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Planets & Stars
Planets & Stars

... A star’s brightness depends on its size and how hot it is. Larger and hotter stars are brighter than smaller and cooler stars. Brighter stars send out more light energy. A dim star that is close to Earth can appear brighter than a more distant star that is actually very bright. ...
Atomic Physics Explaining the Universe
Atomic Physics Explaining the Universe

... some cases, line width limits show that the turbulent support for clusters is < 13% of that needed (Sanders et al. 2010). So any heat input is relatively ‘gentle.’ ...
3_Ocean126_2006
3_Ocean126_2006

...  Darwin - really old based on time for natural selection (biological argument)  Hutton – really old based on uniformitarianism (processes in the past taking place at rates comparable to today) (geological argument) ...
Today The Sun Events
Today The Sun Events

... could not explain how the Sun could sustain its luminosity for more than about 25 million years. – The Sun shines because gravitational equilibrium keeps its core hot and dense enough to release energy through nuclear fusion. • Hydrogen fuses into Helium in a 3-step process called the proton-proton ...
Applicability of Polytropes The four equations of stellar structure
Applicability of Polytropes The four equations of stellar structure

Stars presentation by lauren
Stars presentation by lauren

Intro Astro PP
Intro Astro PP

... • His systematic method was to name a star by using a letter or number followed by the Latin name of the constellation. ...
The Transient Radio Sky Astrophysical and Artificial
The Transient Radio Sky Astrophysical and Artificial

... Goal 2: Dark energy – Baryon oscillations (Blake) •Standard (comoving) rod, S, fixed by sound horizon (acoustic oscillations) at recombination – measured as acoustic peaks in CMB fluctuations •Follow evolution of S down to lower redshift through source clustering  measure angular diameter distance ...
A breath of oxygen for the Sun
A breath of oxygen for the Sun

Homework
Homework

... claim people are made of stardust. What does this mean? Pick the answer that best matches what you think “being made of stardust” means. a. “Being made of stardust” is not intended to be taken literally. It means that nobody really knows where atoms come from, and more than we know what “stardust” i ...
Shemansky-Saturn upper atmosphere structure
Shemansky-Saturn upper atmosphere structure

... opacity removes measureable flux from the stellar or solar source. ...
Document
Document

30-1 Directed Reading
30-1 Directed Reading

Directed Reading Section: Characteristics of Stars
Directed Reading Section: Characteristics of Stars

... _____ 20. What two kinds of motion are associated with stars? a. inferred motion and actual motion b. actual motion and apparent motion c. actual motion and imagined motion d. inferred motion and apparent motion _____ 21. What causes the apparent motion of the stars, which we can see with the unaide ...
Determination of Latitude
Determination of Latitude

... can be done any time of the day. The true azimuth of the sun is calculated using a sight reduction form, and compared to the measured value of true azimuth. – Calculations are more involved since a complete sight reduction is required. ...
Kepler`s First Law
Kepler`s First Law

... used to describe the motion of stars around black holes. QuickTime™ and a • The study of the motion of the GIF decompressor are needed to see this picture. nearby stars can be used to determine the mass of the black hole. • A good example is the determination of the mass of the black hole at the cen ...
New findings show magnetic organization of the Sun
New findings show magnetic organization of the Sun

m 1
m 1

... composition of outer layers (if line present, element present ...
Does the Sun contribute to Climate Change
Does the Sun contribute to Climate Change

Chapter 13 Practice Questions
Chapter 13 Practice Questions

... excess energy and therefore will not produce the additional gas pressure to halt the collapse. D) Iron nuclei are so large that they occupy all remaining space and so the collapse ...
Name: Period: ______ Date: Fission and Fusion Simulations Fission
Name: Period: ______ Date: Fission and Fusion Simulations Fission

... Fusion Go back to this page and watch the video about fusion http://www.atomicarchive.com/Movies/ 20. What particles and how many of each does the reaction start with? ...
Comets and asteroids
Comets and asteroids

... Asteroids - rocky or metallic objects orbiting the Sun; smaller than a planet and show no evidence of an atmosphere or of other types of activity.  Mostly found in the broad space between Mars and Jupiter  Too small to be seen without a telescope  First of them discovered at the beginning of 19 t ...
It`s time to eat humble pie: latest evidence gives humans a
It`s time to eat humble pie: latest evidence gives humans a

... least one Moon, except for which two? 3. How many satellites have been destroyed by a meteor? 4. Which planet boasts the largest known volcano in our solar system? 5. What does DEWHA, the acronym for an Australian Government department, stand for? ...
Why didn`t Copernicus`s model accurately predict
Why didn`t Copernicus`s model accurately predict

... “lap” another planet (or when Mercury or Venus laps us) • But very difficult to explain if you think that Earth is the center of the universe! • In fact, ancients considered but rejected the correct explanation ...
the link to the powerpoint for Monday
the link to the powerpoint for Monday

... the 1st detector 10 cm away from light bulb, how far away do you put the second detector to get one half the detection? ...
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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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