Hourglass region

E514345

The Hourglass region is a bright, compact star-forming nebular core within the Lagoon Nebula (Messier 8), notable for its intense radiation, young massive stars, and striking hourglass-shaped appearance.

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Statements (48)

Predicate Object
instanceOf astronomical object
nebular core
star-forming region
contains dust lanes
embedded star cluster
ionized gas
young massive stars
distanceApprox about 4,000–5,000 light-years from Earth
emits infrared radiation
optical emission lines
strong H-alpha emission
hasAlternateDescription bright core of the Lagoon Nebula
hasAppearance bright
compact
hasColor predominantly red in optical images
shows blue and green components from different emission lines
hasEnvironment dense molecular gas
intense ultraviolet radiation
strong stellar winds
hasProperty high surface brightness
intense radiation field
hasRoleIn triggered star formation in surrounding gas
hasShape hourglass-shaped
hasSignificance example of compact H II region
laboratory for massive star formation studies
hasStructure bright ionization fronts
dark obscuring clouds
nebular filaments
hostGalaxy Milky Way NERFINISHED
illuminatedBy massive O-type stars
young stellar objects
isImagedBy Hubble Space Telescope NERFINISHED
ground-based observatories
isNearbyTo central regions of Lagoon Nebula
isRegionOf active star formation
isStudiedIn nebular dynamics research
star formation research
isSubstructureOf H II region in Lagoon Nebula
locatedIn Sagittarius constellation NERFINISHED
namedAfter its hourglass-like morphology
observedIn infrared wavelengths
optical wavelengths
radio wavelengths
partOf Lagoon Nebula NERFINISHED
Messier 8 NERFINISHED
physicalProcess ongoing gravitational collapse of dense clumps
photoionization by massive stars
stellar wind–driven shaping of gas

Referenced by (1)

Full triples — surface form annotated when it differs from this entity's canonical label.

Messier 8 hasRegion Hourglass region