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Planetary geology

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impact crater
circular depression in a solid astronomical body formed by the impact of a smaller object
bolide
A bolide is normally taken to mean an exceptionally bright meteor, but the term is subject to more than one definition, according to context. It may refer to any large crater-forming body, or to one that explodes in the atmosphere. It can be a synonym for a fireball, sometimes specific to those with an apparent magnitude of −4 or brighter.
Earth mass
unit of mass equal to that of Earth
chondrite
A chondrite (, ) is a stony (non-metallic) meteorite that has not been modified by either melting or differentiation of the parent body. They are formed when various types of dust and small grains in the early Solar System accreted to form primitive asteroids. Some such bodies that are captured in the planet's gravity well become the most common type of meteorite by arriving on a trajectory toward the planet's surface. Estimates for their contribution to the total meteorite population vary between 85.7% and 86.2%.
cryovolcano
alt=An image of two large cryovolcanoes|thumb|upright=1.5|Leviathan Patera (center) and [[Ruach Planitia (upper left), two large cryovolcanic features on Neptune's moon Triton]]
planetary core
innermost layer(s) of a planet
Earth radius
mean distance from the Earth's center to its surface
planetary geology
geology of astronomical objects
planetary mantle
layer inside a planetary body
planetary nomenclature
system of uniquely identifying features on the surface of a planet or natural satellite
volatiles
chemical elements or compounds with low boiling points associated with planet’s or moon’s crust or atmosphere
arachnoid
large structure of unknown origin on Venus
rupes
[[File:Rupes Recta (LROC287 - recta thumb2).png|thumb|Rupes Recta is a well-known linear rille that extends over 100 km in length. Portion of LROC WAC monochrome mosaic, illumination is from the left, and asterisk notes location of LROC NAC (below) [NASA/GSFC/Arizona State University].]] In planetary geology, rupes (, plural: ) are escarpments on planets other than Earth.
albedo feature
area which shows a contrast in albedo with adjacent areas
crater chain
chain of craters
palimpsest
type of crater whose relief has disappeared
chasma
In planetary nomenclature, a chasma (plural: chasmata ) is a deep, elongated, steep-sided depression. As of 2020, the IAU has named 122 such features in the Solar System, on Venus (63), Mars (25), Saturn's satellites Mimas (6), Tethys (2), Dione (8) and Rhea (5), Uranus's satellites Ariel (7), Titania (2) and Oberon (1) and Pluto's satellite Charon (3). An example is Eos Chasma on Mars.
rille
left|thumb|Rima Hyginus, an eminent rille, in selenochromatic format thumb|Rimae on the floor of the lunar crater Gassendi (crater)|Gassendi, from [[Apollo 16.]] thumb|Mamers Valles rille on Mars. thumb|Rima Ariadaeus is categorized as a straight rille (graben) and is over 300 km in length. thumb|Hadley Rille at center is a sinuous rille visited by the Apollo 15 mission. thumb|Detail of part of Hadley Rille
corona
oval feature on Venus or Miranda
chaos terrain
distinctive area of broken or jumbled terrain
geology of Pluto
Scientific study of the surface, crust, and interior of the dwarf planet Pluto
macula
unusually dark area on the surface of a planet or moon
patera
irregular crater
vallis
valley in Mars, Moon, etc
linea
thumb|right|Low resolution view of lineae on Europa taken by NASAs Galileo (spacecraft)|Galileo spacecraft.
Irnini Mons
mons on Venus
secondary crater
impact crater formed by the ejecta that was thrown out of a larger crater
inverted relief
landscape features that have reversed their elevation relative to other features
Preliminary Reference Earth Model
model representing the average Earth properties as a function of planetary radius
colles
small hill or knob on a celestial body
scopulus
thumb|right|360 px|False color oblique view of Nilokeras Scopulus on Mars. Mars Orbital Laser Altimeter (MOLA) colorized elevation overlying [[Thermal Emission Imaging System (THEMIS) Infrared (IR) daytime mosaic from Mars Odyssey spacecraft. Yellow and light green represent high elevations; dark green and blue are lower elevations. Image is approximately 175 km across. Vertical exaggeration is 3X.]] In planetary geology, a scopulus (pl. scopuli , from Greek σκόπελος "peak") is a lobate or irregular escarpment. In the early 1970s, the International Astronomical Union (IAU) adopted scopulus as
magma ocean
large area of molten rock on the surface of a planet
planetary surface
where the solid (or liquid) material of the outer crust on certain types of astronomical objects contacts the atmosphere or outer space
mensa
flat-topped prominence with cliff-like edges
Geology of Ceres
geologic structure and composition of Ceres
pedestal crater
type of impact crater
mons
mountain on a celestial body
scalloped margin dome
volcanic dome on Venus that has experienced collapse and mass wasting such as landslides on its perimeter
G. K. Gilbert Award
award given by the Planetary Geology Division of the Geological Society of America for outstanding contributions to the solution of fundamental problems in planetary geology (1983–)
Lithosphere-Asthenosphere boundary
level representing a mechanical difference between layers in Earth’s inner structure
Astrogeology Research Program