• 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
Our Star, the Sun Chapter Eighteen Guiding Questions
Our Star, the Sun Chapter Eighteen Guiding Questions

... • The Sun’s surface features vary in an 11-year cycle • This is related to a 22-year cycle in which the surface magnetic field increases, decreases, and then increases again with the opposite polarity • The average number of sunspots increases and decreases in a regular cycle of approximately 11 ye ...
Jupiter`s Moons - cloudfront.net
Jupiter`s Moons - cloudfront.net

... They are large, about the size of the Earth’s Moon. These and four more smaller moons all orbit in the same direction as Jupiter spins. These 8 moons all probably formed with Jupiter like a Solar System in miniature. ...
ρ ρ ρ ρ - Bryn Mawr College
ρ ρ ρ ρ - Bryn Mawr College

... Moment of inertia factors I/MR2 (and other information) for the various planets can be found at (http://nssdc.gsfc.nasa.gov/planetary/planetfact.html). Find the values for the Sun, Venus, Mars, the moon, Earth, and Jupiter. Put these in order from large to small and explain what they tell about the ...
Year of the Sun
Year of the Sun

... This photo was taken using ultraviolet light, so the green colour is artificial. ...
Twinkle, Twinkle, Little Star
Twinkle, Twinkle, Little Star

... What are stars? Giant balls of gas that undergo nuclear fusion. Nuclear fusion is when the nuclei of two atoms join together to make a bigger nucleus and release energy. ...
The Sun: Our Extraordinary Ordinary Star
The Sun: Our Extraordinary Ordinary Star

... • Dim layer of less dense stellar gas • Pinkish strip 200 km thick • Spicules – jets of gas shooting up 1000 km • 1/3 of a million at any given time covering a few percent of the Chromosphere • Occur at boundaries of supergranules – slightly larger than Earth ...
The Solar System
The Solar System

... (Where do stars come from?) - Stars begin as a large cloud of gas and dust called a nebula, which contracts due to gravity when it gets large enough. As temperatures increase, nuclear fusion begins and light is given off. Now it’s a star. - Most of its life is spent as a main sequence star -- an ave ...
Dead Earth – Lesson 1
Dead Earth – Lesson 1

... GAMMA RAYS ...
Midterm 3 Review Sessions Two choices:
Midterm 3 Review Sessions Two choices:

... shuts off after Heflash. ...
The Synodic and Orbit Periods of the Planets
The Synodic and Orbit Periods of the Planets

What are we going to do in science during Quarter 2?
What are we going to do in science during Quarter 2?

... What are we going to do in science during Quarter 2?     These are the CT Science Frameworks that will guide our class activities.  GRADE 8 Forces and Motion 8.1 — An object’s inertia causes it to continue to moving the way it is moving unless it is acted upon by a force. State Framework 8.1.a The m ...
Moons of Jupiter Age of Surface
Moons of Jupiter Age of Surface

... Roche’s limit and the Rings Large objects cannot form in this region, or get broken up even if they do form. 4. Why can’t the material in the rings collect to form moons? a. There is not enough material b. The rings are too thin c. The rings are inside the Roche limit d. The rings are not made of s ...
geography-vocabulary-word-list
geography-vocabulary-word-list

... Q10. Fill in the blanks:1. Our solar system is a part of________galaxy. 2. The brightest star in the saptarishi is________. 3. The word planet is derived from greek word________. 4. The planet having rings around it is _______. 5. Planets which rotate from west to east is______. 6. Nearest planet to ...
Questions - HCC Learning Web
Questions - HCC Learning Web

1 The Synodic and Orbit Periods of the Planets
1 The Synodic and Orbit Periods of the Planets

... Calculate the percent difference between your Voyager observations and these accepted S values. Make a graph of accepted S vs. planet number (Mercury = 1, Venus = 2, etc.). Is this relationship monotonic? ___________ Is this relationship linear? _____________ Describe the curve in words. (Do not try ...
37) What is the largest planet in the solar system?
37) What is the largest planet in the solar system?

... A) Mars, Mercury, Venus, Earth, Jupiter, Saturn, Uranus, Neptune B) Mercury, Venus, Earth, Mars, Jupiter, Saturn, Neptune, Uranus C) Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune D) Mars, Venus, Earth, Mercury, Saturn, Jupiter, Uranus, Neptune E) Venus, Mercury, Earth, Mars, Saturn, ...
File
File

the solar system
the solar system

... moving through space (dirty snowball) 1) Nucleus—center of a comet 2) Coma—cloud of vaporized (turned to gas) ice that surrounds the nucleus 3) Tail—the coma of a comet that is being blown back by solar winds 4) Oort cloud—birthplace of comets found beyond Pluto (a) Objects are dislodged by the grav ...
Seasonal and Daily Temperatures and the Earth’s General
Seasonal and Daily Temperatures and the Earth’s General

... • Sunlight heats mountain slopes during the day and they cool by radiation at night • Air in contact with surface is heated/cooled in response • A difference in air density is produced between air next to the mountainside and air at the same altitude away from the mountain • Density difference produ ...
Design of a Locomotive Engine for Dalian Locomotive & Rolling
Design of a Locomotive Engine for Dalian Locomotive & Rolling

...  The shape of the oldest crater size-frequency ...
Extraterrestrial Life
Extraterrestrial Life

Recap: High Mass Stars
Recap: High Mass Stars

... away! • From ½ all the way down to 0.075% of the Sun’s mass • Burn cool, less than 3500 K. Dim light. • Can live a REALLY long time. 10,000,000,000,000 years? • Our nearest star neighbor is Proxima Centauri, a red dwarf. • Most numerous stars in the entire Universe! ...
Pluto
Pluto

... • You need “metals” to make planets –Metals are elements heavier in mass than helium ...
Astronomy Comprehensive Test
Astronomy Comprehensive Test

... 20. The planet Uranus is unusual because its axis of rotation lies almost in the plane of its revolution. If the axis is pointing toward the sun as in the picture, what would occur at point X when the planet turns once on its axis? a. the point would be in twilight for the full rotation b. the point ...
File
File

... • What about the development of intelligence? • Many anthropologists think intelligence is favored by natural selection and closely linked to language. • Cultural evolution on Earth began around 10,000 years ago. ...
< 1 ... 330 331 332 333 334 335 336 337 338 ... 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