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