ceres; and Minerva family after 93 Minerva | cat | |
| 517 | König family | KON | 578 | B | CX | 0.04 | 2.571 | 0.139 | 8.85 | 3815 König | cat | |
| 518 | Rafita family | RAF | 775 | B | S | 0.25 | 2.547 | 0.173 | 7.74 | 1644 Rafita, adj. Rafitian ; members and | cat | |
| 519 | Hoffmeister family | HOF | 2095 | C | CF | 0.04 | 2.787 | 0.047 | 4.36 | 1726 Hoffmeister | cat | |
| 520 | Iannini family | IAN | 150 | B | S | 0.32 | 2.644 | 0.267 | 12.19 | 4652 Iannini | cat | |
| 521 | Kazuya family | KAZ | 44 | B | S | 0.21 | 2.568 | 0.141 | 14.56 | 7353 Kazuya | cat | |
| 522 | Ino family | INO | 463 | C | S | 0.24 | 2.743 | 0.172 | 13.52 | 173 Ino | cat | |
| 523 | Emilkowalski family | EMI | 4 | B | S | 0.20 | 2.599 | 0.178 | 17.42 | 14627 Emilkowalski; members:, and | cat | |
| 524 | Brugmansia family | 524 | 3 | B | S | – | 2.620 | 0.179 | 2.80 | 16598 Brugmansia; members: and | cat | |
| 525 | Schulhof family | SHF | 5 | B | S | 0.27 | 2.610 | 0.163 | 13.30 | 2384 Schulhof; members:,,, | cat | |
| 526 | unnamed family | 526 | 81 | C | C | 0.06 | 2.721 | 0.173 | 14.35 | — | ||
| 527 | Lorre family | LOR | 2 | C | C | 0.05 | 2.747 | 0.263 | 28.18 | 5438 Lorre; other member: | cat | |
| 528 | Leonidas family | [|LEO] | 111 | B | CX | 0.07 | 2.681 | 0.193 | 3.81 | 2782 Leonidas; identical to the Vibilia family: ; | cat | |
| 529 | Vibilia family | VIB | 180 | B | C | 0.06 | 2.655 | 0.191 | 3.82 | 144 Vibilia; namesake only listed in family by Zappalà, but not by Nesvorý; identical to the Leonidas family: LEO. | cat | |
| 530 | Phaeo family | PAE | 146 | C | X | 0.06 | 2.782 | 0.199 | 9.47 | 322 Phaeo | cat | |
| 531 | Mitidika family | MIT | 653 | B | C | 0.06 | 2.587 | 0.247 | 12.50 | 2262 Mitidika ; members: and | cat | |
| 532 | Henan family | HEN | 1872 | B | L | 0.20 | 2.699 | 0.063 | 2.80 | 2085 Henan | cat | |
| 533 | Hanna family | HNA | 280 | C | CX | 0.05 | 2.807 | 0.180 | 4.17 | 1668 Hanna | cat | |
| 534 | Karma family | KRM | 59 | B | CX | 0.05 | 2.577 | 0.106 | 10.75 | 3811 Karma | cat | |
| 535 | Witt family | WIT | 1618 | C | S | 0.26 | 2.760 | 0.030 | 5.79 | 2732 Witt, alternatively named after 10955 Harig | cat | |
| 536 | Xizang family | XIZ | 275 | C | – | 0.12 | 2.754 | 0.154 | 2.76 | 2344 Xizang | cat | |
| 537 | Watsonia family | WAT | 83 | C | L | 0.13 | 2.760 | 0.122 | 17.33 | 729 Watsonia | cat | |
| 538 | Jones family | JNS | 22 | B | T | 0.05 | 2.626 | 0.110 | 12.35 | 3152 Jones | cat | |
| 539 | Aëria family | AER | 272 | B | X | 0.17 | 2.649 | 0.056 | 11.76 | 369 Aeria | cat | |
| 540 | Julia family | JUL | 33 | B | S | 0.19 | 2.552 | 0.124 | 16.70 | 89 Julia | cat | |
| 541 | Postrema family | POS | 108 | C | CX | 0.05 | 2.738 | 0.242 | 16.53 | 1484 Postrema | cat | |
| 801 | Pallas family | PAL | 45 | C | B | 0.16 | 2.771 | 0.281 | 33.20 | 2 Pallas | cat | |
