CHAPTER 2 NOTES (STARS AND GALAXIES)
... 3 types of galaxies are: 1. spiral- arms like a pinwheel ex our galaxy- Milky Way 2. elliptical- nearly spherical to flatdisks (older than other galaxies) 3. irregular- no orderly or definite shape, not very common Milky Way Galaxy- pinwheel shaped disk with bulge in center -the older stars are near ...
... 3 types of galaxies are: 1. spiral- arms like a pinwheel ex our galaxy- Milky Way 2. elliptical- nearly spherical to flatdisks (older than other galaxies) 3. irregular- no orderly or definite shape, not very common Milky Way Galaxy- pinwheel shaped disk with bulge in center -the older stars are near ...
Cosmic Distance Ladder
... the Earth causes nearby stars to appear to move relative to the more distant stars. • The annual parallax is defined as the difference in position of a star as seen from the Earth and Sun, i.e. the angle subtended at a star by the mean radius of the Earth's orbit around the Sun. ...
... the Earth causes nearby stars to appear to move relative to the more distant stars. • The annual parallax is defined as the difference in position of a star as seen from the Earth and Sun, i.e. the angle subtended at a star by the mean radius of the Earth's orbit around the Sun. ...
Apparent motion
... Moon Phases • Full moon Full moon takes 29 ½ days →Earth moves in its orbit as the moon travels around the Earth →When the moon makes one full revolution around the Earth it is not seen on Earth as being in the same phase due to the Earth’s change in position Moon must go further to be seen in ...
... Moon Phases • Full moon Full moon takes 29 ½ days →Earth moves in its orbit as the moon travels around the Earth →When the moon makes one full revolution around the Earth it is not seen on Earth as being in the same phase due to the Earth’s change in position Moon must go further to be seen in ...
Planetarium Key Points
... Latitude is the elevation of the visible pole and, roughly, of Polaris The motion of the sphere seems uniform, for this reason it was the source for time telling, but the time scale that comes from is NOT uniform: rotation is slowing down, the day is longer and longer at the rate of 2 ms a centu ...
... Latitude is the elevation of the visible pole and, roughly, of Polaris The motion of the sphere seems uniform, for this reason it was the source for time telling, but the time scale that comes from is NOT uniform: rotation is slowing down, the day is longer and longer at the rate of 2 ms a centu ...
Earth and Stars
... the Earth is the Sun - all other known stars are at distances greater than 1 pc and parallax angles less than 1 arcsec. When measuring the parallax of a star, it is important to account for the star's proper motion, and the parallax of any of the 'fixed' stars used as ...
... the Earth is the Sun - all other known stars are at distances greater than 1 pc and parallax angles less than 1 arcsec. When measuring the parallax of a star, it is important to account for the star's proper motion, and the parallax of any of the 'fixed' stars used as ...
Ch. 16 Notes
... The tail consists of two parts. A dust tail made of pieces of the comet lit by sunlight and an ion tail made of charged particles created by passing through the solar wind. The tail is only visible as the comet approaches the sun. It shrinks and disappears as the comet orbits away. Studying comets l ...
... The tail consists of two parts. A dust tail made of pieces of the comet lit by sunlight and an ion tail made of charged particles created by passing through the solar wind. The tail is only visible as the comet approaches the sun. It shrinks and disappears as the comet orbits away. Studying comets l ...
The Sun to the Earth - Stanford Solar Center
... A solar “wind” streams into the solar system and shapes Earth’s magnetosphere ...
... A solar “wind” streams into the solar system and shapes Earth’s magnetosphere ...
Volume 1 (Issue 3), March 2012
... therefore, the Moon will be fully illuminated as seen from Earth. March 14, 2012 - Conjunction of Venus and Jupiter The two bright planets will appear 3 degrees apart from each other in the sky in the west direction. ...
... therefore, the Moon will be fully illuminated as seen from Earth. March 14, 2012 - Conjunction of Venus and Jupiter The two bright planets will appear 3 degrees apart from each other in the sky in the west direction. ...
Chpt 26- Studying Space:
... • The Voyager 1 and Voyager 2 spacecraft investigated Jupiter, Saturn, Uranus, and Neptune, and collected images of these planets and their moons. • The Galileo spacecraft orbited Jupiter and its moons from 1995 to 2003. • The Cassini-Huygens spacecraft will study Titan, Saturn’s largest moon. Like ...
... • The Voyager 1 and Voyager 2 spacecraft investigated Jupiter, Saturn, Uranus, and Neptune, and collected images of these planets and their moons. • The Galileo spacecraft orbited Jupiter and its moons from 1995 to 2003. • The Cassini-Huygens spacecraft will study Titan, Saturn’s largest moon. Like ...
