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