A) Right ascension and declination. B) Ecliptic longitude and latitude. C) Galactic latitude and longitude. D) Altitude and azimuth.
A) To observe black holes. B) To measure the temperature of planets. C) To study the chemical composition of stars. D) To determine the positions, distances, and motions of celestial objects.
A) 1989. B) 1979. C) 2009. D) 1999.
A) To measure the rotation speed of Mars. B) To study the origin of comets. C) To search for extraterrestrial life. D) To create a precise 3D map of the Milky Way galaxy.
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) Miles B) Kilometers C) Light-years D) Parsec
A) Industrial Revolution. B) Middle Ages. C) Age of Exploration. D) Renaissance.
A) It observes black hole accretion disks. B) It tracks meteor showers. C) It studies distant quasars. D) It helps identify habitable exoplanets by studying their orbital parameters.
A) Locating the North celestial pole. B) Determining the center of mass in a binary star system. C) Finding the center of a galaxy. D) Calculating the rate of expansion of the universe.
A) Hipparchus. B) Kepler. C) Copernicus. D) Galileo.
A) Ecliptic B) Equator C) Prime meridian D) Zenith
A) Greeks B) Romans C) Babylonians D) Egyptians
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) 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. |