Formation vs. shock vs. CRE ages of meteorites

a shock-age model for Flora?
Ang shock ages?
Bra shock ages?
Pal shock ages? (not found)
CC irons (IID, IVB) shock ages?
CC irons CRE ages?
H, L, LL formation ages?
HED formation ages?
iron IAB^non-magmatic .. Kalliope?
iron IIIAB^magmatic .. Hertha?


Sequence of condensation lines:

|H2O |NH3 |CO2 |CH4 |N2  |CO
|    |    |    |    |    |     
165  85   75   35   25   22


Sequence from anomalies:

Ure HED+Pal+Mes Aca Ang LL L H Mars EC IAB! Earth+Moon R | CO+CK+CV CM CB CR CI  CAI
                                         <- neutron-poor | neutron-rich, s-process, SN, pre-solar grains ->

from oxygen:

CAI  CO+CK+CV CR CH Ure! CM | Aca-Lod HED+Mes+Pal Ang Bra IAB Win Earth+Moon Mars EC IIE H L LL IVA R CI! CM_meta CI_meta
               <- shielding | evaporation ->

from fugacity:

CAI Aub Ure EC IIE IIIAB IAB CB CH Aca H L LL Pal | R CR Bra Ang HED CO CV CK CM CI
                                       <- reduced | oxidized ->

from ages:

IC..IVA Ang Ure Mes Aca-Lod IAB! Win | Aub EH EL H L LL R IIC..IVB CO CV CH CR CM CI CB
                            <- early | late ->
--

Known formation regions:

HED+Pal+Mes .. ???, neutron-poorest, evaporation a bit, oxidized (core-formation?), earliest
Ure         .. ???, neutron-poorest, shielding as CCs!, highly reduced!, earliest!

Earth+Moon  .. oxidized (core-formation)
IAB         .. ???, neutron-poor as Earth!, evaporation, reduced, early-to-late
Win         .. ???, neutron-poor, evaporation, reduced, early-to-late

EC          .. NEO, Mars-crossers, or E-belt?, neutron-poor, evaporation, highly reduced, late

Mars        .. migration ^^^ (Dauphas et al. 2024)

H           .. main belt, neutron-poor, evaporation, reduced, late
L           .. main belt, neutron-poor, evaporation, reduced, late
LL          .. main belt, neutron-poor, evaporation, reduced, late

IIIAB       .. ???, neutron-poor, evaporation, reduced, early 
R           .. below snowline?, neutron-poor a bit, evaporation, oxidized a bit, late

-- H2O

CO+CK+CV    .. Jupiter?, neutron-rich, most shielding, oxidized, late
CR          .. ???, neutron-rich, shielding, oxidized, latest
CH          .. ???, neutron-rich, shielding, reduced (metal), latest
CB          .. ???, neutron-rich, shielding, reduced (metal), latest
CM          .. trans-Saturn, neutron-rich, least shielding, oxidized, latest

-- NH3
-- CH4

CI          .. trans-Neptune, neutron-richest, evaporation a lot!, oxidized, latest


Ang         .. ???, neutron-poor, evaporation, oxidized (core-formation?), earliest
Bra         .. ???, neutron-poor, evaporation, oxidized (core-formation?), early
Aca-Lod     .. ???, neutron-poor, evaporation a bit, reduced, early


Note: See Clayton (1983) on irons.
Note: See Baker et al. (2005) on angrites.
Note: See Greenwood et al. (2007) on primitive achondrites.

For reference, anomalies: Warren (2011), Fig. 2 Burkhardt et al. (2019), Fig. 10 See also https://www.lpi.usra.edu/meteor/drawplot.cfm

For reference, oxygen (CAIs .. more along "CCAM"):

For reference, D/H (Jupiter .. protosolar):

Anomalies of Ti, Ca, Cr, Sr, Zr, Ba, Nd (litophile):

Ti vs. Ca	Ti vs. Cr	Ti vs. Sr	Ti vs. Zr	Ti vs. Ba	Ti vs. Nd

Anomalies of Mo, Ni, Ru, W (siderophile, i.e., for irons):

Mo	Mo vs. Ni	Mo vs. Ru	Mo vs. W

Note IAB irons <=> Earth, other irons <=> Ure, Ang, Aca?!