7th Grade Astronomy Study Guide
... c. day b. year d. month ____ 26. Why do astronomers put telescopes in space? a. to avoid interference from the Earth’s atmosphere b. to avoid noise pollution c. to reduce air pollution d. to get closer to objects in space ____ 27. An advantage of reflecting telescopes over refracting telescopes is t ...
... c. day b. year d. month ____ 26. Why do astronomers put telescopes in space? a. to avoid interference from the Earth’s atmosphere b. to avoid noise pollution c. to reduce air pollution d. to get closer to objects in space ____ 27. An advantage of reflecting telescopes over refracting telescopes is t ...
UCCS Solar Energy ENSC/PES 1600 Fall 2010 Earth, Sun, Time
... 15) What kind of time can be read directly from a sundial? A) apparent solar time B) mean solar time C) standard time D) daylight saving time E) sidereal time 16) All the following statements are true. Which one explains why mean solar time differs from apparent solar time? A) The length of a solar ...
... 15) What kind of time can be read directly from a sundial? A) apparent solar time B) mean solar time C) standard time D) daylight saving time E) sidereal time 16) All the following statements are true. Which one explains why mean solar time differs from apparent solar time? A) The length of a solar ...
Regents Review Questions.Unit 1.PlanetEarthTopo.Map.KEY
... 4 The diagram on the right shows latitude measurements every 10 degrees and longitude measurements every 15 degrees. ...
... 4 The diagram on the right shows latitude measurements every 10 degrees and longitude measurements every 15 degrees. ...
Components of the Solar System Learning Targets
... Venus hottest, greenhouse effect, dense atmosphere, rotates opposite of other planets, Earth’s sister (because of size only), layers, volcanic activity, longest day (day is longer than its year), no moons, Earth liquid water, one moon, layers, atmosphere, greenhouse effect, volcanic activity, only p ...
... Venus hottest, greenhouse effect, dense atmosphere, rotates opposite of other planets, Earth’s sister (because of size only), layers, volcanic activity, longest day (day is longer than its year), no moons, Earth liquid water, one moon, layers, atmosphere, greenhouse effect, volcanic activity, only p ...
PowerPoint file - High Point University
... • How do we know the mass of Pluto? • Its density is 2 g/cm3. What do you think it’s made of? • It’s similar to the moons of the Jovian planets. Why is it most likely not a “lost moon” of one of the Jovian planets? • If there’s one object like Pluto, could there be more? ...
... • How do we know the mass of Pluto? • Its density is 2 g/cm3. What do you think it’s made of? • It’s similar to the moons of the Jovian planets. Why is it most likely not a “lost moon” of one of the Jovian planets? • If there’s one object like Pluto, could there be more? ...
PowerPoint Presentation - AST121 Introduction to Astronomy
... • How do we know the mass of Pluto? • Its density is 2 g/cm3. What do you think it’s made of? • It’s similar to the moons of the Jovian planets. Why is it most likely not a “lost moon” of one of the Jovian planets? • If there’s one object like Pluto, could there be more? ...
... • How do we know the mass of Pluto? • Its density is 2 g/cm3. What do you think it’s made of? • It’s similar to the moons of the Jovian planets. Why is it most likely not a “lost moon” of one of the Jovian planets? • If there’s one object like Pluto, could there be more? ...
Lecture
... • The main reason is that the moon’s orbit is tilted from the earth’s orbit. • A total eclipse from a given point on the surface of the Earth is not a common occurrence. • Eclipse can be predicted: two eclipses every year. ...
... • The main reason is that the moon’s orbit is tilted from the earth’s orbit. • A total eclipse from a given point on the surface of the Earth is not a common occurrence. • Eclipse can be predicted: two eclipses every year. ...
Sun, Moon and Stars - Siemens Science Day
... Use the flashlight to show students how the sun shines onto Earth, creating daytime on one half of the planet and nighttime on the other half. Demonstrate for students that sunlight and darkness travel to different areas of Earth because Earth spins on its axis. It takes 24 hours for this process to ...
... Use the flashlight to show students how the sun shines onto Earth, creating daytime on one half of the planet and nighttime on the other half. Demonstrate for students that sunlight and darkness travel to different areas of Earth because Earth spins on its axis. It takes 24 hours for this process to ...
What Makes Up the Solar System?
... Saturn is best known for its rings, which is made of ice, dust, boulders, and frozen gases. Like Jupiter, Saturn has dozens of moons. Jupiter and Saturn are the only planets that can be seen from a telescope. ...
... Saturn is best known for its rings, which is made of ice, dust, boulders, and frozen gases. Like Jupiter, Saturn has dozens of moons. Jupiter and Saturn are the only planets that can be seen from a telescope. ...
