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Lecture6
Lecture6

... • As already noted in Section (i), the interstellar matter (ISM) is not uniform, but clumpy. New stars are formed in these clumpy, cool, dense clouds called `dark nebulae’ in or near molecular clouds (cool clouds with CO and H2 molecules). Bursts of protostar formation takes place when these dense r ...
Week8Lecture1
Week8Lecture1

Black Holes & Quasars—18 Nov • Black hole • Quasar Ast 207 F2009
Black Holes & Quasars—18 Nov • Black hole • Quasar Ast 207 F2009

... SgrA* acts like a point. Orbit is consistent with Sgr A* being a black hole. If SgrA* is made of stars, there would be a million stars packed within the size of the solar system. The stars would collide. Therefore Sgr A* is a black hole. ...
Makeup labs will be done this week (requires permission from TA).
Makeup labs will be done this week (requires permission from TA).

... electromagnetic radiation (light). Additional important information will be provided in the “Lab and Discussion Syllabus” given during the first week of lab and discussion. Instructions on how to subscribe to our Listserver, MILKYWAY, will be provided in the first lab. The Discussion/Lab Schedule ca ...
The Sun and Stars 4.1 Energy formation and layers of the Sun 4.2
The Sun and Stars 4.1 Energy formation and layers of the Sun 4.2

... is easy to believe that the light from stars reaches us "instantaneously," like that of a light bulb being turned on, it is only with very distant luminescent objects that we can notice that light takes time to travel. The more distant the star, the longer it will take the light to reach Earth. For ...
Big Bang and Beyond
Big Bang and Beyond

... • Technically, galaxies are not moving away from each other • Reality: space expands – When there are more space between galaxies, they “move” away from each other – Analogy: dots on an expanding balloon ...
R - AMUSE code
R - AMUSE code

... At the surface of the star its not so clear, but we use approximations to allow solution. There is no sharp edge to the star, but for the the Sun ρ(surface)~10-4 kg m-3. Much smaller than mean density ρ(mean)~1.4×103 kg m-3 (which we derived). We know the surface temperature (Teff=5780K) is much sma ...
What is a white dwarf?
What is a white dwarf?

... Shrinkage of White Dwarfs • Quantum mechanics says that electrons in the same place cannot be in the same state • Adding mass to a white dwarf increases its gravity, forcing electrons into a smaller space • In order to avoid being in the same state in the same place some of the electrons need to mo ...
ASTRO-114--Lecture 37-
ASTRO-114--Lecture 37-

... fine. So we have already been discussing stars. That’s one particular star. We’re now gonna talk about the variety of stars because not all stars are identical to the Sun. They may have similar properties but they’re not necessarily identical to the Sun. One of the first things that I want to mentio ...
electromagnetic spectrum and spectroscopy
electromagnetic spectrum and spectroscopy

... • He noticed that a thermometer recorded energy from the Sun`s spectrum even when placed beyond the red end of the visible rainbow. •He called this emission Calorific Rays and it was the first discovery that light had colors invisible to the human eye. •These rays are known today as infrared light. ...
Part 1: If a 10000 K blackbody has a wavelength of peak emission at
Part 1: If a 10000 K blackbody has a wavelength of peak emission at

... Here is an example that got ½ credit – again even though it’s not even close to correct: “You determine the age by looking at the stars around it. Since they are in a stellar cluster they are the same age. The age of the star is 2 times the age of the Sun.” ...
SylTerNav\4Curr\emet
SylTerNav\4Curr\emet

... orbit and the stability of the axis (ignoring precession) and show how it causes the seasons; 7.1.5 state the dates of the solstices and equinoxes; 7.1.6 explain the concept of the earth's axial rotation causing day and night; 7.1.7 explain what causes the varying length of daylight through the year ...
prehistoric constellations on swedish rock
prehistoric constellations on swedish rock

Mass and the Properties of Main Sequence Stars
Mass and the Properties of Main Sequence Stars

... neutrons, and releasing neutrinos and energy at the same time  Supernova explosion. Eventually the neutron degeneracy pressure will balance the gravitational pressure (if the star is not too massive) to form a neutron star. The estimated of the neutron stars are about 10 km in diameter, with a mass ...
Tutor Marked Assignment
Tutor Marked Assignment

... PLEASE FOLLOW THE ABOVE FORMAT STRICTLY TO FACILITATE EVALUATION AND TO AVOID DELAY. 2) Use only foolscap size writing paper (but not of very thin variety) for writing your answers. 3) Leave 4 cm margin on the left, top and bottom of your answer sheet. 4) Your answers should be precise. 5) While sol ...
October 2013 - Skyscrapers, Inc.
October 2013 - Skyscrapers, Inc.

... Comet actually means “long-haired,” and Greek philosopher and scientist Aristotle (384 BC – 322 BC) is the first known person to use it to describe these “hairy stars.” Comets were very often considered bad omens, supposedly foretelling the death of royalty or the onset of some calamity. They seemed ...
30 Doradus - HubbleSOURCE
30 Doradus - HubbleSOURCE

... Where does the energy of the stars come from? The new stars continue to contract because of gravity. The increasing pressure heats the nucleus of the star and makes it shine. If gravity was the only source of energy our Sun would shine for less than 18,000,000 years. There must be another source of ...
Document
Document

... Where does the energy of the stars come from? The new stars continue to contract because of gravity. The increasing pressure heats the nucleus of the star and makes it shine. If gravity was the only source of energy our Sun would shine for less than 18,000,000 years. There must be another source of ...
Spiral Galaxies - Astronomy Centre
Spiral Galaxies - Astronomy Centre

... Due to this large size, Shapley believed our Galaxy to contain the observed nebulae In 1920 the Great Debate took place between Shapley and Heber Curtis, who argued for the island universe hypothesis ...
Lecture 1
Lecture 1

... On large scales, the universe is isotropic and homogeneous. Saying the universe is isotropic means that there are no preferred directions in the universe. Saying the universe is homogeneous means that there are no preferred locations in the universe. Note that homogeneity does not imply isotropy, an ...
Life of the Sun—16 Oct
Life of the Sun—16 Oct

... hydrogen in the center in 5Byr • Center of sun must shrink to get hotter to balance gravity • Sun will become a red giant. Surface expands. • Sun will become a planetary nebula • Sun will become a white dwarf ...
Adrian`s December 2016 Night Sky
Adrian`s December 2016 Night Sky

... On the 17th/18th Comet C/2015V2 Johnson is in a straight line with the two end stars of The Plough. From the end star of The Plough follow along this line towards the bright star Arcturus for 6 degrees (almost the same distance between the end two stars of The Plough) and you will find its locatio ...
Night Sky Observations
Night Sky Observations

... educational institution, usually in the field of Astrophysics, and “get paid each month” for the work they do. Astronomy is one of the oldest sciences. It is also one of the few remaining sciences where the amateur astronomer can make a contribution towards professional research. There are few thing ...
Measuring the Stars pages 813-820
Measuring the Stars pages 813-820

... The twelve houses of the zodiac correspond to the constellation that is just behind the Sun on the day you were born. ...
Time
Time

... tracked it with the annual harvest. These methods were inaccurate. ...
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Timeline of astronomy

Timeline of astronomy around 2300 BC.
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