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2.5.2 development of a star
2.5.2 development of a star

...  In the star it is known as hydrostatic equilibrium. ...
protostars and pre-main
protostars and pre-main

End of the line for a star like ours
End of the line for a star like ours

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The Electromagnetic Spectrum
The Electromagnetic Spectrum

... charged gases can travel far beyond the Sun…solar wind. ...
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SDO | SOLAR DYNAMICS OBSERVATORY HTTP://WWW.NASA

... solid, different regions rotate at different rates: about 24 Earth days at the equator & 30 days at the poles. ...
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The Melbourne Solar System Trail

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... Notation: =0 means solar abundance. [ ] denotes logarithmic ratio. At very early times, [Fe/H]=negative (e.g. =-1.5) since the heavy elements have not be created yet, Type II Supernovae occur at earlier times. They produce both O and Fe and so [O/Fe] is zero. At later times, Type I Supernovae make m ...
A-105 Homework 1
A-105 Homework 1

... 19. (1 pt.) If a star the size of the sun collapses to form a white dwarf the size of Earth, by what factor will its density increase? (The volume of a sphere is 43  r 3 . See Appendix A for the radii of the sun and Earth.) ...
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... Problem 1 (20 points): Our sun is located about 8.5 kpc = 2.6×1020 m from the center of our galaxy, where most of the galactic mass (about 7×1011 solar masses) is concentrated. Assuming the sun executes circular orbits about the galactic center, how long does it take to make a round trip? ...
EARTH & SPACE SCIENCE
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... hydrogen in the sun is always a helium nucleus. The helium nucleus has about 0.7% less mass than the hydrogen nuclei that combined to form it do. The lost mass is converted into energy during the series of fusion reactions that forms helium. The energy released during the three steps of nuclear fusi ...
History of Astronomy
History of Astronomy

...  observed the phases of Venus and the moons of Jupiter. Both observations supported the heliocentric model. ...
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The Solar System - Georgia Standards

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Ancient Astronomy

... -Invented Simple solar calendar- 365 days; 12 months of 30 days (month 3 weeks of 10 days) -aligned pyramids/Tombs with star alignments -astronomers calculated time of flood; around summer solstice -5 constellations -36 groups of stars called decans -Nabta Stone Circle (only stone circle in Egypt) - ...
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... P=nkT where n= the number of atoms/volume, k=Boltzman's constant T=temperature. As 4 protons -> 1 helium, n decreases ...
Chapter Six Science: The Solar System and Beyond Study Guide
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... -Main-Sequence Stars-when a protostar reaches a temperature of several million degrees a nuclear reaction occurs; protostar now becomes a main-sequence star that is fusing hydrogen into helium; where it spends most of its life on the main sequence. -Giants and Supergiants-when a star uses up the sup ...
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Our Solar System
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... Wow, there is just too much to say about Earth, I don’t know where to begin. For starters, Earth is the only planet that has Reese’s peanut butter cups! It is also the only planet that can support life . This is because we are the PERFECT spot, if we were any closer to the sun, all the water would ...
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Astronomy lab: Planets

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... • Sun shows an 11-year sunspot cycle. • Solar maximum: the most sunspots, other activity. • In alternate cycles, the direction of the Sun’s ...
MAJOR NUCLEAR BURNING STAGES The Coulomb barrier is
MAJOR NUCLEAR BURNING STAGES The Coulomb barrier is

... Three general principles influence the roles that these nuclear burning stages may play: 1.Successive nuclear burning stages, involving more massive nuclei with higher charges, will require increasingly high temperatures to overcome the increased electrical repulsion. 2.The amount of energy released ...
Study Guide for the Final Astronomy Exam
Study Guide for the Final Astronomy Exam

... C) Explain the inverse square law nature of gravity. 5) Unit 32 to 34: Planetary Science A) In a written essay contrast the properties of the Terrestrial and Jovian planets. B) Answer multiple choice questions & short answer questions regarding the Solar Nebula Theory for the formation of Planetary ...
approximate temperature of the corona
approximate temperature of the corona

... A false eclipse or coronagraph view of the corona can be produced when a total eclipse is not occurring. An opaque, circular disc, which blocks out the majority of light from the Sun, allows the appearance of the corona to be seen and the magnetic field of the Sun to be viewed. Charged particles in ...
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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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