Statements (49)
Predicate | Object |
---|---|
gptkbp:instance_of |
gptkb:spiral_galaxy
|
gptkbp:contains |
old stars
|
gptkbp:contains_star |
very low rate
|
gptkbp:diameter |
about 1,000 light-years
|
gptkbp:discovered_by |
gptkb:Hubble_Space_Telescope
|
gptkbp:discovery_year |
gptkb:2000
|
gptkbp:distance_from_earth |
approximately 2.7 million light-years
|
gptkbp:has |
low metallicity
|
gptkbp:has_color |
gptkb:red
|
gptkbp:has_luminosity |
about 1,000 times less than the Milky Way
|
https://www.w3.org/2000/01/rdf-schema#label |
Cetus Dwarf Galaxy
|
gptkbp:is_associated_with |
dark matter halo
the Local Group of galaxies |
gptkbp:is_considered |
a satellite of the Milky Way
a candidate for future observations a faint dwarf galaxy a member of the Milky Way's satellite system |
gptkbp:is_known_for |
its low star formation rate
|
gptkbp:is_located_at |
declination -11° 50′ 00″
right ascension 00h 25m 27s |
gptkbp:is_located_near |
gptkb:Andromeda_Galaxy
|
gptkbp:is_notable_for |
being one of the faintest galaxies
its discovery in the 21st century its faintness and distance |
gptkbp:is_observed_in |
optical wavelengths
infrared wavelengths ground-based telescopes |
gptkbp:is_part_of |
gptkb:Local_Group
the Virgo Supercluster the cosmic web the Local Volume the study of galaxy morphology the Hubble Space Telescope survey |
gptkbp:is_studied_for |
its dark matter content
its chemical composition its evolutionary history galaxy formation theories its stellar dynamics |
gptkbp:is_visible_from |
with telescopes
|
gptkbp:lighting |
very low
|
gptkbp:located_in |
gptkb:Cetus_constellation
|
gptkbp:mass |
mostly old stars
about 10 million solar masses |
gptkbp:orbit_type |
gptkb:Cetus_II
Cetus III |
gptkbp:redshift |
0.0015
|
gptkbp:type |
spheroidal galaxy
|
gptkbp:bfsParent |
gptkb:Milky_Way_satellites
|
gptkbp:bfsLayer |
6
|