• Study Resource
  • Explore Categories
    • 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
here - Immersive Theatres
here - Immersive Theatres

... dimmer – just by fractions of a percent. But this, too, can be measured with high precision,  and allows us to determine the size and orbit of the planet.  It was discovered that the planet of “51 Pegasi” is rather strange. It is almost as large as  Jupiter, but orbits so close to the star that it i ...
Lecture 21: Planet formation III. Planet
Lecture 21: Planet formation III. Planet

solar-activity-ref
solar-activity-ref

... The core is the central region of the Sun and has a temperature of 15 million degrees. From here comes the star’s power; every second 564 million tons of hydrogen are fused, through thermonuclear reactions, to 560 million tons of helium. Hydrogen nuclei (protons) become helium nuclei at a rate of f ...
I. Abundances – The Composition of the Universe
I. Abundances – The Composition of the Universe

... “Independent of any theory of the origin of the universe, one may try to find indications For the nature of the last nuclear reaction that took place …going backwards in time One may then try to find out how the conditions developed under which these reactions took place. … a cosmogenic model may th ...
Introduction This book will teach you all you need to know about the
Introduction This book will teach you all you need to know about the

... The earth has four layers. The first layer is the crust. The crust makes only one percent of the entire earth. The crust is filled with the animal, planet life and the water and other things on which life need to thrive. The crust is about 5 to 30 miles deep. There are two types of crust. The first ...
The Milky Way - Houston Community College System
The Milky Way - Houston Community College System

... high-energy particles At this time, no star capable of producing a supernova is less than 50 ly away. The most massive star known (~ 100 solar masses) is ~ 25,000 ly from ...
Wilmslow Guild Lecture 2008
Wilmslow Guild Lecture 2008

... Attempts by the ancient Greeks to measure the distance to the sun using trigonometry were correct in their method but limited by the absence of appropriate astronomical instruments. By 150 BC, they had gauged the sun to lie at a distance of perhaps 8 million km, and this, they reasoned, was also the ...
Sky Watching Talk
Sky Watching Talk

... comments arise because you cannot see the Constellations near where the Sun is in the sky – Sun so bright it washes out rest of stars ...
RIPL Radio Interferometric Planet Search
RIPL Radio Interferometric Planet Search

... Sensitivity is limited by the short lever arm of VLBA observations: ~10 days RIPL will extend this lever arm by factor of 100 ...
Gravitation
Gravitation

... You move a ball of mass m away from a sphere of mass M. 1.  Does the gravitational potential energy of the system of the ball and sphere a)  Increase, or b)  Decrease. 2. Is the Work done by the gravitational force between the ball and the sphere a)  Positive work, or b)  Negative work ...
Distance - courses.psu.edu
Distance - courses.psu.edu

... 3. a) A star with the Sun's luminosity, but located 2 AU from Earth instead of 1 AU, would appear how bright relative to the Sun? b) A star with the Sun's luminosity, but located 20 AU from Earth instead of 1 AU, would appear how bright relative to the Sun? 4. Jupiter's moon Europa, which effectivel ...
Scales This is a 16 meter by 16 meter scene. A meter is close in size
Scales This is a 16 meter by 16 meter scene. A meter is close in size

... now? (ANS: No! We are seeing what it looked like 4.2 years ago when the light left the star. ) What if you were looking at a star 100 light years away? Would you be seeing it the way it looks now? (ANS: No! You’d be seeing it the way it looked 100 years ago, when the light left the star. The star co ...
White Dwarfs
White Dwarfs

White Dwarfs
White Dwarfs

Benchmark lesson
Benchmark lesson

... gas and the helium gas that makes up the Sun. During the reaction, called nuclear fusion, large amounts of energy are given off in the form of light and heat. Many schools and community buildings in Florida use this energy to heat water. The energy from the heated water is used to make electricity. ...
E5 stellar processes and stellar evolution (HL only)
E5 stellar processes and stellar evolution (HL only)

... • Core contracts under its own weight • It stops when electrons have to be forced into the same quantum state. This is not allowed so this “electron degeneracy pressure” stops the star collapsing further • The outer layers are released to form a planetary nebula • The resultant White dwarf has no en ...
Class 8 - ruf.rice.edu
Class 8 - ruf.rice.edu