| 802 | Gallia family | GAL | 137 | C | S | 0.17 | 2.771 | 0.132 | 25.16 | 148 Gallia | cat | |
| 803 | Hansa family | HNS | 1162 | B | S | 0.26 | 2.644 | 0.004 | 22.06 | 480 Hansa adj. Hansian; a-e-i: | cat | |
| 804 | Gersuind family | GER | 415 | B | S | 0.15 | 2.589 | 0.175 | 17.34 | 686 Gersuind | cat | |
| 805 | Barcelona family | BAR | 346 | B | S | 0.25 | 2.637 | 0.251 | 30.83 | 945 Barcelona | cat | |
| 806 | Tina family | TIN | 107 | C | X | 0.34 | 2.793 | 0.082 | 20.76 | 1222 Tina | cat | |
| 807 | Brucato family | BRU | 41 | B | CX | 0.06 | 2.605 | 0.132 | 28.90 | 4203 Brucato | cat | |
| 601 | Hygiea family | HYG | 3145 | G | CB | 0.06 | 3.142 | 0.136 | 5.07 | 10 Hygiea | cat | |
| 602 | Themis family | THM | 5612 | G | C | 0.07 | 3.134 | 0.152 | 1.08 | 24 Themis | cat | |
| 603 | Sylvia family | SYL | 191 | rim | X | 0.05 | 3.485 | 0.054 | 9.76 | 87 Sylvia; family within Cybele group | cat | |
| 604 | Meliboea family | MEL | 444 | G | C | 0.05 | 3.119 | 0.186 | 14.54 | 137 Meliboea, adj. Meliboean | cat | |
| 605 | Koronis family | KOR | 7390 | D | S | 0.15 | 2.869 | 0.045 | 2.15 | 158 Koronis, also named after 208 Lacrimosa | cat | |
| 606 | Eos family | EOS | 16038 | E | K | 0.13 | 3.012 | 0.077 | 9.94 | 221 Eos | cat | |
| 607 | Emma family | EMA | 577 | F | C | 0.05 | 3.046 | 0.113 | 9.09 | 283 Emma | cat | |
| 608 | Brasilia family | BRA | 845 | D | X | 0.18 | 2.862 | 0.127 | 14.98 | 293 Brasilia, adj. Brazilian | cat | |
| 609 | Veritas family | VER | 2139 | G | CPD | 0.07 | 3.174 | 0.066 | 9.06 | 490 Veritas, adj. Veritasian; alt: Undina family after 92 Undina | cat | |
| 610 | Karin family | KAR | 541 | D | S | 0.21 | 2.864 | 0.044 | 2.10 | 832 Karin. Recently formed family located within the Koronis family. | cat | |
| 611 | Naëma family | NAE | 375 | D | C | 0.08 | 2.940 | 0.036 | 11.99 | 845 Naëma, adj. Naëmian | cat | |
| 612 | Tirela family | TIR | 1815 | G | S | 0.07 | 3.116 | 0.195 | 17.06 | 1400 Tirela, alternatively named after 1040 Klumpkea | cat | |
| 613 | Lixiaohua family | LIX | 1241 | G | CX | 0.04 | 3.153 | 0.201 | 10.06 | 3556 Lixiaohua; although member 3330 Gantrisch is both larger and lower numbered ] | cat | |
| 614 | Telramund family | TEL | 513 | E | S | 0.22 | 2.993 | 0.066 | 8.81 | 9506 Telramund; alternatively named after 179 Klytaemnestra by Masiero and by Milani | cat | |
| 615 | unnamed family | 615 | 159 | D | CX | 0.17 | 2.848 | 0.106 | 9.14 | — | ||
| 616 | Charis family | CHA | 808 | D | C | 0.08 | 2.900 | 0.047 | 5.73 | 627 Charis | cat | |
| 617 | Theobalda family | THB | 574 | G | CX | 0.06 | 3.178 | 0.263 | 14.05 | 778 Theobalda, adj. Theobaldian; a-e-i: | cat | |
| 618 | Terentia family | TRE | 80 | D | C | 0.07 | 2.932 | 0.072 | 11.11 | 1189 Terentia | cat | |
| 619 | Lau family | LAU | 56 | D | S | 0.27 | 2.929 | 0.195 | 6.30 | 10811 Lau | cat | |
