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Lecture notes 11
Lecture notes 11

Comet ISON - Lone Star Science with Mr. Zuber
Comet ISON - Lone Star Science with Mr. Zuber

... Comet C/2012 S1 (ISON) • ISON started its journey towards the Sun (out of the Oort Cloud) a few million years ago • Discovered by Russian astronomers, part of the ISON Project (International Scientific Optical Network) in September 2012. • Comet ISON is a sungrazer, a comet that travels close to th ...
Planet Particulars
Planet Particulars

The Sun's Crowded Delivery Room July 6, 2007
The Sun's Crowded Delivery Room July 6, 2007

... Short-lived isotopes no longer actually exist in meteorites, except for a few produced by cosmic ray interactions. They formed in other stars (and perhaps close to the Sun in our Solar System), were incorporated into solids such as meteorite parent bodies and the planetesimals that accreted to form ...
2006ph607chaptertwo
2006ph607chaptertwo

Lesson 2 Power Notes Outline
Lesson 2 Power Notes Outline

Introduction to Stellar Evolution
Introduction to Stellar Evolution

... Or surface temperature Our Sun: 5,700 deg Kelvin Or about 10,000 F ...
PISGAH Text by Dr. Bob Hayward ASTRONOMICAL Astronomer
PISGAH Text by Dr. Bob Hayward ASTRONOMICAL Astronomer

... identify sections of the sky with the various seasons, e.g., the “spring skies”? It takes the earth one year to revolve around the sun. Obviously, as we orbit our central star, we are on a different side of it each season of the year. Astronomers identify constellations with the seasons in which the ...
Signatures of stellar surface structure
Signatures of stellar surface structure

Chapter 15. The Chandrasekhar Limit, Iron-56 and Core
Chapter 15. The Chandrasekhar Limit, Iron-56 and Core

... Iron core. It cannot go beyond iron, because 56 F e is the most stable atom, in terms of binding energy per nucleon (see slide accompanying the lecture). It represents the dividing point between fission and fusion as sources of nuclear energy. Lighter atoms can be fused together to form more massive ...
View Teacher`s Guide PDF (F.P.O.)
View Teacher`s Guide PDF (F.P.O.)

The Solar System and its Place in the Galaxy
The Solar System and its Place in the Galaxy

AST 207 Final Exam, Answers 15 December 2010
AST 207 Final Exam, Answers 15 December 2010

... billions of years from now. Explain your reasoning. The hotter main-sequence stars have used up their fuel. The main sequence is truncated. 3. About the sun. Write very brief answers. a. (2 pts.) At the present time, how does the sun produce energy? What is used up, and what is created? Hydrogen fus ...
NuSeti-2015 - Department of Physics and Astronomy
NuSeti-2015 - Department of Physics and Astronomy

Solar System in Your Pocket
Solar System in Your Pocket

THE ROTATION OF THE SUN
THE ROTATION OF THE SUN

... move apparently from east to west. Moreover, our planet moves a little less than one degree per day around its complete orbit, so the westward shift would appear quite trivial even on a week basis. It is clear that the displacements we can see are due to the solar rotation itself. Are the spots keep ...
Objectives for grade E - Particle and Astroparticle Physics
Objectives for grade E - Particle and Astroparticle Physics

... Light travels through empty space at a speed of 300,000 km/s • In 1676, Danish astronomer ...
Abstract
Abstract

Greek geocentric model
Greek geocentric model

... The rotation of the Earth accounts for the apparent daily rotation (diurnal motion) of the stars. The apparent annual cycle of movements of the Sun is caused by the Earth revolving round the Sun. The apparent retrograde (backward) motion of the planets is caused by the motion of the Earth around the ...
WIMPs versus MACHOS
WIMPs versus MACHOS

SEPOF_NGSS_OptionalWebinar-6-8_28AUG13_v1
SEPOF_NGSS_OptionalWebinar-6-8_28AUG13_v1

“And God Said, Let There Be Lights in the Firmament of Heaven”
“And God Said, Let There Be Lights in the Firmament of Heaven”

... and others have endured the intense cold on the high plains of antarctica in order to carry out delicate observations of the sun without interruption night and day for several days still others have built large facilities in deep mine caverns for detecting neutrinos the most elusive of all solar rad ...
Time From the Perspective of a Particle Physicist
Time From the Perspective of a Particle Physicist

Layers of the Sun Test 1 study guide. Intoduction to Stars
Layers of the Sun Test 1 study guide. Intoduction to Stars

... Proton-proton cycle 3 steps ...
Lecture 1: Welcome to Astronomy 106
Lecture 1: Welcome to Astronomy 106

... Subtract mass of end product Subtract mass of expanding shell Apply the equation to what is left over ...
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Standard solar model

The standard solar model (SSM) is a mathematical treatment of the Sun as a spherical ball of gas (in varying states of ionisation, with the hydrogen in the deep interior being a completely ionised plasma). This model, technically the spherically symmetric quasi-static model of a star, has stellar structure described by several differential equations derived from basic physical principles. The model is constrained by boundary conditions, namely the luminosity, radius, age and composition of the Sun, which are well determined. The age of the Sun cannot be measured directly; one way to estimate it is from the age of the oldest meteorites, and models of the evolution of the Solar System. The composition in the photosphere of the modern-day Sun, by mass, is 74.9% hydrogen and 23.8% helium. All heavier elements, called metals in astronomy, account for less than 2 percent of the mass. The SSM is used to test the validity of stellar evolution theory. In fact, the only way to determine the two free parameters of the stellar evolution model, the helium abundance and the mixing length parameter (used to model convection in the Sun), are to adjust the SSM to ""fit"" the observed Sun.
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