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A) Right ascension and declination. B) Altitude and azimuth. C) Galactic latitude and longitude. D) Ecliptic longitude and latitude.
A) To determine the positions, distances, and motions of celestial objects. B) To measure the temperature of planets. C) To study the chemical composition of stars. D) To observe black holes.
A) 1999. B) 2009. C) 1989. D) 1979.
A) To create a precise 3D map of the Milky Way galaxy. B) To measure the rotation speed of Mars. C) To study the origin of comets. D) To search for extraterrestrial life.
A) Apparent motion of a star across the sky over time. B) Brightness of a star. C) Size of a planet. D) Distance to a galaxy.
A) Parsec B) Light-years C) Kilometers D) Miles
A) Middle Ages. B) Age of Exploration. C) Industrial Revolution. D) Renaissance.
A) It helps identify habitable exoplanets by studying their orbital parameters. B) It studies distant quasars. C) It tracks meteor showers. D) It observes black hole accretion disks.
A) Determining the center of mass in a binary star system. B) Locating the North celestial pole. C) Finding the center of a galaxy. D) Calculating the rate of expansion of the universe.
A) Kepler. B) Galileo. C) Copernicus. D) Hipparchus.
A) Ecliptic B) Prime meridian C) Zenith D) Equator
A) Greeks B) Romans C) Egyptians D) Babylonians
A) A projection of Earth's equator onto the celestial sphere. B) A line that connects the North and South celestial poles. C) A region in space with high concentration of galaxies. D) An imaginary line connecting the stars Sirius and Procyon.
A) A collection of asteroid names. B) A list of exoplanets discovered by NASA. C) A compilation of meteorite impact craters. D) A stellar catalog that provides positions and proper motions of 2.5 million stars. |