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