Supermaxman/esa-hubble huggingface dataset:
Proplyds in the Orion Nebula: Glowing protoplanetary disks (first discovered with the Hubble in 1992, and dubbed "proplyds") that are believed to be embryonic solar systems that will eventually form planets. (Our solar system has long been considered the relic of just such a disk that formed around the newborn Sun). The abundance of such objects in the Orion nebula strengthens the argument that planet formation is a common occurrence in the universe. Some of the proplyds, those that are closest to the Trapezium stars at the centre of the Orion Nebula, are shedding some of their gas and dust. The pressure of starlight from the hottest stars forms "tails" which act like wind vanes pointing away from the Trapezium. These tails result from the light from the star pushing the dust and gas away from the outside layers of the proplyds. In addition to the luminescent proplyds, seven disks are silhouetted against the bright background of the nebula. These dark objects allow Hubble astronomers to estimate the masses of the disks as at least 0.1 to 730 times the mass of our Earth.

Name: Messier 42, Orion Nebula, Orion Proplyd
Type: Milky Way : Nebula : Type : Star FormationMilky Way : Nebula : Appearance : Dark : Proplyd
Category: Nebulae
Distance: 1400 light years
Release date: 20 November 1995, 06:00
Credit: NASA, C.R. O'Dell and S.K. Wong (Rice University)

Starbirth: This mosaic shows the center of the Orion Nebula. Many of the nebula's details can't be captured in a single picture - any more than one snapshot of the Grand Canyon yields clues to its formation and history.  Like the Grand Canyon, the Orion nebula has a dramatic surface topography — of glowing gasses instead of rock — with  peaks, valleys and walls.  They are illuminated and heated by a torrent of energetic ultraviolet light from its four hottest and most massive stars, called the Trapezium, which lie near the center of the image.

Name: Messier 42, NGC 1976, Orion Nebula
Type: Milky Way : Star : Circumstellar Material : Disk : ProtoplanetaryMilky Way : Nebula : Type : Star Formation
Category: Nebulae
Constellation: Orion
Distance: 1400 light years
Release date: 20 November 1995, 06:00
Credit: NASA, C.R. O'Dell and S.K. Wong (Rice University)

Trapezium, Orion Nebula: Like the Grand Canyon, the Orion nebula has a dramatic surface topography — of glowing gasses instead of rock — with  peaks, valleys and walls.  They are illuminated and heated by a torrent of energetic ultraviolet light from its four hottest and most massive stars, called the Trapezium, which are pictured here. In addition to the Trapezium, this stellar cavern contains 700 hundred other young stars at various stages of formation.  High-speed jets of hot gas spewed by some of the infant stars send supersonic shock waves tearing into the nebula at  100,000 miles per hour.

Name: Messier 42, NGC 1976, Trapezium Cluster
Type: Milky Way : Star : Grouping : Cluster : OpenMilky Way : Nebula : Type : Star Formation
Category: Star Clusters
Constellation: Orion
Distance: 1400 light years
Release date: 20 November 1995, 06:00
Credit: NASA, C.R. O'Dell and S.K. Wong (Rice University)