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Motions and Their Effects
Motions and Their Effects

... equator Every part of the Earth experiences equal hours of day and night ...
Xtra_credit_MC_chapt_10−12_2014.txt Xtra_credit_MC_chapt_10
Xtra_credit_MC_chapt_10−12_2014.txt Xtra_credit_MC_chapt_10

General Astronomy - Stockton University
General Astronomy - Stockton University

... One of the more notable ‘computors’ (not shown here since she died in 1911) was Wilhelmina Fleming. Fleming was placed in charge of dozens of women hired to do mathematical classifications and edited the observatory's publications. Fleming moved from Scotland to Boston with her husband, Once there, ...
Micro_lect20a
Micro_lect20a

... + 12.9 MeV ...
Linking Asteroids and Meteorites through Reflectance Spectroscopy
Linking Asteroids and Meteorites through Reflectance Spectroscopy

... • As a planet moves around its orbit, it sweeps out equal areas in equal times. • This means that the planet travels faster when it is nearer the Sun and slower when it is farther from the Sun ...
Final Review Sheet
Final Review Sheet

... lower temperature (by about 1000 K) than their surroundings and have strong magnetic fields (1000 Gauss). They generally come in pairs with opposite magnetic polarity. The sun experiences a 22 year cycle during which its magnetic field goes through one complete reordering of its magnetic field. The ...
Name Origins: Back to the Beginning Video Questions http://www
Name Origins: Back to the Beginning Video Questions http://www

... http://www.pbs.org/wgbh/nova/space/origins-series-overview.html#origins-back-beginning 1. The Big Bang theory has been called the greatest discovery in cosmology. Describe it. ...
Chapter 16, Exercises 51–52, 54
Chapter 16, Exercises 51–52, 54

Lecture 02a: Setting a context for us in the Universe
Lecture 02a: Setting a context for us in the Universe

... Consequences of the Big Bang theory The Universe… … enlarged and cooled with time … started out as pure H and He. … continues to age… The Big Bang theory accurately explains the relative H and He concentrations in the Universe, its clumpiness, age, background radiation, and other things. ...
Notes Chapter 20 - Universe and Stars
Notes Chapter 20 - Universe and Stars

... Lack regular shapes and do not have a well-defined structure ...
HOW WAS THE SOLAR SYSTEM FORMED? Scientists have
HOW WAS THE SOLAR SYSTEM FORMED? Scientists have

... have also learned a lot about how our solar system was formed by studying other astronomical phenomena, like nebulas, that are in different stages of their life cycles. Because of advances in technology, scientists have been able to view other solar systems in their development process. Astronomers ...
H-R Diagrams
H-R Diagrams

... 2 The y-axis - luminosity - doesn’t increase linearly: for equal intervals it increases by the same multiple. This is a logarithmic scale - useful for ...
The Moons of the Giants
The Moons of the Giants

... Jupiter’s Io ...
The Sun
The Sun

... by the magnetic field The basic law of magneto-hydrodynamics: ...
Chapter 1 - Scholastic Shop
Chapter 1 - Scholastic Shop

Astronomy MCAS Questions Multiple Choice 1.) The diagram below
Astronomy MCAS Questions Multiple Choice 1.) The diagram below

... a. Name two types of eclipses that involve the Sun, the Moon, and Earth. b. Identify the phase of the Moon during each type of eclipse you named in part (a). c. Choose one of the types of eclipses that you named in part (a) and describe (or draw a diagram that shows) the relative positions of the Su ...
Life of the Sun—16 Oct
Life of the Sun—16 Oct

... F = area P = R2 MkT/(mR3) =M kT/(mR) In balance ...
Dead Stars - University of Iowa Astrophysics
Dead Stars - University of Iowa Astrophysics

... “Most stars end their lives as white dwarfs. These glowing embers scattered throughout space are a galaxy’s memory of its past glory. Because no fusion occurs in their interiors, white dwarfs simply cool off at an essentially constant radius as they slowly deplete their supply of thermal energy”…Car ...
Dead Stars They do exist! The white dwarf stars
Dead Stars They do exist! The white dwarf stars

Stellar Deaths - Mid
Stellar Deaths - Mid

... 1) formed at about same time 2) are at about the same distance 3) have same chemical composition The ONLY variable property among stars in a cluster is mass! ...
Hot-plate model of stars Test 2 & grades • Public viewing sessions
Hot-plate model of stars Test 2 & grades • Public viewing sessions

... Sirius A is slightly larger than the sun. Sirius B is 100 1 times smaller. The same size as the Earth! Stars come in 3 sizes. ...
What`s That Up In The Sky???
What`s That Up In The Sky???

... known as The Milky Way. p. 167 ...
L3 - QUB Astrophysics Research Centre
L3 - QUB Astrophysics Research Centre

... Minimum mean temperature of a star We have seen that pressure, P, is an important term in the equation of hydrostatic equilibrium and the Virial theorem. We have derived a minimum value for the central pressure (Pc>4.5  108 atmospheres) What physical processes give rise to this pressure – which ar ...
Nuclear Astrophysics
Nuclear Astrophysics

... Energy generation rate per unit mass of material ...
–1– 1. The Luminosity of Protostars We derived in the previous
–1– 1. The Luminosity of Protostars We derived in the previous

< 1 ... 169 170 171 172 173 174 175 176 177 ... 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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