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