Mn-Cr isotopic systematics of chondrules from the Bishunpur and Chainpur meteorites

Bibcode
1997LPI....28.1033N
Nyquist, L.; Lindstrom, D.; Shih, C.-Y.; Wiesmann, H.; Mittlefehldt, D.; Wentworth, S.; Martinez, R.
Referencia bibliográfica

Conference Paper, 28th Annual Lunar and Planetary Science Conference, p. 033.

Fecha de publicación:
3
1997
Número de autores
7
Número de autores del IAC
0
Número de citas
8
Número de citas referidas
6
Descripción
Mn-Cr data are reported for chondrules from the Bishunpur and Chainpur LL chondrites. It is shown that variations in Mn/Cr for these chondrules were established during condensation of solids from the solar nebula; the whole-chondrule isochrons should give an upper limit to the time of chondrule formation and an estimate of when the chondrule precursors were condensing from the gaseous solar nebula.
Tipo
Sin árbitro
Meteoritos

Te puede interesar

  • Sin árbitro
    joshspeagle/dynesty: v3.0.0
    This is major release with several infrastructural changes that will make future development of dynesty easier, as well as significant speedups. The release also deprecated some rarely used options. Major refactor of the code that makes it easier to add new samplers. Major speedup of the uniform sampler when sampling in parallel You can now provide
    Koposov, Sergey et al.

    Fecha de publicación:

    10
    2025
    Bibcode
    2025zndo..17268284K
    Número de citas
    1
  • Sin árbitro
    (163) Erigone, (302) Clarissa, and (752) Sulamitis as seen with JWST's NIRSpec
    Primitive asteroids in the Main Belt possess one of the most pristine inventories of materials in the Solar System. Main Belt primitive asteroids are particularly interesting due to clear evidence of phyllosilicates, i.e., silicates that have encountered liquid water and undergone chemical alteration. Since asteroids are thought to be likely
    Harvison, Brittany et al.

    Fecha de publicación:

    9
    2025
    Bibcode
    2025epsc.conf.1004H
    Número de citas
    0
  • Sin árbitro
    NEOMIR: project statut of ESA's space-based infrared mission for NEO detection and early warning
    To warn about potential asteroid or comet impacts, we must first observe and discover these objects through dedicated NEO surveys. Most current and planned surveys are ground-based and use visible light, but they face limitations like weather dependency, limited sky visibility, difficulty detecting at low galactic latitudes, and inability to
    Conversi, Luca et al.

    Fecha de publicación:

    9
    2025
    Bibcode
    2025epsc.conf.1329C
    Número de citas
    0