... that the distance of the planet from the Sun varies during its orbit. Its closest point is called perihelion. ...
Gravity and Motion
Gravity and Motion

... Action at a Distance  In ...
The Sun
The Sun

... Sunlight absorbed through the skin is used by humans to make vitamin D, an important vitamin for bone health. The Changing Sun Much like everything else in the Solar System, the Sun is constantly changing. Every eleven years, the Sun goes through a solar cycle, which causes an increase in its magnet ...
ASTRONOMY 0089: EXAM 1 Class Meets M,W,F, 1:00 PM Feb 12
ASTRONOMY 0089: EXAM 1 Class Meets M,W,F, 1:00 PM Feb 12

... 25. The reason that the primary mirror of an astronomical telescope is often polished to a parabolic shape is a. to avoid chromatic aberration which would be produced by a spherical mirror. b. because it is easier to produce than a spherically shaped mirror. c. to avoid spherical aberration by brin ...
ASTR-100 - Jiri Brezina Teaching
ASTR-100 - Jiri Brezina Teaching

... bodies) is resisted by internal friction, which causes heating. This way, the rotational (and, if applicable orbiting) energy is consumed and the driving motions become slower. ...
SES_Book_Interactive 508
SES_Book_Interactive 508

... taken from space, that there is and never was a solar constant. The total amount of energy emitted from the Sun varies on all scales of time, from seconds to years, as does the energy emitted in any of the different spectral components that contribute to that sum. Everything changes, all of the time ...
Issue 122 - Aug 2014
Issue 122 - Aug 2014

... Only, that's not quite right. Depending on how thick the Earth's crust is, whether you're slightly closer to or farther from the Earth's center, or what the density of the material beneath you is, you'll experience slight variations in Earth's gravity as large as 0.2%, something you'd need to accoun ...
Celestial Motions
Celestial Motions

... The Greeks knew that the lack of observable parallax could mean one of two things: 1. Stars are so far away that stellar parallax is too small to notice with the naked eye 2. Earth does not orbit Sun; it is the center of the universe With rare exceptions such as Aristarchus, the Greeks rejected the ...
Opakování z minulého cvičení
Opakování z minulého cvičení

... renewed by 'new' comets picked up by the Solar System when it passes through giant molecular clouds. The Oort cloud may contain 100 billion comets. From time to time, the gravitational influence of a passing star will disturb the Oort cloud and send comets in towards the Sun, where the gravitational ...
< 1 ... 196 197 198 199 200 201 202 203 204 ... 503 >

Formation and evolution of the Solar System



The formation of the Solar System began 4.6 billion years ago with the gravitational collapse of a small part of a giant molecular cloud. Most of the collapsing mass collected in the center, forming the Sun, while the rest flattened into a protoplanetary disk out of which the planets, moons, asteroids, and other small Solar System bodies formed.This widely accepted model, known as the nebular hypothesis, was first developed in the 18th century by Emanuel Swedenborg, Immanuel Kant, and Pierre-Simon Laplace. Its subsequent development has interwoven a variety of scientific disciplines including astronomy, physics, geology, and planetary science. Since the dawn of the space age in the 1950s and the discovery of extrasolar planets in the 1990s, the model has been both challenged and refined to account for new observations.The Solar System has evolved considerably since its initial formation. Many moons have formed from circling discs of gas and dust around their parent planets, while other moons are thought to have formed independently and later been captured by their planets. Still others, such as the Moon, may be the result of giant collisions. Collisions between bodies have occurred continually up to the present day and have been central to the evolution of the Solar System. The positions of the planets often shifted due to gravitational interactions. This planetary migration is now thought to have been responsible for much of the Solar System's early evolution.In roughly 5 billion years, the Sun will cool and expand outward many times its current diameter (becoming a red giant), before casting off its outer layers as a planetary nebula and leaving behind a stellar remnant known as a white dwarf. In the far distant future, the gravity of passing stars will gradually reduce the Sun's retinue of planets. Some planets will be destroyed, others ejected into interstellar space. Ultimately, over the course of tens of billions of years, it is likely that the Sun will be left with none of the original bodies in orbit around it.
  • studyres.com © 2025
  • DMCA
  • Privacy
  • Terms
  • Report