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Chapter 18—Observing the Sky Astronomy—the study of all physical objects beyond Earth Calendar—a system for organizing time; most calendars organize time within a single unit called a year Year—the time required for the Earth to orbit the sun once Month—roughly the amount of time required for the moon to orbit the Earth once Day—the time required for the Earth to rotate once on its axis Leap year—a year in which an extra day is added to the calendar Constellation—a section of the sky that contains a recognizable star pattern Altitude—the angle between an object in the sky and the horizon Right ascension—a measure of how far east an object is from the point at which the sun appears on the first day of spring Declination—a measure of how far north or south an object is from the celestial equator Celestial equator—imaginary circle created by extending Earth’s equator into space Ecliptic—the apparent path the sun takes across the celestial sphere each year Light-year—a unit of length equal to the distance that light travels through space in 1 year Telescope—an instrument that collects electromagnetic radiation from the sky and concentrates it for better observation Refracting telescope—a telescope that uses a set of lenses to gather and focus light Chapter 18—Continued Reflecting telescope—a telescope that uses curved mirrors to gather and focus light Electromagnetic spectrum—all the wavelengths of electromagnetic radiation Chapter 19—Formation of the Solar System Solar system—the system composed of the sun (a star) and the planets and other bodies that travel around the sun Nebula—a large cloud of dust and gas in interstellar space; the location of star formation Solar nebula—the nebula that formed into the solar system Planetesimal—the tiny building block of the planets that formed as dust particles stuck together and grew in size Rotation—the spinning motion of a body on its axis Orbit—the elliptical path a body takes as it travels around another body in space; the motion itself Revolution—the elliptical motion of a body as it orbits another body in space Period of revolution—the time it takes for one body to make one complete orbit; or revolution, around another body in space Ellipse—a closed curve in which the sum of the distances from the edge of the curve to two points inside the ellipse is always the same Astronomical unit (AU)—the average distance between the Earth and the sun, or approximately 150,000,000 km Corona—the sun’s outer atmosphere, which can extend outward a distance equal to 10-12 times the diameter of the sun Chromosphere—a thin region of the sun’s atmosphere between the corona and the photosphere; too faint to see unless there is a total solar eclipse Photosphere—the layer of the sun at which point the gases get thick enough to see; the surface of the sun Chapter 19—Continued Convective zone—a region of the sun where gases circulate in convection currents, bringing the sun’s energy to the surface Radiative zone—a very dense region of the sun in which the atoms are so closely packed that light can take millions of years to pass through Core—the center of the sun where the sun’s energy is produced Nuclear fusion—the process by which two or more nuclei with small masses join together, or fuse, to form a larger, more massive nucleus, along with the production of energy Sunspot—an area on the photosphere of the sun that is cooler than surrounding areas, showing up as a dark spot Crust—the thin, outermost layer of the Earth, or the uppermost part of the lithosphere Mantle—the layer of the Earth between the crust and the core Core—the central, spherical part the Earth below the mantle Chapter 20—A Family of Planets Astronomical unit (AU)—the average age distance between the Earth and the sun, or approximately 150,000,000 km Terrestrial planets—the small, dense, rocky planets of the inner solar system Prograde rotation—the counter-clockwise spin of a planet or moon as seen from above the planet’s North Pole Retrograde rotation—the clockwise spin of a planet or moon as seen from above the planet’s North Pole Gas giants—the large, gaseous planets of the outer solar system Satellite—a natural or artificial body that revolves around a planet Phases—the different appearances of the moon due to varying amounts of sunlight on the side of the moon that faces the Earth; results from the changing relative positions of the moon, Earth, and the sun Eclipse—an event in which the shadow of one celestial body falls on another Comet—a small body of ice, rock, and cosmic dust loosely packed together that gives off gas and dust in the form of a tail as it passes close to the sun Asteroid—a small, rock body that revolves around the sun Asteroid belt—the region of the solar system most asteroids occupy; roughly between the orbits of Mars and Jupiter Meteoroid—a very small, rocky body that revolves around the sun Meteorite—a meteoroid that reaches the Earth’s surface without burning up completely Meteor—a streak of light caused when a meteoroid or comet dust burns up in the Earth’s atmosphere before it reaches the ground Chapter 21—The Universe Beyond Spectrum—the rainbow of colors produced when white light passes through a prism or spectrograph Apparent magnitude—how bright a light appears to an observer Absolute magnitude—the actual brightness of a star Light-year—a unit of length equal to the distance that light travels through space in 1 year Parallax—an apparent shift in the position of an object when viewed from different locations H-R diagram—Hertzsprung-Russell diagram; a graph that shows the relationship between a star’s surface temperature and its absolute magnitude Main sequence—a diagonal pattern of stars on the H-R diagram White dwarf—a small, hot star near the end of its life; the leftover center of an old star Red giant—a star that expands and cools once it runs out of hydrogen fuel Supernova—the death of a large star by explosion Neutron star—a star in which all the particles have become neutrons; the collapsed remains of a supernova Pulsar—a spinning neutron star that emits rapid pulses of light Black hole—an object with more than three solar masses squeezed into a ball only 10 km across whose gravity is so strong that not even light can escape Galaxy—a large grouping of stars in space Spiral galaxy—a galaxy with a bulge in the center and very distinctive spiral arms Chapter 21—Continued Elliptical galaxy—a spherical or elongated galaxy with a bright center and very little dust and gas Irregular galaxy—a galaxy that does not fit into any other category; one with an irregular shape Nebula—a large cloud of dust and gas in interstellar space; the location of star formation Open cluster—a group of stars that are usually located along the spiral disk of a galaxy Globular cluster—a group of older stars that looks like a ball of stars Quasar—“quasi-stellar” object; a star-like source of light that is extremely far away; one of the most powerful sources of energy in the universe Cosmology—the study of the origin and future of the universe Big bang theory—the theory that states the universe began with a tremendous explosion Cosmic background radiation—radiation left over from the big bang that fills all of space Chapter 22—Exploring Space Rocket—a machine that uses escaping gas to move NASA—National Aeronautics and Space Administration; founded to combine all of the separate rocket-development teams in the United States Thrust—the force that accelerates a rocket Orbital velocity—the speed and direction a rocket must have in order to orbit the Earth Escape velocity—the speed and direction a rocket must travel in order to completely break away from a planet’s gravitational pull Artificial satellite—any human-made object placed in orbit around a body in space Low Earth orbit—an orbit located a few hundred kilometers above the Earth’s surface Geosynchronous orbit—an orbit in which a satellite travels at a speed that matches the rotational speed of the Earth exactly, keeping the satellite positioned above the same spot on Earth at all times Space probe—a vehicle that carries scientific instruments to planets or other bodies in space Space shuttle—a reusable vehicle that takes off like a rocket and lands like an airplane Space station—a long-term orbiting platform from which other vehicles can be launched or scientific research can be carried out