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Voyage Through the Solar System
Voyage Through the Solar System

ASTR 1020 FINAL EXAM STUDY GUIDE
ASTR 1020 FINAL EXAM STUDY GUIDE

Formation of the Universe
Formation of the Universe

... to and it becomes a white dwarf. After it cools, which takes billions of years, a white dwarf becomes a black dwarf. In larger stars, when fuel runs out and the material contracts a huge explosion occurs. Depending on the size of the star, this explosion is called a nova or supernova. These explosio ...
Earth and Beyond - We can`t sign you in
Earth and Beyond - We can`t sign you in

... The end of the life cycle of really massive stars is different to that of massive stars. After a really massive red giant collapses in a supernova explosion, it leaves a star so dense that not even light can escape its gravitational pull. This is called a black hole! ...
Study Guide for the Final Exam
Study Guide for the Final Exam

... Since fusion is creating such a powerful outward force (radiation pressure), what holds the Sun together? From where - and by what process - is that energy derived that makes fusion possible? What is the importance and probability of the "proton-proton chain?" Why does this complete reaction only oc ...
Lecture 2
Lecture 2

... Further evidence comes from the amounts of Helium and Lithium in the universe, which are well predicted by Big Bang theory, and the large-scale structure of the universe. Large simulations of how a universe would evolve if it started with a Big Bang give results that look very much like what is obse ...
The Exact Solution of Nonlinear Stress
The Exact Solution of Nonlinear Stress

... As the sun rotates, the convection zone spins faster at the equator than it does at the poles. Beneath the convection zone, the radiation zone spins as a solid mass. The different way that these two zones move causes the sun’s magnetic field to stretch at the equator. As the solar cycle continues. t ...
N j
N j

... Often only a relatively small number of sources of a given class are detected in Xray surveys, requiring careful handling of the statistics. We previously addressed this issue in the case of the luminosity function of normal/starburst galaxies in the GOODS area by fitting the luminosity functions us ...
Solar Images Taken with Calcium K
Solar Images Taken with Calcium K

Understanding the stability of stars by means of thought experiments
Understanding the stability of stars by means of thought experiments

... production rate deviates toward lower values, the temperature will increase and thc reaction rate will again be corrected. When consulting a typical textbook about astrophysics, one gets the impression that it is not easy to understand this ...
Lesson Planner Beyond our solar system.indd
Lesson Planner Beyond our solar system.indd

Earth in Space
Earth in Space

... because the Earth is tilted on its axis. The Sun can be observed directly overhead at the equator (and 23.5 degrees below and 23.5 above the equator). The Sun’s angle of separation is less than 90 degrees in the northern hemisphere. ...
The Solar System
The Solar System

... Mercury has a greater temperature range than any of the other planets. A day on Venus is longer than its year. The reddish tinge on Mars is caused by the breakdown of iron-rich ...
Scavenger Hunt: Who am I
Scavenger Hunt: Who am I

... _____________________ 2. We discovered the relationship between a star’s temperature and its brightness. _____________________ _____________________ 3. I discovered Pluto. _____________________ 4. My theory of the universe was held as law for thousands of years even though I was wrong. _____________ ...
1.3. Basic Principles of Nuclear Physics
1.3. Basic Principles of Nuclear Physics

BIL3: YILDIZ
BIL3: YILDIZ

... the central regions of stars are primarily determined by total mass of the overlying layers and its distribution. These physical conditions give the luminosity. Radius depends on radiation field ...
Lecture14-ASTA01
Lecture14-ASTA01

... asteroids, not in comets, which contradicts the importance of the ice line to inner-vs-outer planet division • Other reasons for relative unimportance of ice line are: • Migration and thus mixing of solids in the solar nebula • Roughly 1:1 mass ratio of ice and rock in comets – not important enough ...
Science OGT Review e..
Science OGT Review e..

... years ago Galaxies are moving away from central location Red-shift- the light most galaxies gives off is close to the red end of the spectrum because energy weakens as it is stretched out. Stars moving toward us will shift to the blue end of the spectrum ...
April 2017 - Newbury Astronomical Society
April 2017 - Newbury Astronomical Society

my brief profile
my brief profile

Source of zodiac glow identified ground vehicles
Source of zodiac glow identified ground vehicles

... The eerie glow that straddles the nighttime zodiac in the eastern sky is no longer a mystery. First explained by Joshua Childrey in 1661 as sunlight scattered in our direction by dust particles in the solar system, the source of that dust was long debated. In a paper to appear in the April 20 issue ...
ASTRONOMY 301 PROBLEM SET NUMBER 3 DUE IN CLASS
ASTRONOMY 301 PROBLEM SET NUMBER 3 DUE IN CLASS

... Read these instructions first. Print your name on each page of your answer sheets and staple them together. It is important to show the reasoning you used to solve the problem and any formulae you used and algebraic manipulation that you did. You are encouraged to work together to figure out the met ...
Lecture06-ASTA01 - University of Toronto
Lecture06-ASTA01 - University of Toronto

... • A sidereal year is the time taken for a complete orbit relative to the stars • the time between successive spring (or autumnal) equinoxes is called a tropical year (or solar year) and it should come as no surprise that these two years differ. ...
Pre-supernova evolution of massive stars
Pre-supernova evolution of massive stars

Axions and White Dwarfs
Axions and White Dwarfs

< 1 ... 91 92 93 94 95 96 97 98 99 ... 237 >

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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