Statements (110)
Predicate | Object |
---|---|
gptkbp:instance_of |
gptkb:galaxy
|
gptkbp:bfsLayer |
4
|
gptkbp:bfsParent |
gptkb:Cetus
|
gptkbp:apparent_magnitude |
11.0
11.5 elliptical diagram |
gptkbp:body_style |
active nucleus
|
gptkbp:contains |
gptkb:football_club
low elliptical |
gptkbp:coordinates |
RA 02h 41m 04.0s, Dec -08° 15' 20"
l= 100.0°, b= -30.0° |
gptkbp:depicted_in |
gptkb:battle
optical wavelengths |
gptkbp:diameter |
approximately 50,000 light-years
approximately 30,000 light-years |
gptkbp:discovered_by |
gptkb:John_Herschel
|
gptkbp:distance |
approximately 60 million light-years
|
gptkbp:exhibition |
gptkb:NGC
|
gptkbp:features |
bright central region
|
gptkbp:has |
gptkb:physicist
a complex morphology a prominent dust lane a significant amount of hot gas old stellar population several satellite galaxies a relatively low star formation rate low surface brightness regions |
gptkbp:has_color |
B-V 0.9
|
gptkbp:has_feature |
E0-1
|
gptkbp:has_luminosity |
high
|
gptkbp:has_spectral_type |
S0
E0 |
gptkbp:has_team |
NED 1052
|
https://www.w3.org/2000/01/rdf-schema#label |
NGC 1052
|
gptkbp:is |
a source of radio emissions
a galaxy that has been analyzed for its gravitational lensing effects visible in amateur telescopes one of the brightest galaxies in its group a galaxy that has been observed in multiple wavelengths a part of the cosmic web a subject of various astronomical surveys a galaxy that has been studied for its chemical composition a subject of photometric studies often included in galaxy catalogs a target for gravitational wave studies part of the larger structure of the universe an object of interest for stellar dynamics research a galaxy that has been studied for its interaction with nearby galaxies a galaxy that exhibits signs of past mergers a galaxy with a notable core structure a galaxy with a significant history of observation a member of the NGC catalog a target for studying galaxy evolution an example of a low-luminosity active galaxy an important object in cosmology studies associated with a group of galaxies often compared to other elliptical galaxies often imaged in deep-sky photography often studied in X-ray astronomy a galaxy that has been used as a benchmark for other studies. a galaxy that has been observed for its peculiar features a galaxy that has been included in various astronomical databases a galaxy that has been used to test cosmological models a galaxy that has been the subject of numerous research papers a galaxy that contributes to our understanding of dark matter |
gptkbp:is_active_in |
gptkb:battle
|
gptkbp:is_associated_with |
gptkb:physicist
radio emissions |
gptkbp:is_known_for |
gptkb:UGC_2200
|
gptkbp:is_observed_in |
gptkb:Hubble_Space_Telescope
infrared wavelengths |
gptkbp:is_part_of |
gptkb:Laniakea_Supercluster
gptkb:Cetus_constellation local supercluster Cetus constellation group Cetus constellation region Cetus group of galaxies Cetus supercluster NGC 1052 cluster NGC 1052 group NGC 1052 group of galaxies |
gptkbp:is_studied_in |
gptkb:spacecraft
gptkb:observatory stellar evolution stellar populations black hole physics galaxy evolution galaxy dynamics |
gptkbp:isotopes |
gptkb:battle
|
gptkbp:lighting |
gptkb:battle
low |
gptkbp:located_in |
constellation Cetus
Declination -8° 15' 20" Right Ascension 2h 41m 4s |
gptkbp:mass |
approximately 10^11 solar masses
approximately 10 billion solar masses |
gptkbp:notable_models |
elliptical structure
E0 NGC 1052-D F2 stable dynamics |
gptkbp:orbital_period |
none known
|
gptkbp:part_of |
NGC 1052 group
|
gptkbp:population |
low density
|
gptkbp:redshift |
0.0053
0.0054 |
gptkbp:speed |
160 km/s
|
gptkbp:type |
gptkb:galaxy
|
gptkbp:year_created |
1827
1834 |