• Study Resource
  • Explore
    • Arts & Humanities
    • Business
    • Engineering & Technology
    • Foreign Language
    • History
    • Math
    • Science
    • Social Science

    Top subcategories

    • Advanced Math
    • Algebra
    • Basic Math
    • Calculus
    • Geometry
    • Linear Algebra
    • Pre-Algebra
    • Pre-Calculus
    • Statistics And Probability
    • Trigonometry
    • other →

    Top subcategories

    • Astronomy
    • Astrophysics
    • Biology
    • Chemistry
    • Earth Science
    • Environmental Science
    • Health Science
    • Physics
    • other →

    Top subcategories

    • Anthropology
    • Law
    • Political Science
    • Psychology
    • Sociology
    • other →

    Top subcategories

    • Accounting
    • Economics
    • Finance
    • Management
    • other →

    Top subcategories

    • Aerospace Engineering
    • Bioengineering
    • Chemical Engineering
    • Civil Engineering
    • Computer Science
    • Electrical Engineering
    • Industrial Engineering
    • Mechanical Engineering
    • Web Design
    • other →

    Top subcategories

    • Architecture
    • Communications
    • English
    • Gender Studies
    • Music
    • Performing Arts
    • Philosophy
    • Religious Studies
    • Writing
    • other →

    Top subcategories

    • Ancient History
    • European History
    • US History
    • World History
    • other →

    Top subcategories

    • Croatian
    • Czech
    • Finnish
    • Greek
    • Hindi
    • Japanese
    • Korean
    • Persian
    • Swedish
    • Turkish
    • other →
 
Profile Documents Logout
Upload
The Sun
The Sun

... viewing the Sun from a distant star.  In addition, the Sun is not a solid body like the Earth, and unlike the Earth it’s made up of hot gas, and therefore it exhibits differential rotation. That means that the rotation period can vary with latitude and depth.In the photosphere, it varies from 25 da ...
The Sun
The Sun

... viewing the Sun from a distant star.  In addition, the Sun is not a solid body like the Earth, and unlike the Earth it’s made up of hot gas, and therefore it exhibits differential rotation. That means that the rotation period can vary with latitude and depth.In the photosphere, it varies from 25 da ...
The Solar System…
The Solar System…

... smaller, rocky planets that are closer? • How do we have an estimate of our solar system’s age? • What makes something a dwarf planet? The IAU says it is a celestial body orbiting the Sun a) massive enough to be rounded by its own gravity b) has not cleared its orbit of planetesimals. ...
Study Guide Solar Systems
Study Guide Solar Systems

... outer layers are gases and have liquid interiors •All of the outer planets have lots of moons, as well as planetary rings made of dust and other particles ...
The Formation of Our Solar System
The Formation of Our Solar System

... • Centuries ago, most people thought Earth was the center of the solar system, not the sun. This theory is called the geocentric theory. • The idea that the sun is the center of the solar system is called the heliocentric theory. • Copernicus was an astronomer. He suggested that the sun, not Earth, ...
Asteroids, Meteoroids and Comets
Asteroids, Meteoroids and Comets

File
File

What tool do astronomers use to understand the evolution of stars?
What tool do astronomers use to understand the evolution of stars?

... t B M B L A 1 300 300 60 Sun's lifetime ~ 10 billion years = 1010 yr = 10 Gyr. Lifetime of 5 solar mass star is 1010 yr/60 ~ 1010/102 yr = 108 yr = 102106 yr = 100 million yr = 100 Myr This is the age of the star cluster. ...
lec1_2008 - Stanford Solar Physics
lec1_2008 - Stanford Solar Physics

... Grades: bi- weekly assessments + presentations ...
Fizix Chapter 7 Notes.cwk
Fizix Chapter 7 Notes.cwk

... slow as they are more distant. The second law goes further: If one draws a line from the sun to a planet at two different points in its orbit and repeat this at two other points in the orbit, then if the the time between the two points are equal the area “swept out” are equal. ...
CALIFORNIA WRITING STANDARDS
CALIFORNIA WRITING STANDARDS

... 2. The Earth and other planets move through space in two ways: rotation on an axis and revolution around the sun. Earth’s tilt causes seasonal differences in the height of the perceived path of the sun and the number of hours of sunlight. Seasons are not related to a change in distance between the E ...
PP and CNO-Cycle Nucleosynthesis
PP and CNO-Cycle Nucleosynthesis

... K. This is consistent with the observed (and theoretical) core temperature of the sun. Another factor that may affect barrier penetration is electron screening, which is intuitively conceptualized as a ‘decrease’ in Coulombic repulsion due to the background ‘sea’ of electrons present in high-tempera ...
A generic relation between baryonic and radiative energy densities
A generic relation between baryonic and radiative energy densities

... λ = (nσ )−1 , ...
The Solar System
The Solar System

SolarDermatology
SolarDermatology

... Spicules: jets of hot material seen in the chromosphere, flowing 20 km/sec from the ...
Why can the sun persistently produce energy for the stable output of
Why can the sun persistently produce energy for the stable output of

... The sun is a huge volume of gas and its total mass is very great. As a result of gravitational force, the pressure will be greater when it is closer to the center of the sun. Therefore, the solar core is a highly compressed region in which nuclear fusion can occur under the high­density, high­ tempe ...
here - Atomki
here - Atomki

ppt document - FacStaff Home Page for CBU
ppt document - FacStaff Home Page for CBU

... c-2) Nuclear fusion. This energy comes from combining light elements into slightly heavier elements (like hydogen into helium, or helium into carbon). This is the source of the extra energy in a hydrogen bomb. We do NOT have any fusion reactors, but we are working on them. The main problem is that i ...
ASTRONOMY 220C ADVANCED STAGES OF
ASTRONOMY 220C ADVANCED STAGES OF

Key Facts
Key Facts

... hydrogen and helium undergoing nuclear fusion at very high temperatures, hence producing vast quantities of energy in the form of heat and light. ...
Document
Document

... moon, the asteroid belt, comets, meteoroids, and interplanetary dust and gas. Our solar system has an elliptical shape and is part of a galaxy known as the Milky Way. The Sun is the center of the solar system. It contains 99.8% of all of the mass in our solar system. Consequently, it exerts a tremen ...
Solar System Distance Model - www .alexandria .k12 .mn .us
Solar System Distance Model - www .alexandria .k12 .mn .us

... -Correct portrayal & details of the planets (moons, rings, spots, rotational orientations). ...
大爆炸---宇宙的起源
大爆炸---宇宙的起源

... body thermal energy coming from all parts of the sky. The radiation is isotropic to roughly one part in 100,000. As the universe expanded, adiabatic cooling caused the plasma to lose energy until it became favorable for electrons to combine with protons, forming hydrogen atoms. This recombination ev ...
PHYSICS 015
PHYSICS 015

... As in the p-p cycle, the fusion takes place in a series of steps. The net result is that helium nuclei are converted principally to carbon (also oxygen), with a net release of energy. ...
Where Are We Going?
Where Are We Going?

< 1 ... 154 155 156 157 158 159 160 161 162 ... 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.
  • studyres.com © 2025
  • DMCA
  • Privacy
  • Terms
  • Report