accretion$566$ - meaning and definition. What is accretion$566$
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What (who) is accretion$566$ - definition

ASTROPHYSICAL PROCESS IN WHICH MATTER GRAVITATIONALLY COLLECTS INTO A MASSIVE OBJECT
Accretion (astronomy); Accretion of planets; Runaway accretion; Planetary accretion
  • fall onto the compact star]], forming an accretion disk
  • Artist's impression of a [[protoplanetary disk]] showing a young star at its center
  • [[Chondrule]]s in a [[chondrite]] meteorite. A millimeter scale is shown.
  • Infrared image of the molecular outflow from an otherwise hidden newborn star HH 46/47
  • lk=on}} away in the constellation Sagittarius
  • ALMA]] image of [[HL Tauri]], a [[protoplanetary disk]]

Accretion (meteorology)         
ACCUMULATION OF FROZEN WATER AS PRECIPITATION OVER TIME AS IT DESCENDS THROUGH THE ATMOSPHERE
Accretion (atmospheric science); Accretion (atmosphere)
Accretion is defined as the gradual collection of something over time.Accretion (definition) Merriam-Webster.
Accretion (astrophysics)         
In astrophysics, accretion is the accumulation of particles into a massive object by gravitationally attracting more matter, typically gaseous matter, in an accretion disk. Most astronomical objects, such as galaxies, stars, and planets, are formed by accretion processes.
Accretion disk         
  • Artist's conception of a black hole drawing matter from a nearby star, forming an accretion disk
  • [[HH-30]], a [[Herbig–Haro object]] surrounded by an accretion disk
  • Artist's view of a star with accretion disk
STRUCTURE FORMED BY DIFFUSE MATERIAL IN ORBITAL MOTION AROUND A MASSIVE CENTRAL BODY
Accretion Disc; Accretion disks; Accretion theory; Accretion Disk; Diskoseismology; Disko-seismology; Disko seismology; Advection-dominated accretion flow; Advection Dominated Accretion Flow; Excretion disk; Excretion disc; Accretion disc
An accretion disk is a structure (often a circumstellar disk) formed by diffuse material in orbital motion around a massive central body. The central body is typically a star.

Wikipedia

Accretion (astrophysics)

In astrophysics, accretion is the accumulation of particles into a massive object by gravitationally attracting more matter, typically gaseous matter, in an accretion disk. Most astronomical objects, such as galaxies, stars, and planets, are formed by accretion processes.