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observingnebulaeclusters-1
observingnebulaeclusters-1

... "Flying" into the Orion Nebula This animation was produced by Walt Feimer in the Astronomy Visualization Laboratory at the Space Telescope Science Institute. It begins with a "backyard" view of the sky around the constellation Orion (by Skip Westphal, STScI) and a more detailed view of the Orion Neb ...
Star Formation - University of Redlands
Star Formation - University of Redlands

... a. it is hot and things that are hot glow red. b. it is ionized hydrogen which appears red because the brightest emission line is red. c. it is cold and things that are cold appear red. d. it is full of red stars. e. dust between the observer and the region blocks the blue light, but lets the red li ...
December 2010 Clear Skies Newsletter PDF
December 2010 Clear Skies Newsletter PDF

starevolution - Global Change Program
starevolution - Global Change Program

... negligible mass compared to the nucleus. Some atoms can have different numbers of neutrons, called isotopes, but if we change the number of protons we change atomic species. The atomic number of H is 1 and its mass is ~1.67E-24 gram; atomic weight is typically expressed as reference mass, and is sli ...
About SDSS - Astro Projects
About SDSS - Astro Projects

... because these objects are remnants of dead stars and therefore mainly to be found in the disc of the Milky Way. The survey also imaged very few globular clusters as these are spread out around the whole galaxy so that few of them happen to be in a direction directly above the Sun's position in the d ...
01-Syllabus
01-Syllabus

... scores will be posted by your course and ID# on the web. If you feel there’s a mistake on the multiple-choice part of an exam, please see the secretary in the astronomy department office, Fraser 345. Questions about essay questions should be directed to the professor. Environmental theme: This cours ...
29 Jan: Maps of the Sky
29 Jan: Maps of the Sky

... • Method 2: understand the physics of the solar system (later) • New coordinate system is like defining your location on Earth (what are the coordinates for locating a position on Earth?) ...
MULTIPLE CHOICE. Choose the one alternative that best
MULTIPLE CHOICE. Choose the one alternative that best

Distance Measurement
Distance Measurement

... Surveying the Stars ...
SASS_Talk_4_16_08
SASS_Talk_4_16_08

... • Stars and other things outside our solar system have a particular Right Ascension and Declination or RA and DEC (almost constant) • Earth’s Equator, North Pole, and South Pole line up with the Equator and North Pole, and South Pole, of the Celestial Sphere ...
Chapter 18 Notes - Valdosta State University
Chapter 18 Notes - Valdosta State University

... The Sun has an apparent magnitude of -27 because it is so close to us. The closest star other than the Sun is Proxima Centauri, part of a three star system that is about 4.3 light years away from us. When comparing the actual brightness of stars it is necessary to introduce absolute magnitude. This ...
Document
Document

... • Tycho thought he had measured stellar distances, so lack of parallax seemed to rule out an orbiting Earth. • Galileo showed stars must be much farther than Tycho thought—in part by using his telescope to see that the Milky Way is countless individual stars.  If stars were much farther away, then ...
36040345-1 - Space Medicine Association
36040345-1 - Space Medicine Association

... detail we shall first attempt to systematize the entire realm of biological investigation related to astronautics. By definition we tend to think of life today in terms of biological forms already familiar to us on earth. We call this "terrestrial" life, classified according to location, geobiolagy ...
Testing - Chabot College
Testing - Chabot College

... • Tycho thought he had measured stellar distances, so lack of parallax seemed to rule out an orbiting Earth. • Galileo showed stars must be much farther than Tycho thought—in part by using his telescope to see that the Milky Way is countless individual stars.  If stars were much farther away, then ...
Starry Lives, Starry Skies
Starry Lives, Starry Skies

... The handout sheet has examples of objects in each stage, but it would be good for students to use  the Web or some astronomy books to find examples for themselves.  4. Have them make a star map of the location of one object for each stage, using the Your Sky  Tonight  star chart.  Most sky objects a ...
GRAVITY FIELD IN EXTERNAL PARTS OF THE SOLAR SYSTEM
GRAVITY FIELD IN EXTERNAL PARTS OF THE SOLAR SYSTEM

