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