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The correct answers are written in bold, italic and underlined. The
The correct answers are written in bold, italic and underlined. The

... 7. The reason the inner planets are mostly rock and iron and the outer planets are mostly lighter material like hydrogen and ices is that • the inner solar system was warm enough that the lighter material vaporized (or never solidified), leaving rock and iron to form the inner planets. • rock and ir ...
THE SUN - University of Mass Lowell, Space Science Laboratory
THE SUN - University of Mass Lowell, Space Science Laboratory

SCI-103 Introductory Astronomy
SCI-103 Introductory Astronomy

... c. Types of Mathematical Problems i. Ratio ii. Proportion iii. V=d/t d. Distribute HW #1 Unit 02: Beyond the Solar System 1) Stellar Evolution A) http://antwrp.gsfc.nasa.gov/apod/image/0808/ngc290_hst_big.jpg B) By the naked eye, almost all stars appear to be white – physiological issue C) Stars wil ...
Round 1 – Physics – multi choice 1) In 1921 Albert Einstein was
Round 1 – Physics – multi choice 1) In 1921 Albert Einstein was

Edexcel GCE - physicsinfo.co.uk
Edexcel GCE - physicsinfo.co.uk

... (ii) When the Sun nears the end of its life it will burn helium in its core for a further 100 million years and become a red giant star. When it has depleted the helium in its core it is estimated that its surface temperature will fall from its present value of 5780 K to 3160 K and its radius will i ...
zenith - Gardner-Webb University
zenith - Gardner-Webb University

... the southern sky at midnight. Virgo is to the east of Leo and Cancer is to the west. One month earlier, which of these constellations was high in the southern sky at midnight? ...
Topic IV: The Solar System & Universe
Topic IV: The Solar System & Universe

... that all matter and energy was concentrated into an area the size of an atom and then it exploded— matter went out in all directions ...
File - Physical Science
File - Physical Science

... enormous amount of energy. This makes stars hot and bright. Nuclear fusion is an atomic reaction that fuels stars. In fusion, many nuclei (the centers of atoms) combine together to make a larger one (which is a different element). The result of this process is the release of a lot of energy. Stars a ...
Iron does not burn.
Iron does not burn.

... parallel) or spin in the direct opposite direction as the proton's spin (i.e., anti-parallel). The energy state of an electron spinning anti-parallel is slightly lower than the energy state of a parallel-spin electron. Remember that the atom always wants to be in the lowest energy state possible, so ...
Formation of the Solar System
Formation of the Solar System

...  Composed primarily of hydrogen and helium, but there must have been some heavier elements, including metals, since we find them in the terrestrial planets for example. This property of the cloud will dictate how the planets ended up in two main types. Think about phases of matter… Elements heavier ...
Name
Name

... imaginary line through Earth that goes from the North Pole to the South Pole. As the Earth rotates only part of the Earth’s surface faces the _______________ at a time. This rotation is what causes ____________ and ______________. One complete rotation takes place every _______________________ (1 da ...
A Simple Planetary Evolution Model Using the Solar Nebular Theory
A Simple Planetary Evolution Model Using the Solar Nebular Theory

The HLCO Project - High Legh Community Observatory
The HLCO Project - High Legh Community Observatory

... found within a comparable environment, that is capable of supporting the full range of interests from the casual observer, to the dedicated ‘professional’ ...
Part 1, Some Basics
Part 1, Some Basics

... temperature) to bottom-right (low luminosity and low surface temperature) – 90% stars in this band – The Sun is one of main sequence stars – Hydrogen burning as energy source ...
Parent Meeting Materials
Parent Meeting Materials

... definitions of important words found in the text. It is usually located at the end of a book. ...
evolution of low
evolution of low

Pre-Main Sequence Evolution
Pre-Main Sequence Evolution

Sun Misconceptions - Florida Solar Energy Center
Sun Misconceptions - Florida Solar Energy Center

–1– 1. Polytropes – Derivation and Solutions of the Lane
–1– 1. Polytropes – Derivation and Solutions of the Lane

plasmas and fusion reactions
plasmas and fusion reactions

A mineral must be inorganic, which means that it contains
A mineral must be inorganic, which means that it contains

... 63. Scientists think the moon was formed when a large object struck Earth, and material from both bodies combined. ...
Kepler`s First Law
Kepler`s First Law

... locations of the celestial poles and celestial equator remains the same ...
Study Guide: Use your notes and handouts to
Study Guide: Use your notes and handouts to

... Saturn is composed of mostly gas, and has a core composed of rock and metallic hydrogen. Rings are probably composed of small particles of ice and rock Uranus. It is covered by a thick layer of gas, and has a fairly uniform blue-green color. Uranus is surrounded by a system of nine rings. Tilted alm ...
Mass-radius Relations for Helium White Dwarfs
Mass-radius Relations for Helium White Dwarfs

... The purpose of this study is to present the effect of neutrino emission at finite temperatures. We considered fully degenerate configuration for WDs with pure helium composition to obtain M-R relation for masses greater than 0.4 M with neutrino emission taken into account as well. In section 2 we d ...
Star Formation and Lifetimes
Star Formation and Lifetimes

... The Sun has a lifetime of approximately 10 billion years. If you could determine the rate of nuclear fusion for a star with twice the mass of the Sun, which of the following would best describe how its fusion rate would compare to the Sun? Circle the best possible response to complete the sentence g ...
< 1 ... 122 123 124 125 126 127 128 129 130 ... 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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