Hyperonyms
(has_hyperonym)
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07951464-n:
several things grouped together or considered as a whole
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Hyponyms
(has_hyponym)
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08271457-n:
a galaxy having a spiral structure; arms containing younger stars spiral out from old stars at the center
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Hyponyms
(has_hyponym)
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09291781-n:
a massive grouping of galaxies in the direction of Centaurus and Hydra whose gravitational attraction is believed to cause deviations in the paths of other galaxies
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Hyponyms
(has_hyponym)
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09345503-n:
either of two small galaxies orbiting the Milky Way; visible near the south celestial pole
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Hyponyms
(has_hyponym)
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09354984-n:
the galaxy containing the solar system; consists of millions of stars that can be seen as a diffuse band of light stretching across the night sky
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Holonyms
(has_holo_member)
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09466280-n:
everything that exists anywhere
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Meronyms
(has_mero_madeof)
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11441416-n:
clouds of particles or gases occurring throughout interstellar space
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Meronyms
(has_mero_member)
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09444100-n:
(astronomy) a celestial body of hot gases that radiates energy derived from thermonuclear reactions in the interior
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Related
(has_pertainym)
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02849098-a:
of or relating to a galaxy (especially our galaxy the Milky Way)
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Related
(has_pertainym)
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02849257-a:
outside or beyond a galaxy
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Related
(has_pertainym)
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02849367-a:
between or among galaxies
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Related
(related_to)
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02849098-a:
of or relating to a galaxy (especially our galaxy the Milky Way)
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Domain
(category)
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06095022-n:
the branch of physics that studies celestial bodies and the universe as a whole
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Glosses
(gloss)
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07951464-n:
several things grouped together or considered as a whole
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Glosses
(gloss)
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09366940-n:
an immense cloud of gas (mainly hydrogen) and dust in interstellar space
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Glosses
(gloss)
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09444100-n:
(astronomy) a celestial body of hot gases that radiates energy derived from thermonuclear reactions in the interior
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Glosses
(gloss)
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13776432-n:
a very large indefinite number (usually hyperbole)
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Glosses
(gloss)
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14840092-n:
free microscopic particles of solid material
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Glosses
(rgloss)
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02849098-a:
of or relating to a galaxy (especially our galaxy the Milky Way)
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Glosses
(rgloss)
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02849257-a:
outside or beyond a galaxy
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Glosses
(rgloss)
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02849367-a:
between or among galaxies
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Glosses
(rgloss)
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05879204-n:
(astronomy) the generalization that the speed of recession of distant galaxies (the red shift) is proportional to their distance from the observer
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Glosses
(rgloss)
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08271457-n:
a galaxy having a spiral structure; arms containing younger stars spiral out from old stars at the center
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Glosses
(rgloss)
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08501887-n:
the space between galaxies
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Glosses
(rgloss)
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09251229-n:
a constellation in the northern hemisphere between Ursa Major and Bootes; contains a cluster of some 10,000 galaxies
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Glosses
(rgloss)
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09291781-n:
a massive grouping of galaxies in the direction of Centaurus and Hydra whose gravitational attraction is believed to cause deviations in the paths of other galaxies
|
Glosses
(rgloss)
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09345503-n:
either of two small galaxies orbiting the Milky Way; visible near the south celestial pole
|
Glosses
(rgloss)
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09354984-n:
the galaxy containing the solar system; consists of millions of stars that can be seen as a diffuse band of light stretching across the night sky
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Glosses
(rgloss)
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11215541-n:
Dutch astronomer who proved that the galaxy is rotating and proposed the existence of the Oort cloud (1900-1992)
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Glosses
(rgloss)
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11513357-n:
(astronomy) a shift in the spectra of very distant galaxies toward longer wavelengths (toward the red end of the spectrum); generally interpreted as evidence that the universe is expanding
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Glosses
(rgloss)
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13590598-n:
(cosmology) the ratio of the speed of recession of a galaxy (due to the expansion of the universe) to its distance from the observer; the Hubble constant is not actually a constant, but is regarded as measuring the expansion rate today
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