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HR Diagram
HR Diagram

... It has been shown through observational data of many stars that the more massive a star, the more luminous it is. If you observe the H-R diagram on the cover of the lab, it is clear that there are fewer luminous stars as compared to the less luminous ones. In terms of the diagram, there are more sta ...
Where do elements come from?
Where do elements come from?

... – O  Ne  Mg  Si  Fe © 2004 Pearson Education Inc., publishing as Addison-Wesley ...
lecture_1_mbu - X-ray and Observational Astronomy Group
lecture_1_mbu - X-ray and Observational Astronomy Group

... Cool, dense clouds suspended above surface by magnetic field. ...
Lecture 1 - X-ray and Observational Astronomy Group
Lecture 1 - X-ray and Observational Astronomy Group

Astronomy Today 7th Edition Chaisson/McMillan
Astronomy Today 7th Edition Chaisson/McMillan

... Now known: Solar system has 166 moons, one star, eight planets (added Uranus and Neptune), eight asteroids, and more than 100 Kuiper belt objects more than 300 km in diameter (smaller asteroids, comets, and meteoroids) ...
Full Poster - Cool Cosmos
Full Poster - Cool Cosmos

... Almost everything that we know about the Universe comes from studying the light that is emitted or reflected by objects in space. Apart from a few exceptions, such as the collection of moon rocks, astronomers must rely on collecting and analyzing the faint light from distant objects in order to stud ...
Gravitational Waves – detectors, sources & science
Gravitational Waves – detectors, sources & science

... • There are many potential sources of gravitational waves for our detectors, ranging from binary star systems to supermassive black hole mergers to cosmic string cusps. • We are on the verge of making our first direct gravitational wave detection. This should happen within 5-10 years, ...
Chapter 6
Chapter 6

... Now known: Solar system has 166 moons, one star, eight planets (added Uranus and Neptune), eight asteroids, and more than 100 Kuiper belt objects more than 300 km in diameter (smaller asteroids, comets, and meteoroids) ...
MSci Astrophysics 210PHY412 - Queen's University Belfast
MSci Astrophysics 210PHY412 - Queen's University Belfast

... • Magnitudes are measured in some wavelength band e.g. UBV. To compare with theory it is more useful to determine bolometric magnitude – defined as absolute magnitude that would be measured by a bolometer sensitive to all wavelengths. We define the bolometric correction to be BC = Mbol – Mv Bolometr ...
PowerPoint Presentation - The Sun as a Power House
PowerPoint Presentation - The Sun as a Power House

... The c2 is the square of the speed of light. 1 gram of matter is equivalent to the energy obtained by burning 15,000 barrels of oil. ...
Page 1 of 4 KEY PSCI 1055 Test #4 (Form A) KEY Spring 2008
Page 1 of 4 KEY PSCI 1055 Test #4 (Form A) KEY Spring 2008

... a. Our Sun is considered to be a class G star. What is the expected temperature range of the Sun? Class G stars are about 5000 K – 6000 K b. What type of star has the lowest temperature but the highest level of brightness on the H-R diagram? giants/supergiants c. A particular star has an absolute ma ...
Archaeoastronomy, Astronomy of Celts, A. Gaspani
Archaeoastronomy, Astronomy of Celts, A. Gaspani

Stars PowerPoint Slides
Stars PowerPoint Slides

Lecture 5/10 The interstellar medium and star formation Ulf
Lecture 5/10 The interstellar medium and star formation Ulf

... recombination of protons and electrons. During the recombination events the electrons cascade down through the energy levels and among other spectral lines they generate the Balmer lines that can be seen in ordinary light. In general these HII regions appear red because of the Balmer-α line. In larg ...
Desert Skies - Tucson Amateur Astronomy Association
Desert Skies - Tucson Amateur Astronomy Association

... bluish. Uranus is unique in that its pole is tipped 98degrees to the ecliptic, so it almost “rolls” along its orbital path. Why this is so isn’t understood. William Herschel discovered Uranus in 1781. In 1846, after John Couch Adams and Urbain Jean Joseph Le Verrier independently calculated where Ne ...
Galaxy Zoo: Pre and post‐workshop information
Galaxy Zoo: Pre and post‐workshop information

... Hubble analysed the light from very distant galaxies and found that their spectra were all redshifted. This Doppler effect whereby wavelengths of spectral lines are affected by the motion of the light source indicates all distant galaxies are receding from us. This was a huge discovery as previously ...
Absolute Magnitude - School
Absolute Magnitude - School

The Early Evolution of the Atmospheres of Earth, Venus, and Mars
The Early Evolution of the Atmospheres of Earth, Venus, and Mars

... The terrestrial planets formed from accretion of materials that partly contained volatiles (Schönbächler et al. 2010). These volatiles were released to form a secondary atmosphere during the formation of Earth (Hashimoto et al. 2007), subsequently during magma ocean solidification (Elkins-Tanton 2 ...
Spectral Classification
Spectral Classification

... How do we Classify and why? ...
The Origin, Structure, and Evolution of the Stars
The Origin, Structure, and Evolution of the Stars

... diagram. Our calculations indicate that the more massive stars “burn” their fuel so rapidly they cannot last very long. Some of these bright stars must have been formed more recently than the earth, perhaps some even as recently as the appearance of early man. By the same arguments, there must have ...
May
May

astrocoursespring2012lec5-1-1
astrocoursespring2012lec5-1-1

... Astronomical Procedure: From Apparent Magnitudes of Variable Stars to their Distances Plot apparent magnitude values from observations at different times results in a light curve for a Cepheid in the Large Magellic Clouds – our closest extragalactic neighbour.Henrietta Leavitt did just that. ...
The Earth in Space and finding where we are.
The Earth in Space and finding where we are.

... • In terms of latitude, 0 is easy to define, it it the line between the north and south poles where the earth's rotational speed is at its maximum • 0 degrees longitude is much more difficult, as all lines of longitude are equally valid as the base line or ‘0’ • The French (of course) wanted 0 to ru ...
Reading the Stars
Reading the Stars

... In order to piece together the story of stellar evolution, you have to have all the data. In this exercise, the focus is on analysis of data, so data will be presented to you and explained to you and you will have to analyze and interpret the data to draw conclusions about stellar evolution. 1. Exam ...
THE HR DIAGRAM
THE HR DIAGRAM

... began to classify stars based on spectral differences, and although these classes were known,  their  significance  was  not.  Remember,  knowledge  about  the  existence  of  other  galaxies,  the  Hubble redshift, quantum mechanics, and the fusion process generating stellar energy came in  the thi ...
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Timeline of astronomy

Timeline of astronomy around 2300 BC.
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