
Faux Final
... 13) What is the “local group” of galaxies and what are the most massive galaxies in it? 14) What is the evidence for dark matter? 15) Sketch, for galaxies within 1000 Mpc, the velocity-distance diagram. State the common name of the diagram. What is the implication of the diagram for cosmology? 16) D ...
... 13) What is the “local group” of galaxies and what are the most massive galaxies in it? 14) What is the evidence for dark matter? 15) Sketch, for galaxies within 1000 Mpc, the velocity-distance diagram. State the common name of the diagram. What is the implication of the diagram for cosmology? 16) D ...
Astronomy- The Original Science
... Telescope to the Sky •In 1609, Galileo Galilei became one of the first people to use a telescope to observe objects in space. •He discovered craters and mountains on the Earth’s moon, four of Jupiter's moons, sunspots on the sun, and the phases of Venus. •These discoveries showed that the planets ar ...
... Telescope to the Sky •In 1609, Galileo Galilei became one of the first people to use a telescope to observe objects in space. •He discovered craters and mountains on the Earth’s moon, four of Jupiter's moons, sunspots on the sun, and the phases of Venus. •These discoveries showed that the planets ar ...
Chapter 24 Test:Stars/Galaxies
... viewed from two locations. (a) Apparent magnitude, (b) The Doppler shift, (c) Absolute magnitude, (d) Parallax. ...
... viewed from two locations. (a) Apparent magnitude, (b) The Doppler shift, (c) Absolute magnitude, (d) Parallax. ...
Origin of the Universe
... energy in specific portions-wavelengths-within the electromagnetic spectrum. Because the human eye observes different wavelengths of visible light as different colors, people can distinguish specific portions of the electiomagrretic spectrum. When scientists study the spectrum of electromagnetic ene ...
... energy in specific portions-wavelengths-within the electromagnetic spectrum. Because the human eye observes different wavelengths of visible light as different colors, people can distinguish specific portions of the electiomagrretic spectrum. When scientists study the spectrum of electromagnetic ene ...
Rachel Henning
... Sun will start to run out. The helium will get squeezed. This will speed up the hydrogen burning. Our star will slowly puff into a red giant, which is a star that has exhausted it hydrogen and is burning helium fuel. It will eat all of the inner planets, even the Earth. Then the sun would burn into ...
... Sun will start to run out. The helium will get squeezed. This will speed up the hydrogen burning. Our star will slowly puff into a red giant, which is a star that has exhausted it hydrogen and is burning helium fuel. It will eat all of the inner planets, even the Earth. Then the sun would burn into ...
Science, 4th 9 weeks
... The cosmos is vast and explored well enough to know its basic structure and operational principles. Everything in the Universe exerts a gravitational force on everything else; there is interplay between magnetic fields and electrical currents. ...
... The cosmos is vast and explored well enough to know its basic structure and operational principles. Everything in the Universe exerts a gravitational force on everything else; there is interplay between magnetic fields and electrical currents. ...
Announcements
... hydrogen. At first the deuterons are broken up by the high energy gamma rays. Once the temperature cools enough they can survive long enough for the next step. ...
... hydrogen. At first the deuterons are broken up by the high energy gamma rays. Once the temperature cools enough they can survive long enough for the next step. ...
Owsley Brown II Portable Planetarium 9
... ● Kepler’s laws describe common features of the motions of orbiting objects, including their elliptical paths around the sun. Orbits may change due to the gravitational effects from, or collisions with, other objects in the solar system. (HS-ESS1-4) ● Cyclical changes in the shape of Earth’s orbit a ...
... ● Kepler’s laws describe common features of the motions of orbiting objects, including their elliptical paths around the sun. Orbits may change due to the gravitational effects from, or collisions with, other objects in the solar system. (HS-ESS1-4) ● Cyclical changes in the shape of Earth’s orbit a ...
Hubblecast 70: Peering around cosmic corners Visual notes 00:00
... 8. This isn’t the only intriguing effect that gravitational lensing can produce. Take these five quasars photographed by Hubble back in 2006. They all look very similar and close together… perhaps a little too similar. In fact, these are not quasar quintuplets, but a single quasar seen five separate ...
... 8. This isn’t the only intriguing effect that gravitational lensing can produce. Take these five quasars photographed by Hubble back in 2006. They all look very similar and close together… perhaps a little too similar. In fact, these are not quasar quintuplets, but a single quasar seen five separate ...
Teacher`s Guide - Discovery Education
... Context: Our sun is one of 100 to 200 billion stars in our Milky Way galaxy. light-year Definition: The distance light travels in one year; about six trillion miles Context: Astronomers use light-years to describe the vast distances in the universe. planet Definition: A low-mass body that orbits a s ...
