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