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