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Solutions to test #2 taken on Monday
Solutions to test #2 taken on Monday

... 2. (13) Millions, Billions or One. This is an “order of magnitude” question. Pick the number (the order of magnitude) that is closest for each. a) ___one_____ Average distance (in parsecs) between stars. b) ____billions____ Current age of the Sun in years. c) ___millions_____ Length of time a star l ...
Part 2
Part 2

Power Point
Power Point

... • The sun is a star with nine planets orbiting around it. • This family of planets is called the solar system. • The planets all travel around the sun in the same direction, and are held in orbit by the gravitational pull of the sun. • The orbits of the planets are slightly elliptical in shape. • Th ...
Document
Document

... • In a matter of just a few minutes they heat material to many millions of degrees and release as much energy as a billion megatons of TNT. ...
Standard Solar Model
Standard Solar Model

Neutrino Physics and Astrophysics with SuperKamiokande Jordan A
Neutrino Physics and Astrophysics with SuperKamiokande Jordan A

...  In 1934 Bethe & Peierls calculated the cross section for neutrino interaction of 10-44 cm2.  Nature (London) 133, 532(1934) “It is therefore absolutely impossible to observe processes of this kind with neutrinos created in nuclear transformations” “… one can conclude that there is no practically ...
astronomy review sheet2
astronomy review sheet2

... 19. How many degrees in its orbit does the Earth move each day? (think about what the shape of our orbit is close to and how many days are in a year) 20. Calculate the eccentricity of the ellipse below: ...
Friday, February 12, 2016 Astronomy in the news?
Friday, February 12, 2016 Astronomy in the news?

... To understand the roles of thermal pressure, charge repulsion, and the strong nuclear force in controlling the way massive stars evolve. ...
12-Sun
12-Sun

... Photosphere -- light sphere The surface in “visible” light T ~ 6500 - 4000 K Depth 100’s kms ...
The Sun as a Star
The Sun as a Star

Physics Projects Brochure (Word Document)
Physics Projects Brochure (Word Document)

... The detector is located underground in the Kamioka mine to provide adequate shielding from cosmic ray events that could interfere with the measurements of rare neutrino interactions. It detects antineutrinos from many of the nuclear power plants located in Japan (antineutrinos are formed during radi ...
Our Sun - Stephen W. Ramsden
Our Sun - Stephen W. Ramsden

... hydrogen fuel, it either stops burning (becoming a dwarf star) or, if it is large enough (so that gravity compresses the helium strongly) it begins burning the helium into heavier elements. Because fusion reactions cease to release energy once elements heavier than iron are involved, the larger star ...
Sun - Dalton Local Schools
Sun - Dalton Local Schools

... When you write a paragraph you need to: 1. Use the correct paragraph shape. 2. Begin with a “2-finger” indent. 3. The 1st line is the only line in a paragraph that is indented. 4. Include 5 to 7 complete sentences. 5. Begin each sentence with a capital. 6. Put a space after each period. (1-finger sp ...
NAME___________ _PERIOD____DATE_____________ 29.3
NAME___________ _PERIOD____DATE_____________ 29.3

... _____1.Stars more massive than the Sun use up their fuel at a slower rate. ...
Sun Test Answers
Sun Test Answers

... 25. This same gaseous soup of charged particles is found in lightning. a) true b) false 26. In the core, protons fuse together and release small packets of heat and light called a) photons b) plasma c) spicules d) positrons 27. This gaseous soup of charged particles is made up of what two elementary ...
The Sun`s Magnetic Field Twisting Magnetic Fields PRS: Sunspots
The Sun`s Magnetic Field Twisting Magnetic Fields PRS: Sunspots

... 1) They repel hydrogen atoms so the nuclear fusion is less intense. 2) They stop convection in the plasma so heat can’t rise through them. 3) They attract iron particles that block the light ...
Solutions for the Homework 8
Solutions for the Homework 8

... you calculate the wavelength of maximum energy, it will red and so this star is called a “red supergiant ”. Problem 7.56: The planet Venus is different from the earth in several respects. First, it is only 70% as far from the sun. Second, its thick clouds reflect 77% of all incident sunlight. Finall ...
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... • But: come up with theory that explains all the features of the Sun and predicts new things • Do more experiments to test predictions • This lends plausibility to theory ...
Space History - Net Start Class
Space History - Net Start Class

... on a bigger circle at different rates and some have backward movements ...
Astronomy 120
Astronomy 120

... 1. Zeilik Study Exercise 13.1 In the winter sky, you see the following stars: Capella (yellowish), Betelgeuse (reddish), and Sirius (bluish). List these stars in order of increasing surface temperature. Estimate the surface temperature of Betelgeuse and of Sirius. 2. Zeilik Study Exercise 13.9 Jupit ...
Chapter 16 The Sun
Chapter 16 The Sun

... foot or so away, but the Sun delivers that energy flux to every square meter of the Earth, and does it from 93 million miles (1AU) away. Total luminosity of the sun is about 4 × 1026 W—the equivalent of 10 billion 1-megaton ...
LAGUNA
LAGUNA

... ~25% of events are due to v’s originating from SN @ z>1! ...
Science 2nd 9 weeks
Science 2nd 9 weeks

... 2016.17 Second Grade Science, Quarter 2 Big Ideas/Key Concepts:  Various forms of energy are constantly being transformed into other types without any net loss of energy from the system.  The cosmos is vast and explored well enough to know its basic structure and operational principles  Everythin ...
Space Science Unit 2 Lesson 2 Worksheet 1. Which of Kepler`s laws
Space Science Unit 2 Lesson 2 Worksheet 1. Which of Kepler`s laws

... 5. What force caused a solar nebula to collapse toward the center, making the center of a star dense and hot? gravity 6. Which diagram below, A or B, will have the greater gravitational force? Why? B, The objects are closer together. ...
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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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