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Lecture 6 - Stars and Distances
Lecture 6 - Stars and Distances

Modeling Planet Distances
Modeling Planet Distances

chapter5 - Homework Market
chapter5 - Homework Market

... flowing outward from the sun’s interior. • With all that energy radiating into space, the sun’s surface would cool rapidly if energy did not flow up from inside to keep the surface hot. ...
Perspectives of the Earth, Moon and Sun
Perspectives of the Earth, Moon and Sun

Stars as thermonuclear reactors: their fuels and ashes
Stars as thermonuclear reactors: their fuels and ashes

... of the matter of which we are made?”. Our high entropy universe, presumably resulting from the Big Bang, contains many more photons per particle of matter with mass, e.g. electrons, protons and neutrons. Because of the high entropy and the consequent low density of matter (on terrestrial or stellar ...
Main-sequence stage Stellar lifetimes
Main-sequence stage Stellar lifetimes

... Weight (kg) ...
Notes: Stellar Nucleosynthesis
Notes: Stellar Nucleosynthesis

... Fusion of Heavier Elements • Iron is a “star killer” • fusion of iron takes energy (endothermic) instead of giving off energy (exothermic) • therefore, stars begin to “die” once iron is created. ...
Earth Science Regents Basic Review Guide
Earth Science Regents Basic Review Guide

... Nuclear fusion of hydrogen atoms into helium is the source for the sun’s energy. Our solar system is located on one of the outer arms of the Milky Way galaxy. Most celestial objects appear to rise in the east and set in the west because Earth rotates on its axis from west to east (not Polaris and th ...
Folie 1 - astro.uni
Folie 1 - astro.uni

... A „nebula“ (Urnebel), a cloud of dust and meteorites, existed The nebula was flattened by rotation ...
Simulations and radiative diagnostics of turbulence and waves in
Simulations and radiative diagnostics of turbulence and waves in

... • MHD simulations are a great thing • We are able to make a “what if” case and show the observational consequences ...
Space Weather User Needs Related to Solar Observations
Space Weather User Needs Related to Solar Observations

... • Free-space/near-Earth measurements or reliable models of higherenergy (~100-1000MeV) proton/ion spectra. • ACE type data/models on mission termination. • Be able to predict magnitude / duration / characteristics of SPE from information received at onset of event – Corollary: model predictions for ...
4. Sketch and label the life cycle of a star. Give a short phrase
4. Sketch and label the life cycle of a star. Give a short phrase

... Mass – A measure of how much matter an object contains. It is a property of the object and not affected by gravity. Your mass is the same, no matter where you are in the universe! Weight – The resulting force of the gravitational pull on an object. You will weigh less on the moon because there is le ...
red giant
red giant

... • The vast majority of stars in a newly formed star cluster are ________ ? ...
Two-Body Central
Two-Body Central

... • model was no more accurate than Ptolemaic model in predicting planetary positions, because still used perfect circles. ...
A Closer Earth and the Faint Young Sun Paradox
A Closer Earth and the Faint Young Sun Paradox

... Abstract: Given a solar luminosity LAr = 0.75L0 at the beginning of the Archean 3.8 Ga ago, where L0 is the present-day one, if the heliocentric distance, r, of the Earth was rAr = 0.956r0 , the solar irradiance would have been as large as IAr = 0.82I0 . It would have allowed for a liquid ocean on t ...
Blackbody Radiation From Isolated Neptunes The Harvard
Blackbody Radiation From Isolated Neptunes The Harvard

AST 207 Homework 2 Due 17 September 2010
AST 207 Homework 2 Due 17 September 2010

... Alternatively, you can calculate. If the star is on the meridian at sunset, the star is 6h ahead of the sun. That makes the sun’s position R.A. of the star - 6h. The sun is at zero right ascension on Mar. 21. So, convert the sun’s position from R.A. into time and add it to Mar. 21 to find the date. ...
Luminosity and magnitude
Luminosity and magnitude

... • 1 – 6 range spans a factor of 100 in apparent brightness. ( a 1st magnitude star is 100 X brighter than a 6th magnitude star). • The physiology of the human eye dictates that each magnitude change of 1 corresponds to a change of 2.5 in apparent brightness. ...
Review for Midterm—Chapter 1
Review for Midterm—Chapter 1

... • Temperature – relation to the motions of a large collection of particles • Thermal radiation – Relationship between apparent color and temperature – How do we measure temperature of distant objects? • Particle and wave properties of light – Photons: energy per photon – Waves: wavelength, frequency ...
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Section I. SpuItering of ices ASTROPHYSICAL IMPLICATIONS OF
Section I. SpuItering of ices ASTROPHYSICAL IMPLICATIONS OF

... is the modification of the surface layers of the comet due to particle impact on the ice mixtures [14,19-241. Since the particle fluxes are unknown beyond the orbit of Pluto, it is not possible to reliably estimate the irradiation history of comets in the Oort cloud. It is also very difficult to rel ...
The Cosmic Perspective A Modern View of the Universe
The Cosmic Perspective A Modern View of the Universe

... Which is farther, the distance from San Francisco to Los Angeles, or the distance from you to the space shuttle if the shuttle passes ...
Chapter 14
Chapter 14

Oceanic zone
Oceanic zone

...  The surface was still so hot that when water vapor formed clouds, then rain, the rain boiled off again when it hit the ground.  Finally, the Earth cooled enough to allow the rainwater to accumulate and the oceans formed as water vapor condensed. ...
Earth, Sun, and Moon - Uplift North Hills Prep
Earth, Sun, and Moon - Uplift North Hills Prep

... causes it to glow. In this way, sunlight is more similar to a light bulb than to a flame. A tiny piece of metal inside a light bulb is heated using electricity. It becomes so hot that it begins to glow with a bright light. The Sun’s glow works in a similar way. However, instead of electricity it use ...
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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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