| 620 | Beagle family | BGL | 148 | G | C | 0.09 | 3.155 | 0.154 | 1.34 | 656 Beagle. Recently formed family is located within the Themis family. Includes 7968 Elst–Pizarro. | cat | |
| 621 | Koronis family | K-2 | 246 | D | S | 0.14 | 2.869 | 0.045 | 2.15 | 158 Koronis "second family" | cat | |
| 622 | Terpsichore family | TRP | 138 | D | C | 0.05 | 2.854 | 0.182 | 8.23 | 81 Terpsichore | cat | |
| 623 | Fringilla family | FIR | 134 | D | X | 0.05 | 2.914 | 0.093 | 16.68 | 709 Fringilla | cat | |
| 624 | Durisen family | DUR | 27 | D | X | 0.04 | 2.943 | 0.185 | 16.19 | 5567 Durisen | cat | |
| 625 | Yakovlev family | YAK | 67 | D | C | 0.05 | 2.870 | 0.290 | 7.89 | 5614 Yakovlev | cat | |
| 626 | San Marcello family | SAN | 144 | D | X | 0.19 | 2.922 | 0.078 | 12.50 | 7481 San Marcello | cat | |
| 627 | unnamed family | 627 | 38 | D | CX | 0.05 | 2.868 | 0.219 | 16.02 | — | ||
| 628 | unnamed family | 628 | 248 | D | S | 0.10 | 2.850 | 0.081 | 5.12 | — | ||
| 629 | unnamed family | 629 | 58 | D | A | 0.21 | 2.939 | 0.118 | 10.73 | — | ||
| 630 | Aegle family | AEG | 120 | F | CX | 0.07 | 3.052 | 0.190 | 16.48 | 96 Aegle | cat | |
| 631 | Ursula family | URS | 731 | G | CX | 0.06 | 3.128 | 0.098 | 16.21 | 375 Ursula | cat | |
| 632 | Elfriede family | ELF | 97 | G | C | 0.05 | 3.189 | 0.061 | 15.87 | 618 Elfriede | cat | |
| 633 | Itha family | ITH | 54 | D | S | 0.23 | 2.866 | 0.158 | 12.27 | 918 Itha | cat | |
| 634 | Inarradas family | INA | 43 | F | CX | 0.07 | 3.050 | 0.184 | 14.51 | 3438 Inarradas | cat | |
| 635 | Anfimov family | ANF | 49 | F | S | 0.16 | 3.044 | 0.089 | 3.48 | 7468 Anfimov | cat | |
| 636 | Marconia family | MRC | 34 | F | CX | 0.05 | 3.063 | 0.097 | 2.58 | 1332 Marconia | cat | |
| 637 | unnamed family | 637 | 64 | G | CX | 0.05 | 3.109 | 0.180 | 3.46 | — | ||
| 638 | Croatia family | CRO | 93 | G | X | 0.07 | 3.133 | 0.026 | 10.66 | 589 Croatia | cat | |
| 639 | Imhilde family | IMH | 43 | E | CX | 0.05 | 2.983 | 0.237 | 14.59 | 926 Imhilde | cat | |
| 640 | Gibbs family | GBS | 8 | E | – | – | 3.004 | 0.023 | 10.34 | 331P/Gibbs "P/2012 F5 ". Other members include,, and | — | — |
| 641 | Juliana family | JLI | 76 | E | CX | 0.05 | 3.004 | 0.144 | 13.12 | 816 Juliana | cat | |
| 901 | Euphrosyne family | EUP | 1385 | G | C | 0.06 | 3.155 | 0.208 | 26.54 | 31 Euphrosyne | cat | |
| 902 | Alauda family | ALA | 1294 | G | B | 0.07 | 3.194 | 0.021 | 21.66 | 702 Alauda | cat | |
| 903 | Ulla family | ULA | 37 | rim | X | 0.05 | 3.543 | 0.050 | 17.96 | 909 Ulla; family within Cybele group | cat | |
| 904 | Luthera family | LUT | 232 | G | X | 0.04 | 3.219 | 0.121 | 18.77 | 1303 Luthera; fam. is also named after 781 Kartvelia | cat | |
| 905 | Armenia family | ARM | 67 | G | C | 0.05 | 3.117 | 0.070 | 18.19 | 780 Armenia | cat |