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Video Lesson Information Astronomy: Observations & Theories Astronomy 1
Video Lesson Information Astronomy: Observations & Theories Astronomy 1

... This lesson takes students on a journey from planet Earth to the distant galaxies and superclusters. It is illustrated with stunning computer animation and photographs from NASA, the Jet Propulsion Laboratory (JPL), and astronomical observatories. This journey introduces the planets, stars, and gala ...
The Night Sky - University of Saskatchewan
The Night Sky - University of Saskatchewan

... Students will be able to explain how we see various phases of the Moon at different times, and explain the infrequency of lunar and solar eclipses. Students will remember key aspects of our universe from the Western science cultural point of view. Students will be able to describe how a telescope wo ...
Phases of the Moon: 29.5-day cycle
Phases of the Moon: 29.5-day cycle

... parallax could mean one of two things: 1. Stars are so far away that stellar parallax is too small to notice with the naked eye. 2. Earth does not orbit the Sun; it is the center of the universe. With rare exceptions, such as Aristarchus, the Greeks rejected the correct explanation (1) because they ...
The Stars education kit - Student activities 11-20
The Stars education kit - Student activities 11-20

... Lying between the Southern Cross and the False Cross is the most luminous and massive star in our Milky Way Galaxy – Eta Carinae. It radiates five million times more brightly than the Sun and is about 120 times more massive. It sheds about two Earth masses each day in its stellar wind. If the Sun ga ...
File - South Sevier High School
File - South Sevier High School

eng_gw150914
eng_gw150914

... 3M⊙ (4,62% from the sum of the masses of the two black holes) This gravitational mass defect in about 20 milliseconds (0,02 s) completely switched to energy radiation, including the gravitational waves. Initially, the two black holes are extremely close to each other - at a distance of 350 km (despi ...
Hands-On Lab Activites
Hands-On Lab Activites

... stretching a tape or placing a ruler next to an object to find out how long it is. Direct measurements are made on objects that can be easily handled. If objects are too big or too far away, such as the case with planets and stars, indirect measurements must be made. Parallax is an example of an ind ...
Astro 27 Solar System Formation and ExoPlanets Slide Show
Astro 27 Solar System Formation and ExoPlanets Slide Show

... • Clever astronomers have used a new clue; measure the hydrogen isotope deuterium, whose abundance is directly proportional to ordinary hydrogen. They’ve done this for a young star TW Hydrae, which is only 310M yrs old, and find the disk is much more massive than they had guessed. • Maybe at least m ...
Lec 11 Galileo I Tel..
Lec 11 Galileo I Tel..

...  Venus should be 40 times as large in one position as in another  Venus complete circle = farthest; crescent = closest & largest  Mars should be 60 times as large in one as in another  Thus: naked eye observations do not confirm Copernicanism  Galileo says Copernicus was wise to maintain his vi ...
The Life of the Sun
The Life of the Sun

... Fraser: So even though the Sun is changed to red, it’s now visible from a much further distance than it was before. Pamela: This is part of why so many of the really bright Stars that we see in the Sky are these red Stars. We can just see red Stars at a much greater distance and this is a common pha ...
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... . orbital velocities (due to periodic Doppler shifts) in binaries ...
Planets of Our, and Other, Solar Systems
Planets of Our, and Other, Solar Systems

... • Clever astronomers have used a new clue; measure the hydrogen isotope deuterium, whose abundance is directly proportional to ordinary hydrogen. They’ve done this for a young star TW Hydrae, which is only 310M yrs old, and find the disk is much more massive than they had guessed. • Maybe at least m ...
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STELLAR STRUCTURE AND EVOLUTION

... . orbital velocities (due to periodic Doppler shifts) in binaries ...
The Story of Planet Building
The Story of Planet Building