Jul - Wadhurst Astronomical Society
Jul - Wadhurst Astronomical Society

Sep 2012 - Bays Mountain Park
Sep 2012 - Bays Mountain Park

... and our own orbit through the Solar System. By now the Curiosity rover will be starting to move around Gale Crater and make some new observations and discoveries. Be sure to catch the science briefings that come on the NASA-TV web site and are replayed usually about 7:00 or 8:00 p.m. every night. At ...
Deep Space Mystery Note Form 2
Deep Space Mystery Note Form 2

... was Kepler’s Supernova which was first observed in 1604 (also known as Supernova 1604 or Kepler’s Star). Since then no supernova has been indisputably observed in our galaxy, though many outside our galaxy has. The supernova remnant from Kepler’s Star is still studied. A supernova remnant is what is ...
Word format
Word format

... several types of complexity. First among these is chemical complexity. Although most classes of gas-phase reactions are reasonably if not completely understood, processes occurring on dust particles are more complex for a variety of reasons, including small numbers of reactants and poorly characteri ...
Star Planet - Stony Brook Astronomy
Star Planet - Stony Brook Astronomy

... will watch it disperse over the next 10,000 Earth years. B.  In reality, the supernova remnant has already dispersed, but we will watch it disperse over the next 10,000 Earth years. C.  The image of the supernova dispersing will not ...
ASTR 105 Intro Astronomy: The Solar System
ASTR 105 Intro Astronomy: The Solar System

... the material that orbits it, including planets and moons, asteroids and comets, etc ...
Right Ascension and Declination
Right Ascension and Declination

... Right Ascension and Declination Declination and right ascension are coordinates resembling latitude and longitude, but instead of giving the position of location on Earth, they give a position of an object, like a star, on the sphere of the sky. Together, they make up the equatorial coordinate syste ...
Review Powerpoint - Physics and Astronomy
Review Powerpoint - Physics and Astronomy

... 0.5 Science and the Scientific Method • Observation leads to theory explaining it. • Theory leads to predictions consistent with previous observations. • Predictions of new phenomena are observed. If the observations agree with the prediction, more predictions can be made. If not, a new theory can ...
The Genesis of the Elements
The Genesis of the Elements

... All the matter in the universe was packed as elementary particles into a “nucleus”  This exploded!  Dispersed the matter uniformly as neutrons  These neutrons then decayed ...
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Theoretical astronomy

Theoretical astronomy is the use of the analytical models of physics and chemistry to describe astronomical objects and astronomical phenomena.Ptolemy's Almagest, although a brilliant treatise on theoretical astronomy combined with a practical handbook for computation, nevertheless includes many compromises to reconcile discordant observations. Theoretical astronomy is usually assumed to have begun with Johannes Kepler (1571–1630), and Kepler's laws. It is co-equal with observation. The general history of astronomy deals with the history of the descriptive and theoretical astronomy of the Solar System, from the late sixteenth century to the end of the nineteenth century. The major categories of works on the history of modern astronomy include general histories, national and institutional histories, instrumentation, descriptive astronomy, theoretical astronomy, positional astronomy, and astrophysics. Astronomy was early to adopt computational techniques to model stellar and galactic formation and celestial mechanics. From the point of view of theoretical astronomy, not only must the mathematical expression be reasonably accurate but it should preferably exist in a form which is amenable to further mathematical analysis when used in specific problems. Most of theoretical astronomy uses Newtonian theory of gravitation, considering that the effects of general relativity are weak for most celestial objects. The obvious fact is that theoretical astronomy cannot (and does not try) to predict the position, size and temperature of every star in the heavens. Theoretical astronomy by and large has concentrated upon analyzing the apparently complex but periodic motions of celestial objects.
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