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