Results 111 to 120 of about 10,677 (209)
Being one of the most populated mean motion resonances (MMRs) with Neptune and lying close to the inner boundary of the present-day cold classical disk, observations of the orbital and surface class distributions of the plutinos in the 3:2 MMR provide ...
Cameron Collyer +8 more
doaj +1 more source
Imaging of the Vega Debris System Using JWST/MIRI
We present images of the Vega planetary debris disk obtained at 15.5, 23, and 25.5 μ m with the Mid-Infrared Instrument on JWST. The debris system is remarkably symmetric, smooth, and centered accurately on the star.
Kate Y. L. Su +8 more
doaj +1 more source
GANBISS: a new GPU accelerated N-body code for binary star systems. [PDF]
Zimmermann M, Pilat-Lohinger E.
europepmc +1 more source
Simulations of Multiple Dust Ring Formation in a Subsolar-metallicity Protoplanetary Disk
Super-Earths exist around subsolar-metallicity host stars with a frequency comparable to that around solar-metallicity stars, suggesting efficient assembly of dust grains even in metal-deficient environments.
Ryoki Matsukoba +2 more
doaj +1 more source
Organic Matter in the Asteroid Ryugu: What We Know So Far. [PDF]
Potiszil C +8 more
europepmc +1 more source
Ureilite meteorites provide a new model of early planetesimal formation and destruction [PDF]
Nachiketa Rai, Hilary Downes, CL Smith
openalex +1 more source
Possible Ribose Synthesis in Carbonaceous Planetesimals. [PDF]
Paschek K +7 more
europepmc +1 more source
Thermal evolution and sintering of chondritic planetesimals IV. Temperature dependence of heat conductivity of asteroids and meteorites [PDF]
H. P. Gail, M. Trieloff
openalex +1 more source
87th Annual Meeting of the Meteoritical Society 2025: Contents
Meteoritics &Planetary Science, Volume 60, Issue S1, Page 2-29, August 2025.
wiley +1 more source
Distinguishing the Origin of Asteroid (16) Psyche. [PDF]
Elkins-Tanton LT +21 more
europepmc +1 more source

