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The lifes of a star
The lifes of a star

... plants; these, however, are not the ones or relevance in stellar processes. The relevant reactions present inside stars go under the name of nuclear fusion. Recall that all atoms are made of a very dense and small nucleus which is positively charged and a bunch of electrons, which are negatively cha ...
Project 4: The HR diagram. Open clusters
Project 4: The HR diagram. Open clusters

... Exercise 2:  Sirius is about twice as massive as the Sun. How much brighter is it with  respect to the Sun? In the HR diagram, where will you find the least massive stars? and  the most massive stars?  If I double the mass of a main sequence star, the luminosity increases by a factor 2  3.5 ~  11.3. ...
Dark Matter Capture in the first stars
Dark Matter Capture in the first stars

... • Star reaches T=10^7K, fusion sets in. • 800 solar mass Pop III star lives a million years, then becomes a Black Hole • Very high mass: can avoid Pair instability SN which arise from 140-260 solar mass stars (and whose chemical imprint is not seen) • Helps explain observed black holes: • (I) in cen ...
Einstein coefficients
Einstein coefficients

050802CWUhighSchoolStudents
050802CWUhighSchoolStudents

... Space and time (spacetime) are curved. Matter causes this curvature – “matter tells space how to curve” “Space tells matter how to move” This looks to us like gravity General relativity predicts 43 arc sec. of perihelion shift for Mercury due to the curvature of spacetime near the sun. ...
revealing star formation processes in the nearby universe
revealing star formation processes in the nearby universe

January 2016 - Newbury Astronomical Society
January 2016 - Newbury Astronomical Society

... As well as being one of the most spectacular and A star like our Sun will fuse Hydrogen into Helium and beautiful constellations, Orion is also very interesting towards the end of its life will begin to fuse some of the because we can see evidence of all the stages of the life Helium. A larger star ...
How do Dichroic Filters work?
How do Dichroic Filters work?

... When the film has a thickness equal to ¼ wavelength, the ray c will be reflected with change of phase, and will therefore add to ray a, increasing the brightness of the reflection. These results also occur when the thickness is multiple of ¼ wavelength. As a general rule, therefore, for a particular ...
Gamma - Ray Observations of Olaf Reimer
Gamma - Ray Observations of Olaf Reimer

... GLAST: Expectations translated into full-scale transient trigger and follow-up program, in place by now. ...
Problems and Solutions
Problems and Solutions

... of this spectrum is very strong. Determine the wavelength of this spectral line. Estimate the accuracy of your measurement. Note: If you happen to know the wavelength of the laser light beforehand you are not allowed to use that value in your computation. Warning. Do not look into the laser beam. Do ...
Formation of the Oort Cloud28 Mar Assignment for Fri •
Formation of the Oort Cloud28 Mar Assignment for Fri •

... a function of its semi‐major axis for different external  perturbers. Dashed curves are for perturbers from the present  galactic environment. Solid curves are for assumed perturbers in an early galactic environment. ...
Review - misshoughton.net
Review - misshoughton.net

... Chap. 10 Review: p.444 – #1-8, 11-15, 18, 20, 24 Chap. 11 Review: p.482 – #1-6, 9, 12, 13, 16-19 Chap. 12 Review: p.518 – #10-14 ...
α Cen A + iodine cell spectrum - Department of Physics and Astronomy
α Cen A + iodine cell spectrum - Department of Physics and Astronomy

... For α Centauri A: habitable zone 1.1 – 1.3 AU (1 from A) For α Centauri B: habitable zone 0.5 – 0.9 AU (0.6 from B) ...
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... that neutronization occurs converting the electrons and protons into neutrons and releasing a blast of neutrinos ...
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Abstract

... manipulate a nucleus by (VUV) laser light for the first time. Apart from exciting fundamental research questions (including the search for temporal variations of fundamental constants), this well-shielded narrow-linewidth transition opens up the possibility to realize a compact solid-state optical t ...
VLT observations of GRS 1915+ 105
VLT observations of GRS 1915+ 105

... 1915+105, this object has been under strong surveillance by several observers at different wavelengths. In spite of this work, the nature of the X-ray binary system in GRS 1915+105 is still a matter of debate. The strong interstellar absorption towards the source, that implies optical extinctions of ...
bbColors
bbColors

... Often times astronomers will want more information about an object than just its luminosity. Indeed, the color of an object can be even more important. To determine colors, astronomers often use color indices, or the differences in magnitudes as measured in different filters. Of particular interest ...
6. Light Scattering, Reflection, and Refraction
6. Light Scattering, Reflection, and Refraction

... composed of particles whose sizes are much smaller than the wavelength of the incident photon, the scattering process is elastic and is called Rayleigh scattering. In this scattering process, the energy (and therefore the wavelength) of the incident photon is conserved and only its direction is chan ...
Chapter 9a Introduction to Quantum Mechanics
Chapter 9a Introduction to Quantum Mechanics

... Planck associated the energy quanta only with the light emission in the cavity walls and Einstein extended them to the absorption of radiation in his explanation of the photoelectric effect. ...
Lecture 2/10 The Sun Ulf Torkelsson 1 The internal structure of the
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... most obvious of these are the sun spots. Sun spots are dark regions with a temperature that is a 1000 K lower than the rest of the photosphere. These sunspots have strong magnetic fields on the order of 0.1 T. The reason that the sun spots are cooler appears to be that the magnetic field is suppress ...
G06_Works
G06_Works

... Disturbances in the comet motion may be caused by different reasons: comet lose mass when approaching the Sun, comet is affected by solar wind and its variation because of the huge size of the comet halo, comet motion is affected by irregular ejection (evaporation and explosion) of the nucleus mass. ...
The Balmer Lines of Hydrogen and Deuterium
The Balmer Lines of Hydrogen and Deuterium

Limits of Resolution: The Rayleigh Criterion
Limits of Resolution: The Rayleigh Criterion

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... (Actually, it took Prof. Einstein 10 years to come up with that!) ...
The Morphology of Galaxy Clusters
The Morphology of Galaxy Clusters

... 109 yr, i.e. less than the Hubble time. At the same time, on the scale of galaxy clusters the components have not yet had a chance to separate during collapse, and a cluster is therefore probably a representative sample of the composition of the larger Universe. In particular, the proportion of dark ...
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Astronomical spectroscopy



Astronomical spectroscopy is the study of astronomy using the techniques of spectroscopy to measure the spectrum of electromagnetic radiation, including visible light, which radiates from stars and other hot celestial objects. Spectroscopy can be used to derive many properties of distant stars and galaxies, such as their chemical composition, temperature, density, mass, distance, luminosity, and relative motion using Doppler shift measurements.
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