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