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chapter14 - Empyrean Quest Publishers
chapter14 - Empyrean Quest Publishers

... rise in core temperature led to a rapid rise in fusion energy? A. The core would expand and heat up ...
Stellar Evolution
Stellar Evolution

ASTR 101 Deming EXAM II November 18 OFFICE HRS in CSS
ASTR 101 Deming EXAM II November 18 OFFICE HRS in CSS

... Exoplanets: methods of detection, what are they like? Revision of solar nebula theory Electromagnetic radiation—basic properties of light, wavelength & photon energy gamma rays, x rays, ultraviolet, visible, infrared, radio short wavelength--------------------------->long wavelength great photon ene ...
Midterm II Jeopardy
Midterm II Jeopardy

... $400 - Pluto is now called this. (Dwarf planet) $600 – This is the event that killed the remaining dinosaurs and 2/3 of all life (K-T Extinction) $800 - A novae can result when you have these two objects near each other (WD and other star, red giant) ...
Electromagnetic Radiation
Electromagnetic Radiation

... • Auroras, the result of solar flares, are bright displays of ever-changing light caused by solar radiation interacting with the upper atmosphere in the region of the poles. The Solar Interior  Nuclear Fusion • Nuclear fusion is the way that the sun produces energy. This reaction converts four hydr ...
Star/Sun/Spectral Analysis - ppt
Star/Sun/Spectral Analysis - ppt

... is a magnetic storm which includes a sudden, rapid, and intense variation in brightness. Radiation is emitted across almost the entire electromagnetic spectrum. ...
Equivalent Widths and Chemical abundances Equivalent
Equivalent Widths and Chemical abundances Equivalent

... 5) Also note the relative peak of the “iron peak” elements, Fe and Ni. 6) Note that Iron-56 represents the most stable atom in the sense of the greatest binding energy per nucleon, so it is the dividing point between where nuclear reactions yield energy by fusion and where they yield them by fission ...
I. Layers of the Sun
I. Layers of the Sun

... years. 3. Occur in pairs. 4. When 2 sunspots come together, prominences and flares are produced. ...
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Document

... elements ...
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... The Sun is the nearest star to the Earth. It is made up of very hot gases with the center of the Sun measuring about 15 million °C!!! ...
Lecture 7
Lecture 7

... whole weight of the star! ...
The Sun
The Sun

... produces energy. This reaction converts four hydrogen nuclei into the nucleus of a helium atom, releasing a tremendous amount of energy. ...
The Sun - Hicksville Public Schools
The Sun - Hicksville Public Schools

The Sun - the University of Redlands
The Sun - the University of Redlands

... • Sound waves cross the the solar interior and reflect off of the surface (photosphere). ...
Notes
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HOMEWORK 5 SOLUTIONS CHAPTER 9 4.A A red giant star will
HOMEWORK 5 SOLUTIONS CHAPTER 9 4.A A red giant star will

... The radius of the 0.6 solar mass white dwarf will be slightly larger than the radius of the Earth. The radius of the 1.2 solar mass star will be about half the radius of the Earth. 4.C Since the Earth would not be within the even horizon of the black hole, the Earth’s orbit will not change. Since th ...
Today`s Powerpoint
Today`s Powerpoint

... from the Sun and found it to be lower than expected (by 30-50%) Confirmed in subsequent experiments Theory of p-p fusion well understood Solar interior well understood ...
The Sun Notes File
The Sun Notes File

... Interior of the Sun Three layers Core Radiative Zone—energy is transferred as electromagnetic waves—radiation Convective Zone—energy is transferred through convection ...
Sun_and_HR - CASS, UCSD
Sun_and_HR - CASS, UCSD

... Luminosity: ...
The Sun - Moodle
The Sun - Moodle

Topics on the Sun and the Life
Topics on the Sun and the Life

... • Can not be chemical energy (only last 10,000 years) • Can not be gravitational contraction (only last 25 million years) • Energy from nuclear reaction – Corresponds to a reduction of mass according Einstein’s mass-energy equation: ...
AST1001.ch10
AST1001.ch10

... More recent observations also found a deficit of neutrinos. A new theory of the neutrino predicts that they have mass and can change form. This theory agrees with the observed neutrino numbers. ...
Spectral Classification of Stars
Spectral Classification of Stars

... investigate solar interior is through Helioseismology = analysis of vibration patterns visible on the solar surface: Approx. 10 million wave patterns! ...
ASTRONOMY TEST THE SUN
ASTRONOMY TEST THE SUN

... 1. The _______ is the outward flow of charged particles leaving the sun. 2. The ________ is the outermost, hottest part of the sun. 3. Nuclear fusion takes place only in the sun’s _____________. 4. Absorption lines in the solar spectrum are formed in the ________. 5. Solar energy is produced by the ...
Questions about the Sun:
Questions about the Sun:

... temperature. The classes are: O, B, A, F, G, K, and M; O stars are the hottest; M the coolest. The numbers are simply subdivisions of the major classes. The classes are oddly sequenced because they were assigned long ago before we understood their relationship to temperature. O and B stars are rare ...
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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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