Solar System topics
... Pluto was discovered in 1930 by the American astronomer Clyde Tombaugh. It was the culmination of a many-year search at Lowell Observatory in Flagstaff, Arizona. It was regarded as an official planet until 2006. Now it is considered a dwarf planet. To be regarded as a planet an object must: 1) orbi ...
... Pluto was discovered in 1930 by the American astronomer Clyde Tombaugh. It was the culmination of a many-year search at Lowell Observatory in Flagstaff, Arizona. It was regarded as an official planet until 2006. Now it is considered a dwarf planet. To be regarded as a planet an object must: 1) orbi ...
Distribution of Elements in the Earth`s Crust
... The formation of Earth and our solar system was affected by a number of additional physical processes. The newly formed sun sent out a constant stream of particles called solar wind, which tended to sweep lighter elements out toward the farther reaches of the solar system. There they formed planets ...
... The formation of Earth and our solar system was affected by a number of additional physical processes. The newly formed sun sent out a constant stream of particles called solar wind, which tended to sweep lighter elements out toward the farther reaches of the solar system. There they formed planets ...
Gravitational Interactions
... Weight & Weightlessness • Weightlessness is not the absence of gravity. It is the absence of a support force. ...
... Weight & Weightlessness • Weightlessness is not the absence of gravity. It is the absence of a support force. ...
Schedule for Spring 2013 SCI 103 Introductory Astronomy
... Practical Problems Diurnal Motion Long term motion Classification of Interior and Superior planets Brief presentation of Aristotle and Ptolemy’s Universe: Geocentric Model ...
... Practical Problems Diurnal Motion Long term motion Classification of Interior and Superior planets Brief presentation of Aristotle and Ptolemy’s Universe: Geocentric Model ...
Exploring the Universe
... 2. Red shift: the apparent shift toward longer wavelengths of light caused when a luminous object moves away from the observer a. Red shift showed that nearly all galaxies are getting farther away from Earth 3. Blue shift: an apparent shift toward shorter wavelengths of light caused when a luminous ...
... 2. Red shift: the apparent shift toward longer wavelengths of light caused when a luminous object moves away from the observer a. Red shift showed that nearly all galaxies are getting farther away from Earth 3. Blue shift: an apparent shift toward shorter wavelengths of light caused when a luminous ...
fall_2000_final
... C. uniformly composed of hydrogen and helium. D. uniformly composed of helium. E. composed of molecules containing mostly carbon and iron. 45. When two galaxies collide with one another their shapes are distorted by A. collisions of individual stars. B. a gigantic explosion resulting from such a col ...
... C. uniformly composed of hydrogen and helium. D. uniformly composed of helium. E. composed of molecules containing mostly carbon and iron. 45. When two galaxies collide with one another their shapes are distorted by A. collisions of individual stars. B. a gigantic explosion resulting from such a col ...
Geocentric model
In astronomy, the geocentric model (also known as geocentrism, or the Ptolemaic system) is a description of the cosmos where Earth is at the orbital center of all celestial bodies. This model served as the predominant cosmological system in many ancient civilizations such as ancient Greece including the noteworthy systems of Aristotle (see Aristotelian physics) and Ptolemy. As such, they believed that the Sun, Moon, stars, and naked eye planets circled Earth.Two commonly made observations supported the idea that Earth was the center of the Universe. The stars, the sun, and planets appear to revolve around Earth each day, making Earth the center of that system. The stars were thought to be on a celestial sphere, with the earth at its center, that rotated each day, using a line through the north and south pole as an axis. The stars closest to the equator appeared to rise and fall the greatest distance, but each star circled back to its rising point each day. The second observation supporting the geocentric model was that the Earth does not seem to move from the perspective of an Earth-bound observer, and that it is solid, stable, and unmoving.Ancient Roman and medieval philosophers usually combined the geocentric model with a spherical Earth. It is not the same as the older flat Earth model implied in some mythology, as was the case with the biblical and postbiblical Latin cosmology. The ancient Jewish Babylonian uranography pictured a flat Earth with a dome-shaped rigid canopy named firmament placed over it. (רקיע- rāqîa').However, the ancient Greeks believed that the motions of the planets were circular and not elliptical, a view that was not challenged in Western culture until the 17th century through the synthesis of theories by Copernicus and Kepler.The astronomical predictions of Ptolemy's geocentric model were used to prepare astrological and astronomical charts for over 1500 years. The geocentric model held sway into the early modern age, but from the late 16th century onward was gradually superseded by the heliocentric model of Copernicus, Galileo and Kepler. There was much resistance to the transition between these two theories. Christian theologians were reluctant to reject a theory that agreed with Bible passages (e.g. ""Sun, stand you still upon Gibeon"", Joshua 10:12 – King James 2000 Bible). Others felt a new, unknown theory could not subvert an accepted consensus for geocentrism.