NEOMOD: An advanced orbital distribution model for NEOs

[ METEOMOD | NEOMOD | Documentation ]

Compute a probability of coming from a source. A version for kilometre-sized bodies. See examples.

Note: In this example, the orbits of Bennu and Ryugu are used. A user should select the corresponding CI-chondrite-like sources. A conclusion is that both come from Polana.

Orbits: 1. a [au] 2. e [1] 3. i [deg] 4. designation

Sources:

Vesta (HED)
all H
Phocaea (H)
Maria (H)
Merxia (H)
Agnia (H)
Koronis (H)
Koronis(2) (H)
Karin (H)
all L
Massalia (L)
Massalia(2) (L)
Gefion (L)
Juno (L/LL)
all LL
Flora (LL)
Eunomia (LL)
Nysa (LL)
all CM
Vibilia (CM)
Adeona (CM)
Erigone (CM)
Chloris (CM)
Veritas (CM)
Dora (CM)
Theobalda (CM)
Astrid (CM)
König (CM)
all CI
Hygiea (CI)
Themis (CI)
Euphrosyne (CI)
Nemesis (CI)
Polana (CI)
Clarissa (CI)
Ursula (CI)
Misa (CI)
Elfriede (CI)
Beagle (CI)
Alauda (CI)
Naema (CI)
Hoffmeister (CI)
Lixiaohua (CI)
Emma (IDP)
Padua (IDP)
Pallas (B)
all CO/CV/CK
Eos (CO/CV/CK)
Watsonia (CO/CV/CK)
all CR
Baptistina (?)
Aeolia (?)
all M
Kalliope (M)
Brasilia (CH)
Aeria (M)
Brangäne (M)
Tina (M)
all E
Nysa (E)
Hungaria (E)
other
Sylvia (P)
Phaethon (CY?)

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Miroslav Broz (miroslav.broz@email.cz), Oct 10th 2024