impact
(collision of one solid body with another)
In astronomy, the term impact is used for a collision between two
solid bodies.
In such an impact, both may be of significant size,
or one might be much smaller than the other.
Craters are evidence of impacts.
Impacts are assumed in theories of planet formation, both to
explain how planets grew, assuming one of the bodies gained the
material from the other, and how bodies came to have their constituents,
assuming impacts removed the outer surface removed by one or more
impacts (impact erosion), which can leave the body denser if the
densest material had already fallen toward the center of the body.
It is assumed both scenarios occur, depending upon the velocity
of the impact(s).
The favored theory of the Moon's formation is that it results from
a giant impact, the impact of a Mars-sized planet with
Earth (known as the giant-impact hypothesis).
(planets)
Further reading:
https://en.wikipedia.org/wiki/Impact_event
https://en.wikipedia.org/wiki/Giant-impact_hypothesis
https://en.wikipedia.org/wiki/Formation_and_evolution_of_the_Solar_System
https://mobile.arc.nasa.gov/public/iexplore/missions/pages/yss/june.html
Referenced by pages:
101955 Bennu
ATLAS survey
atmosphere formation
atmospheric escape
Chicxulub crater
chondrite
CIG
circumplanetary disk
collisional erosion
Comet Shoemaker-Levy 9
complex crater
debris disk
Europa
extra-solar planet
faint young Sun paradox
globular cluster (GC)
GW detection (GW)
GW170817
iSALE
isolation mass
late heavy bombardment (LHB)
lava planet
LCROSS
magma ocean
mass extinction
maximum iron fraction
metallicity (Z)
meteorite
meteoroid
minimum orbit intersection distance (MOID)
moon
Moon formation
near-Earth object (NEO)
oligarch
pebble accretion
planet formation
planetary protection
quake
Rosetta
siderophile
smoothed-particle hydrodynamics (SPH)
stellar dynamics
stellar encounter
strewn field
Tillotson equation
weathering
Index