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