... Context: Our sun is one of 100 to 200 billion stars in our Milky Way galaxy. light-year Definition: The distance light travels in one year; about six trillion miles Context: Astronomers use light-years to describe the vast distances in the universe. planet Definition: A low-mass body that orbits a s ...
Origin of Elements - Madison Public Schools
... Our galaxy, the Milky Way, contains ~200 billion stars. Outside the Milky Way are billions more galaxies. There is evidence that the universe is expanding, so galaxies are moving farther away from each other. Thermal energy remains constant, so the universe is also cooling down. There is a large bod ...
... Our galaxy, the Milky Way, contains ~200 billion stars. Outside the Milky Way are billions more galaxies. There is evidence that the universe is expanding, so galaxies are moving farther away from each other. Thermal energy remains constant, so the universe is also cooling down. There is a large bod ...
AIM: HOW DO STARS FORM?
... Big Bang Theory explosion from a state? single point about 15 billion years ago. • Matter & energy formed stars & galaxies, which continue to expand outward. ...
... Big Bang Theory explosion from a state? single point about 15 billion years ago. • Matter & energy formed stars & galaxies, which continue to expand outward. ...
A time travel of 14 billion years
... •It occurred right here, nearly 14 billion years ago. • All matter and energy of the Universe were concentrated in a very small space region. •At the beginning temperature was extremely high. Nuclei and atom constituents formed a primordial soup. •Since that moment the Universe expanded and cooled d ...
... •It occurred right here, nearly 14 billion years ago. • All matter and energy of the Universe were concentrated in a very small space region. •At the beginning temperature was extremely high. Nuclei and atom constituents formed a primordial soup. •Since that moment the Universe expanded and cooled d ...
Sky Science Review for Test Part A
... S.O. 6 - Describe seasonal changes in the length of the day and night and in the angle of the Sun above the horizon. Draw the position of the Earth in relation to the Sun in each season. Make sure you include the tilt of the Earth’s axis in each of the diagrams. Label the following: ...
... S.O. 6 - Describe seasonal changes in the length of the day and night and in the angle of the Sun above the horizon. Draw the position of the Earth in relation to the Sun in each season. Make sure you include the tilt of the Earth’s axis in each of the diagrams. Label the following: ...
Solar system
... 3) The singularity: All matter is crammed into a tiny point the size of a proton. 4) Protostars are formed: a dense cloud of gas surrounded by a spinning disk. ...
... 3) The singularity: All matter is crammed into a tiny point the size of a proton. 4) Protostars are formed: a dense cloud of gas surrounded by a spinning disk. ...
Astronomy Review
... began when a dense, hot, supermassive ball violently exploded. 63. Circle the letter of each item that is evidence for the big bang theory. a. Red shift of galaxies b. Supernova explosions c. Cosmic background radiation d. Galactic clusters 64. What are 2 possible ways that universe might end? Expla ...
... began when a dense, hot, supermassive ball violently exploded. 63. Circle the letter of each item that is evidence for the big bang theory. a. Red shift of galaxies b. Supernova explosions c. Cosmic background radiation d. Galactic clusters 64. What are 2 possible ways that universe might end? Expla ...
Volume 20 Number 4 March 2012 - Forsyth Astronomical Society
... clustered together, are so distant that their light has taken 13.1 billion years to reach us. These galaxies are among the brightest galaxies at that early stage of the Universe's history. They are also very young: we are seeing them just 600 million years after the Universe's birth in the Big Bang. ...
... clustered together, are so distant that their light has taken 13.1 billion years to reach us. These galaxies are among the brightest galaxies at that early stage of the Universe's history. They are also very young: we are seeing them just 600 million years after the Universe's birth in the Big Bang. ...
Lecture 33
... If you don't like the Universe, just wait a minute.... :-) • The universe had to expand by more than another order of magnitude in order to cool so that neutrons and protons could combine; before that any that formed were immediately broken apart again by high-energy photons. • Thus, starting at t~ ...
... If you don't like the Universe, just wait a minute.... :-) • The universe had to expand by more than another order of magnitude in order to cool so that neutrons and protons could combine; before that any that formed were immediately broken apart again by high-energy photons. • Thus, starting at t~ ...
The Earth in Space
... stars include: nebula, proto-stars, main sequence, dwarfs, giants, super giants, neutron stars, pulsars, super nova, and black holes. ...
... stars include: nebula, proto-stars, main sequence, dwarfs, giants, super giants, neutron stars, pulsars, super nova, and black holes. ...
Int. Sci. 9 - Universe Powerpoint
... • 2nd largest planet; most visible from Earth • Saturn is composed almost entirely of hydrogen and helium. • Saturn has many rings made of ice. Saturn’s rings are very wide. They extend outward to about 260,000 miles from the surface but are less than 1 mile thick. • Atmosphere is the largest of any ...
