a photograph of a celestial body
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astrophotographa photograph of a celestial body
redshifta displacement of the spectrum of a celestial body
redshiftsREDSHIFT, a displacement of the spectrum of a celestial body
orbitthe curved path of a planet, satellite, etc., around a celestial body
variationA deviation of a celestial body from its mean orbit or motion
orbitsthe curved path of a planet, satellite, etc., around a celestial body
variationsA deviation of a celestial body from its mean orbit or motion
transitsThe apparent passage of a celestial body across the meridian of a place
southingsa. the transit of a heavenly body across the celestial meridian b. south declination
transiting(of a celestial body) Pass across (a specified sign, house, or area of a chart)
transited(of a celestial body) Pass across (a specified sign, house, or area of a chart)
transitsThe passage of a celestial body through a specified sign, house, or area of a chart
swingbyA change in the flight path of a spacecraft using the gravitational pull of a celestial body
transiting(of a planet or other celestial body) Pass across (a meridian or the face of another body)
swingbysA change in the flight path of a spacecraft using the gravitational pull of a celestial body
transited(of a planet or other celestial body) Pass across (a meridian or the face of another body)
aspectsA particular position of a planet or other celestial body relative to another, as measured by angular distance
capturing(of a star, planet, or other celestial body) Bring (a less massive body) permanently within its gravitational influence
afflict(of a celestial body) Be in a stressful aspect with (another celestial body or a point on the ecliptic)
afflicts(of a celestial body) Be in a stressful aspect with (another celestial body or a point on the ecliptic)
perturbationsA minor deviation in the course of a celestial body, caused by the gravitational attraction of a neighboring body
afflicted(of a celestial body) Be in a stressful aspect with (another celestial body or a point on the ecliptic)
perturbationA minor deviation in the course of a celestial body, caused by the gravitational attraction of a neighboring body
afflicting(of a celestial body) Be in a stressful aspect with (another celestial body or a point on the ecliptic)
periheliathe point in the path of a celestial body (as a planet) that is nearest to the sun compare aphelion
suborbitalOf, relating to, or denoting a trajectory that does not complete a full orbit of the earth or other celestial body
slingshotsThe effect of the gravitational pull of a celestial body in accelerating and changing the course of another body or a spacecraft
slingshotThe effect of the gravitational pull of a celestial body in accelerating and changing the course of another body or a spacecraft
grabena depressed segment of the crust of the earth or a celestial body (as the moon) bounded on at least two sides by faults
cometsa celestial body that appears as a fuzzy head usually surrounding a bright nucleus, that has a usually highly eccentric orbit, that consists primarily of ice and dust, and that often develops one or more long tails when near the sun
cometica celestial body that appears as a fuzzy head usually surrounding a bright nucleus, that has a usually highly eccentric orbit, that consists primarily of ice and dust, and that often develops one or more long tails when near the sun
cometarya celestial body that appears as a fuzzy head usually surrounding a bright nucleus, that has a usually highly eccentric orbit, that consists primarily of ice and dust, and that often develops one or more long tails when near the sun
sunthe luminous celestial body around which the earth and other planets revolve, from which they receive heat and light, which is composed mainly of hydrogen and helium, and which has a mean distance from earth of about 93,000,000 miles (150,000,000 kilometers), a linear diameter of 864,000 miles (1,390,000 kilometers), and a mass 332,000 times greater than earth
sunsthe luminous celestial body around which the earth and other planets revolve, from which they receive heat and light, which is composed mainly of hydrogen and helium, and which has a mean distance from earth of about 93,000,000 miles (150,000,000 kilometers), a linear diameter of 864,000 miles (1,390,000 kilometers), and a mass 332,000 times greater than earth