... The Story of Planet Building Task: Create a book that illustrates the story of how our solar system formed. Guidelines & Expectations ___/2 pts.-Title page that includes a title and your name ___/2 pts.- Minimum of 8 pages ___/6 pts.- Book is in correct chronological order ___/6 pts.- All significan ...
Chapter 1: The Sun - New Hampshire Public Television
Chapter 1: The Sun - New Hampshire Public Television

... joins the combined pair. Instantly, there’s another flash of energy. Like magic the trio has become helium-three. Then, by fusing again with an identical trio, they become - in a flash - helium-four. They emit the two extra hydrogen nuclei - and more energy. The mass of the helium-four nucleus is 0. ...
View/Open - SUNY DSpace
View/Open - SUNY DSpace

... 4.5 billion years ago. The first four planets closest to the sun, Mercury, Venus, Earth and Mars are called the inner planets, also known as the terrestrial planets. They are mostly made up of dirt and rocks. These planets are denser the closer you get to the sun because of the gravitational force. ...
Selected topics in the evolution of low
Selected topics in the evolution of low

... From a physical perspective, the situation immediately reminds one of that which was encountered a few decades ago in the field of stellar pulsation, with a persistent disagreement between computed and observed period ratios of double-mode (or “bump”) Cepheids. Simon [77] realized that the problem c ...
PDF format
PDF format

... parallax could mean one of two things: 1.  Stars are so far away that stellar parallax is too small to notice with the naked eye. 2.  Earth does not orbit the Sun; it is the center of the universe. With rare exceptions such as Aristarchus, the Greeks rejected the correct explanation (1) because they ...
Compilation of a Glossary of International Terms Related to
Compilation of a Glossary of International Terms Related to

Space, Earth and Celestial Objects Test Prep
Space, Earth and Celestial Objects Test Prep

... and moves into a more eccentric orbit that brings it into the inner solar system. This sudden change may be caused by an impact with another asteroid or by the gravitational pull of Jupiter or Mars. The closest known near-Earth collision was in 1994, when asteroid 1994 XL1 came within the Moon’s orb ...
What makes a planet habitable?
What makes a planet habitable?

... 20EUV (4.13 Gyr ago): subsolar obstacle distance 12.7REarth N+ion pick up loss rate ~2 ×1030 s-1 Total loss of nitrogen would result in an equivalent amount of ≤ 20 bar during ~ 50 Myr Simulations indicate that the atmosphere should have been protected more efficiently most likely due to higher carb ...
Pata Picante Simon
Pata Picante Simon

... _____ Explain the process of adiabatic cooling and adiabatic temperature changes to the formation of clouds. ...
CHAPTER 8 Survey of Solar Systems
CHAPTER 8 Survey of Solar Systems

... along a line because their orbits, as well as the Earth’s, all lie in nearly the same plane, as shown in the side view of the Solar System in figure 8.5. Mercury’s orbit has the largest tilt, just 7° from the average of the rest of the planets. The Solar System out to Neptune has about the same rela ...
2nd sem eoypp w 3rd mp highlighted 2016-17 File
2nd sem eoypp w 3rd mp highlighted 2016-17 File

... _____ Explain the process of adiabatic cooling and adiabatic temperature changes to the formation of clouds. ...
Lecture 12
Lecture 12

... The magnitude system • Astronomers quantify the intensity of light produced by a source with the unit magnitudes • Magnitudes are a logarithmic representation of the spectral flux density of a source. – Allows for easy comparison of sources with immense ranges in ...
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Astronomical unit

The astronomical unit (symbol au, AU or ua) is a unit of length, roughly the distance from the Earth to the Sun. However, that distance varies as the Earth orbits the Sun, from a maximum (aphelion) to a minimum (perihelion) and back again once a year. Originally conceived as the average of Earth's aphelion and perihelion, it is now defined as exactly 7011149597870700000♠149597870700 meters (about 150 million kilometers, or 93 million miles). The astronomical unit is used primarily as a convenient yardstick for measuring distances within the Solar System or around other stars. However, it is also a fundamental component in the definition of another unit of astronomical length, the parsec.
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