NGC 6302 Nebula

GPTKB entity

Statements (97)
Predicate Object
gptkbp:instance_of gptkb:Nebula_Award
gptkbp:age approximately 1,000 years
gptkbp:body_shape butterfly shape
gptkbp:composed_by gptkb:hydrogen
nitrogen
carbon
helium
gptkbp:contains central star
ionized gas
dust lanes
gptkbp:contains_star gptkb:HD_148937
gptkbp:declination -37° 05' 00"
gptkbp:diameter 1.2 light years
approximately 1.2 light years
gptkbp:discovered_by gptkb:John_Herschel
gptkbp:discovery_year 1834
1884
gptkbp:distance_from_earth approximately 3,800 light years
3,800 light years
gptkbp:exhibition gptkb:NGC_6302
gptkbp:features complex morphology
complex structure
bipolar structure
bipolar outflow
highly collimated jets
gptkbp:first_imaged gptkb:1998
gptkbp:has_color gptkb:blue
gptkb:red
gptkbp:has_spectral_type gptkb:Wolf
https://www.w3.org/2000/01/rdf-schema#label NGC 6302 Nebula
gptkbp:image Hubble image available
gptkbp:is_associated_with planetary nebula phase
mass loss from stars
late-stage stellar evolution
gptkbp:is_located_near the Galactic Center
gptkbp:is_observed_in gptkb:Hubble_Space_Telescope
radio wavelengths
infrared wavelengths
visible wavelengths
gptkbp:is_part_of gptkb:space_exploration
gptkb:interstellar_medium
gptkb:Milky_Way_galaxy
observational astronomy
Galactic Plane
cosmic phenomena
extragalactic astronomy
nebular astronomy
gptkbp:is_studied_for nuclear fusion
stellar nucleosynthesis
stellar winds
gptkbp:is_studied_in gptkb:cosmology
astrophysics
stellar evolution
gptkbp:is_visible_from gptkb:Earth
gptkbp:known_as gptkb:The_Bug_Nebula
gptkb:The_Butterfly_Nebula
gptkbp:lighting magnitude 12.5
magnitude 10.5
gptkbp:located_in gptkb:Milky_Way
constellation Scorpius
gptkbp:notable_feature X-ray emissions
multi-wavelength observations
infrared emissions
ionized gas
asymmetrical shape
scientific interest
astrophysical simulations
high surface brightness
chemical enrichment
dust lanes
spectroscopic studies
ultraviolet emissions
radio emissions
photometric studies
dark lanes
stellar wind interactions
bright central star
complex emission lines
cosmic dust formation
double-lobed structure
high excitation regions
light echoes
mass loss phenomena
nebular dynamics study
photodissociation regions
polar outflows
spectacular colors in images
stellar evolution study
stellar remnant study
gptkbp:research gptkb:spectroscopy
photometry
requires telescope
gptkbp:right_ascension 17h 13m 50s
gptkbp:significance star formation
chemical enrichment
stellar death
gptkbp:type gptkb:Nebula_Award