... • 2nd largest planet; most visible from Earth • Saturn is composed almost entirely of hydrogen and helium. • Saturn has many rings made of ice. Saturn’s rings are very wide. They extend outward to about 260,000 miles from the surface but are less than 1 mile thick. • Atmosphere is the largest of any ...
6-8 question answers
... The Sun will burn up all of its Hydrogen in the next 5,000 years. FALSE. While the Sun will eventually burn itself out, it will not happen this quickly. In the last 4.6 billion years since the Sun’s birth, it has used up roughly half of its fuel only. There is enough Hydrogen for the Sun to last ano ...
... The Sun will burn up all of its Hydrogen in the next 5,000 years. FALSE. While the Sun will eventually burn itself out, it will not happen this quickly. In the last 4.6 billion years since the Sun’s birth, it has used up roughly half of its fuel only. There is enough Hydrogen for the Sun to last ano ...
No Slide Title
... SSPT program at IRF-K The goal: Study the environment and the solar wind interaction as well as the evolution and dynamics of solar system objects with focus on the inner planets, moons, asteroids, comets, and dust. Development of scientific instrumentation for satellite-based measurements in suppor ...
... SSPT program at IRF-K The goal: Study the environment and the solar wind interaction as well as the evolution and dynamics of solar system objects with focus on the inner planets, moons, asteroids, comets, and dust. Development of scientific instrumentation for satellite-based measurements in suppor ...
Big Bang Quiz
... 4) At the time of the Big Bang and just after a) All the matter and energy of the universe was compressed into a point. b) After a few seconds, protons, neutrons and electrons formed. c) After a few minutes, hydrogen formed. d) All of the above. ...
... 4) At the time of the Big Bang and just after a) All the matter and energy of the universe was compressed into a point. b) After a few seconds, protons, neutrons and electrons formed. c) After a few minutes, hydrogen formed. d) All of the above. ...
Solar nebula theory
... The Sun’s outer core will expand and the Sun will become a Red Giant. Theory #1: The Earth will get engulfed by the Sun and exist no more. Theory #2: When the Sun first begins to shrink, gravitational attraction between the Earth and Sun will become less. Some scientists think the Earth may move awa ...
... The Sun’s outer core will expand and the Sun will become a Red Giant. Theory #1: The Earth will get engulfed by the Sun and exist no more. Theory #2: When the Sun first begins to shrink, gravitational attraction between the Earth and Sun will become less. Some scientists think the Earth may move awa ...
Outer space
Outer space, or just space, is the void that exists between celestial bodies, including the Earth. It is not completely empty, but consists of a hard vacuum containing a low density of particles, predominantly a plasma of hydrogen and helium as well as electromagnetic radiation, magnetic fields, neutrinos, dust and cosmic rays. The baseline temperature, as set by the background radiation from the Big Bang, is 2.7 kelvin (K). Plasma with a number density of less than one hydrogen atom per cubic metre and a temperature of millions of kelvin in the space between galaxies accounts for most of the baryonic (ordinary) matter in outer space; local concentrations have condensed into stars and galaxies. In most galaxies, observations provide evidence that 90% of the mass is in an unknown form, called dark matter, which interacts with other matter through gravitational but not electromagnetic forces. Data indicates that the majority of the mass-energy in the observable Universe is a poorly understood vacuum energy of space which astronomers label dark energy. Intergalactic space takes up most of the volume of the Universe, but even galaxies and star systems consist almost entirely of empty space.There is no firm boundary where space begins. However the Kármán line, at an altitude of 100 km (62 mi) above sea level, is conventionally used as the start of outer space in space treaties and for aerospace records keeping. The framework for international space law was established by the Outer Space Treaty, which was passed by the United Nations in 1967. This treaty precludes any claims of national sovereignty and permits all states to freely explore outer space. Despite the drafting of UN resolutions for the peaceful uses of outer space, anti-satellite weapons have been tested in Earth orbit.Humans began the physical exploration of space during the 20th century with the advent of high-altitude balloon flights, followed by manned rocket launches. Earth orbit was first achieved by Yuri Gagarin of the Soviet Union in 1961 and unmanned spacecraft have since reached all of the known planets in the Solar System. Due to the high cost of getting into space, manned spaceflight has been limited to low Earth orbit and the Moon.Outer space represents a challenging environment for human exploration because of the dual hazards of vacuum and radiation. Microgravity also has a negative effect on human physiology that causes both muscle atrophy and bone loss. In addition to these health and environmental issues, the economic cost of putting objects, including humans, into space is high.