Results 121 to 130 of about 4,544 (213)
The Formation of Planetesimals: Building Bricks for Planetary Systems [PDF]
, 2016 The asteroids and Kuiper Belt objects are left overs of building material for our earth and the other planets in our solar systems from 4.567 billion years ago.
Klahr, H., Schreiber, A.
core
The formation and structure of iron-dominated planetesimals
Context. Metal-rich asteroids and iron meteorites are considered core remnants of differentiated planetesimals and/or products of oxygen-depleted accretion. Aims. Investigating the origins of iron-rich planetesimals could provide key insights into planet
Simone Marchi +4 more
core +1 more source
Phosphorus-nitrogen systematics of first-generation planetesimals constrain life-essential element delivery to Earth. [PDF]
Sci AdvPathak D, Dasgupta R, Iyer N.
europepmc +1 more source
Light hydrogen isotopes in terrestrial core. [PDF]
Sci AdvZhang Y, Wang W, Deng Z, Wu Z, Chen B.
europepmc +1 more source
Potential sublimating exocomets around the young star PDS 70. [PDF]
Nat CommunNovais A +6 more
europepmc +1 more source
Asteroid sample return missions are critical for understanding our Solar System. [PDF]
Nat CommunBates H.
europepmc +1 more source
Refractory inclusions in Bennu samples indicative of outer Solar System accretion. [PDF]
Nat CommunKawasaki N +12 more
europepmc +1 more source
Chalcogen isotopes reveal limited volatile contribution from late veneer to Earth. [PDF]
Sci Adv, 2023 Wang W +4 more
europepmc +1 more source
The late formation of chondrites as a consequence of Jupiter-induced gaps and rings. [PDF]
Sci AdvSrivastava B, Izidoro A.
europepmc +1 more source