• 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
Name
Name

... cooler gas is in front of the source of a continuous spectrum. The cooler gas absorbs light energy from the parts of the spectrum where, if heated, it would emit bright lines. The spectrum is broken by dark spaces, which are determined by the number and kinds of gases through which it passes. The da ...
Morphological characteristics of OB spectra and environments
Morphological characteristics of OB spectra and environments

... λλ4647–4650–4652 emission lines comparable to N III λλ4634–4640–4642, they showed evidence of circumstellar activity in terms of sharp absorption features and P Cygni profiles at H and He I lines. During the past decade, all three have been shown to be extreme, periodic spectrum variables, and soon ...
Grade 8 Earth/Space Pretest
Grade 8 Earth/Space Pretest

... About 1.2 billion km The Sun and the nearest star About 40 trillion km Earth’s surface and an orbiting satellite About 400 km The distance between which two objects or places would best be measured in light years? A. Boston and Los Angeles B. Our Sun and the nearest star C. Earth’s maximum distance ...
Grade 8 Earth/Space Pretest Select the best answer to each
Grade 8 Earth/Space Pretest Select the best answer to each

... About 1.2 billion km The Sun and the nearest star About 40 trillion km Earth’s surface and an orbiting satellite About 400 km The distance between which two objects or places would best be measured in light years? A. Boston and Los Angeles B. Our Sun and the nearest star C. Earth’s maximum distance ...
PDF Format
PDF Format

... Chapter 3 Upon its publication in 1543, the Copernican model was ...
Progenitors and Hydrodynamics of Type II and lb Supernovae
Progenitors and Hydrodynamics of Type II and lb Supernovae

The End of the Dark Ages
The End of the Dark Ages

... stages (100 Myr after the source turn on) of the I-front evolution for a Larson (upper panel) and a Salpeter (bottom) IMF. The source stellar mass and other properties of the simulations are the same as those discussed above. For a Salpeter IMF, the volume of the ionized region is smaller by a facto ...
Chapter 4 On the possibility of a helium white dwarf donor in the
Chapter 4 On the possibility of a helium white dwarf donor in the

Spinning Globe
Spinning Globe

... 1. Introduce the activity with the following Motivation / Challenge: “A second grader came to one of my third graders last year and asked, ‘This weekend on Saturday at noon or 12 o’clock, right around lunchtime, I was watching the news and they said they were ‘Live” from Beijing, China and it was mi ...
Chapter 2 Basic Assumptions, Theorems, and Polytropes
Chapter 2 Basic Assumptions, Theorems, and Polytropes

Spinning Globe
Spinning Globe

Excitation of soft dipole modes in electron scattering
Excitation of soft dipole modes in electron scattering

Full Text - Harvard University
Full Text - Harvard University

... (Goody and Yung 1989; Wordsworth et al. 2010a). High-resolution line absorption data for input to the correlated-k model was produced using the open-source software kspectrum and the HITRAN line database (Rothman et al. 2009; Rothman et al. 2010). CO2 collision-induced absorption was included using ...
Frontiers in Neutrino Astrophysics
Frontiers in Neutrino Astrophysics

... The Impossible Dream of Neutrino Astronomy “If [there are no new forces] -- one can conclude that there is no practically possible way of observing the neutrino.” Bethe and Peierls, Nature (1934) “Only neutrinos, with their extremely small interaction cross sections, can enable us to see into the i ...
Simulation of horizontal еlectromagnetic showers in the аtmosphere
Simulation of horizontal еlectromagnetic showers in the аtmosphere

2016October StarStuff - Ford Amateur Astronomy Club
2016October StarStuff - Ford Amateur Astronomy Club

The highest resolution near infrared spectrum of the imaged
The highest resolution near infrared spectrum of the imaged

... The final steps applied to the data cube involved sky subtraction, combining the offset positions, radial subtraction of the host object, and tracing the path of the companion spectrum through the data cube. The targets were observed at different positions on the array in an ABBA pattern sampling two ...
Accretion models
Accretion models

... •Most flux at line center comes from regions where matter is lifted from the disk (larger volume,v~0) . •The wings come from material approaching to the stellar surface (line width~free-fall velocity at the stellar surface) • An acccretion shock is formed, emitting at much higher T than the stellar ...
Document
Document

... This theory states that the universe has always existed as it does now and hasn’t changed. The trouble is that the night sky would be completely lit up because of the billions of stars, but it’s not, so… The “Big Bang” theory This theory states that the universe started off with an explosion and eve ...
(2004) - H. Peter
(2004) - H. Peter

... higher “filling-factor” than Sun?  not enough space on the surface  and: also stellar X-rays are structured stellar corona are not only brighter, they have also  high densities  high temperatures ...
Solar Changes and the Climate
Solar Changes and the Climate

... over cooler sunspots with the result that the irradiance emitted by the sun and received by the earth is higher during active solar periods than during quiet solar periods. The amount of change of the solar irradiance based on satellite measurements since 1978 during the course of the 11 year cycle ...
The evolution of the Sun`s birth cluster and the search for the solar
The evolution of the Sun`s birth cluster and the search for the solar

Peak Bagging of red giant stars observed by Kepler: first results with
Peak Bagging of red giant stars observed by Kepler: first results with

... The discovery of so-called mixed modes [1] has led to a significant improvement in our understanding of the internal structure and evolution of RGs. In particular, the characteristic spacing in period of mixed modes frequencies provides a direct way to disentangle H-shell and He-core burning RGs [2, ...
MASSACHUSETTS INSTITUTE OF TECHNOLOGY Physics Department Physics 8.286: The Early Universe
MASSACHUSETTS INSTITUTE OF TECHNOLOGY Physics Department Physics 8.286: The Early Universe

... Hubble introduced a classification system for galactic shapes, dividing them into elliptical and spiral galaxies of certain visible characteristics. However, this “tuning fork” diagram is not an evolutionary sequence. Instead, a galaxy’s type is mainly determined by its star formation rate: elliptic ...
Globular Clusters - University of Dayton
Globular Clusters - University of Dayton

... Turn Off - As the hydrogen fuel in a star's core runs out the core begins to collapse due to gravity and the star moves away from the main sequence. At the turn off nearly all the central fuel is gone. Red Giant Branch - When the central fuel is gone, hydrogen starts to burn in an envelope around a ...
< 1 ... 42 43 44 45 46 47 48 49 50 ... 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