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