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Lecture 3 notes - Department of Physics and Astronomy
Lecture 3 notes - Department of Physics and Astronomy

... been detected using indirect methods Some binary star systems contain a black hole In such a system, gases captured from the companion star by the black hole emit detectable X ...
Naked-eye astronomy
Naked-eye astronomy

... • It is tilted about 23½° away from the perpendicular & is called the obliquity. • The Earth maintains this tilt as it orbits the Sun, with the Earth’s north pole pointing toward the north celestial pole ...
Astro history 1
Astro history 1

... • With no street lights and no alarm clocks… • The Night sky was a great glowing question… • Who are we? (no answer yet?) • Why are we here (not clear on that one either…?) • Where are we? • Humans have been working on that one for a long time! ...
Hertzsprung-Russell Diagram Astronomy Project Purpose: To
Hertzsprung-Russell Diagram Astronomy Project Purpose: To

... Requirements: For each star that is chosen, the following must be completed along with it. Example: if you work in groups of 3, then you will have three sets of data for each of the stars you chose. 1.) Determine the stars temperature in Celsius and Kelvin 2.) With the provided formula, determine th ...
The Lives of Stars
The Lives of Stars

Stellar Evolution
Stellar Evolution

... • Gravity pulls a nebula’s dust and gas into a denser cloud • As a nebula heats up, it contracts • A contracting cloud of dust with enough mass to form a star ...
E3 STELLAR DISTANCES E4 COSMOLOGY
E3 STELLAR DISTANCES E4 COSMOLOGY

... A main sequence star emits most of its energy at λ = 2.4 x 10-7 m. Its apparent brightness is measure at 4.3 x 10-9 W m-2. How far away is the star? [28 pc] ...
Steve Holmes - KWFN October 22 2012 speaker
Steve Holmes - KWFN October 22 2012 speaker

... Many celestial objects photograph well, but supernovae are among the most breathtaking. A supernova is the end-of-life explosion of a large star. This explosion occurs within a matter of seconds, and appears as a major brightening that fades out over several weeks or months. The event sends out a hi ...
Scale of the Universe in space, time, and motion
Scale of the Universe in space, time, and motion

... neighbor star which could fit in a room, say with a length of 5 m, what would be the diameter of the Sun? Of the Earth? • How long does it take light to travel from the Sun to the Earth? • Find Earth’s rotational speed at the equator from the Earth’s diameter and the length of a day. • Starting at E ...
PowerPoint
PowerPoint

... Basin) Mile-high cliffs (Discovery Scarp) Early shrinkage of crust  no geological activity at present Interior is solid to a significant depth Density comparable to Earth’s, but weak magnetic field - Iron core, few silicates in crust - Cataclysmic impact early in history? ...
A History of Astronomy, Astrophysics and Cosmology
A History of Astronomy, Astrophysics and Cosmology

... the details of the motions of the planets, such as the retrograde motion seen in Figure 1. Ptolemy himself stated that uniform circular motion was the only kind of motion ‘in agreement with the nature of Divine Beings’. Therefore, it was supposed that, in addition to their circular orbits about the ...
constellation - Bucks-Mont Astronomical Association
constellation - Bucks-Mont Astronomical Association

... of background stars. In the infrared, though, the gas glows brilliantly as it forms new stars inside. Combined near-infrared and visible light observations, such as those taken by the Hubble Space Telescope, can reveal the structure of the clouds as well as the young stars inside. In the Chameleon c ...
"WITH THE STARS" i - Royal Astronomical Society of Canada
"WITH THE STARS" i - Royal Astronomical Society of Canada

... nearest star requires more than 4 years for the Sun, Venus receives about twice as much light trip. Most stars seen with the unaided eye and heat as we do. are upwards of 100 "light years" distant, and Next'beyond Earth is Mars. With an average the telescope reveals objects so far off that distance ...
Units
Units

... Discovered April 6 by NASA's Chandra X-ray Observatory, the swirling, 10 million-mile- wide cosmic dust cloud has been likened to an "acid nebula" and is hurtling toward us at close to the speed of light -- making its estimated time of arrival 9:15 a.m. EDT on June 1, 2014. The bad news is that the ...
The Pulsar “Lighthouse”
The Pulsar “Lighthouse”

... • Degenerate pressure of neutrons can support stars only up to 3M • For M > 3M: Further collapse Î black hole • Mass is so concentrated that light cannot escape. • One way to think about it: – vescape = 2GM/R becomes greater than speed of light. – So photons can’t escape. • Black holes now known o ...
Multiple choice test questions 1, Winter Semester
Multiple choice test questions 1, Winter Semester

Theme 5: The Rise of the Telescope:
Theme 5: The Rise of the Telescope:

... Tycho’s observations that the parallax of Mars is actually not more than 1' or 2', so the Sun’s is 1' at most: this was the first real revision of the Greek estimates. (In India around AD 500, Āryabhaṭa estimated 5500 Earth radii, much better though still far too small; but the Indian theories had ...
Study Guide for 1ST Astronomy Exam
Study Guide for 1ST Astronomy Exam

...  Draw and label the celestial sphere for an observer at any latitude,  Draw the apparent motion of stars as seen by any observer looking North, East, South or West at any location in the northern hemisphere.  Define a constellation and distinguish it from an asterism,  Use celestial coordinates ...
angular measure - Empyrean Quest Publishers
angular measure - Empyrean Quest Publishers

... – a collection of ideas that seems to explain a phenomenon  Model – hypotheses that have withstood observational or experimental tests  Theory – a body of related hypotheses can be pieced together into a self consistent description of nature  Laws of Physics – theories that accurately describe th ...
The Night Sky
The Night Sky

... As promised in last month’s article, the world did not end on December 21, 2012. As the year 2013 begins, the earth passes through perihelion on January 2nd, its closest point to the sun in its elliptical orbit. On this date, it is 3% closer to the sun as compared to its farthest point, or aphelion, ...
Sparta High School
Sparta High School

... 5.1 Science Practices: All students will understand that science is both a body of knowledge and an evidence-based, model-building enterprise that continually extends, refines, and revises knowledge. The four Science Practices strands encompass the knowledge and reasoning skills that students must a ...
Astronomy - Troop 179
Astronomy - Troop 179

Lecture 2+3 - University of Texas Astronomy Home Page
Lecture 2+3 - University of Texas Astronomy Home Page

Coordinate System Notes 3 - School District of La Crosse
Coordinate System Notes 3 - School District of La Crosse

... A. Egyptians- divided the sky into rgions conatining distinct star groups. 1. Given names and stories so they wopuld be remembered. B, Constellations are areas which have stars in particular arrangements. 1, No meaning to the arrangement except through imagaination 2. Many are associated with Greek ...
Rosette Nebula - Westchester Amateur Astronomers
Rosette Nebula - Westchester Amateur Astronomers

... Top row, left: H1 strain. Top row, right: L1 strain. GW150914 arrived first at L1 and 6.9 (+0.5/-0.4) ms later at H1; for a visual comparison, the H1 data are also shown, shifted in time by this amount and inverted (to account for the detectors’ relative orientations). Second row: Gravitational-wave ...
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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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