# data[].attributes.body
the earth's natural satellite, orbiting the earth at a mean distance of 238,857 miles (384,393 km) and having a diameter of 2160 miles (3476 km).

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any of the small bodies, often remnants of comets, traveling through space: when such a body enters the earth's atmosphere it is heated to luminosity and becomes a meteor.

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so called major planet. any of the eight large heavenly bodies revolving about the sun and shining by reflected light: Mercury,Venus, Earth, Mars, Jupiter, Saturn, Uranus, or Neptune, in the order of their proximity to the sun. Until 2006, Pluto was classifieds a planet ninth in order from the sun; it has been reclassified also dwarf planet

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a celestial body moving about the sun, usually in a highly eccentricorbit, consisting of a central mass surrounded by an envelope of dustand gas that may form a tail that streams away from the sun.

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Also called minor planet. Astronomy. any of the thousands of small bodies of from 480 miles (775 km) to less than one mile (1.6 km) in diameter that revolve about the sun in orbits lying mostly between those of Mars and Jupiter.

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a large system of stars held together by mutual gravitation and isolated from similar systems by vast regions of space

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any of the heavenly bodies, except the moon, appearing as fixed luminous points in the sky at night.

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the force of attraction by which terrestrial bodies tend to fall towardthe center of the earth.

# data[].attributes.headline
          Universe                                   the totality of known or supposed objects and phenomena throughout space; the cosmos; macrocosm.

# data[].attributes.subject
          Universe                                   the totality of known or supposed objects and phenomena throughout space; the cosmos; macrocosm.

# data[].attributes.body
the star that is the central body of thesolar system, around which the planets revolve and from which theyreceive light and heat: its mean distance from the earth is about 93million miles (150 million km), its diameter about 864,000 miles (1.4million km), and its mass about 330,000 times that of the earth; itsperiod of surface rotation is about 26 days at its equator but longer athigher latitudes.