Origins of the solar system
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The sun formed 4.6 billion years ago from a dust cloud that collapsed under gravity. It is made primarily of hydrogen and helium and is about 93 million miles from Earth. As the sun uses up its hydrogen fuel over billions of years, it will expand into a red giant and later shrink into a white dwarf. The moon's phases are caused by its orbit around Earth as the sun illuminates different parts of the moon each month from our perspective on Earth. As the moon revolves around us, we see more or less of the side that is illuminated by the sun, appearing as a waxing and waning crescent, half moon, and full moon over the course of about 29.5 days.
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Our Solar System
The document summarizes key concepts about the sun and Earth's formation. It describes how the sun generates energy through nuclear fusion in its core, and how this energy reaches the surface in about 8 minutes. It also explains how Earth formed from the accretion of planetesimals, and how its core, mantle and crust layers developed as denser materials sank to the center. The oceans formed from early rainfall, and continents gradually emerged and shifted positions over billions of years.
The future of our solar system
By analyzing radioactive elements in meteorites, astronomers determined that the solar system formed 4.6 billion years ago from the gravitational collapse of a giant molecular cloud. This cloud collapsed over millions of years to form a rotating disk with the sun at the center. The planets formed from this disk, with the inner rocky planets closer to the sun and the outer gas giants farther away. In around 5 billion years, the Milky Way will collide with the Andromeda galaxy, and the solar system will be about 100,000 light years from the center of the new merged galaxy.
Proficiencies
The Solar System formed from a cloud of dust and gas that was disturbed by a nearby exploding star. This caused the cloud to collapse and spin, forming the Sun in the center and clumps of material that became the planets. The inner planets of Mercury, Venus, Earth and Mars are closer to the Sun and warmer, while the outer planets of Jupiter, Saturn, Uranus and Neptune are farther away and colder. Over time, the Sun will burn out and die, ending the Solar System.
Proficiency 2
I can analyze the differences between comets, asteroids, meteors and moons. I will research orbits and discuss differences of what we see from the Earth’s surface (phases). I will analyze the effect the moon’s orbit has on our planet. I will predict what would happen if Earth had a 2nd moon or the distance to the moon was increased or decreased.
Comets, asteroids, meteors, and moons
Comets are balls of ice, gas, and dust that orbit the sun and have four main parts: the nucleus, coma, hydrogen envelope, and tail. Asteroids are large rocky remains from the formation of the solar system, most located in the asteroid belt between Mars and Jupiter. The Earth's moon was likely created from an asteroid impact and orbits the Earth once per month, affecting ocean tides and the Earth's orbit.
Solar System Formation/Sun/Comets/Meteors
The document summarizes theories about how our solar system formed from a collapsing cloud of gas and dust. It describes how:
1) Our solar system likely began from a giant interstellar cloud that collapsed under gravity and formed a rotating disk, with a dense center that became the Sun and a surrounding disk that formed the planets.
2) The solar nebula disk varied in temperature by distance from the Sun, allowing different elements to condense into planetary cores near and far from the Sun, forming the terrestrial and gas giant planets.
3) Asteroids and comets are remnants from solar system formation and provide clues about its early history through observations and analysis of their composition and orbits.
Unit 4: How Our Solar System Formed
As stars die out and explode into supernovae, planets begin to form.
Register to explore the whole course here: https://school.bighistoryproject.com/bhplive?WT.mc_id=Slideshare12202017
Ncert universe
The document provides information about celestial bodies like stars, constellations, and planets in our solar system. It discusses how ancient people used constellations like Ursa Major to determine directions. It describes the nine planets in our solar system, with Mercury being the closest to the sun and Pluto being the farthest, along with other objects like asteroids and meteoroids. The sun and these celestial bodies form our solar system. It also briefly mentions Neil Armstrong being the first person to walk on the moon.
Solar system formation- Claudia and Matthew
Our solar system formed over 4 billion years ago from a giant cloud of gas and dust. An explosion from a nearby star created this cloud, and gravity caused the cloud to collapse and spin, forming a dense, hot center that became our Sun. As the cloud flattened, particles stuck together in the outer regions to form planets and moons, with rocky planets like Earth close to the Sun and massive gas giants like Jupiter farther out. Over time this led to the formation of our current solar system with its eight planets orbiting the Sun.
Formations of the solar system final- Sophie
Stars form from clouds of dust and gas that collapse under their own gravity. As the cloud collapses, a hot protostar forms at the center. Nearby clouds may break into blobs, explaining why most stars exist in pairs or groups. Planets form from disks of dust and gas that surround young stars. As the disk spins, dust clumps stick together, growing into planetesimals that eventually collide and merge into planets. Moons can form alongside planets from leftover material, be captured asteroids, or form from debris after a large impact. Eventually the sun will run out of hydrogen fuel and expand into a red giant, likely consuming the inner planets before collapsing into a white dwarf.
Comets, meteors, and asteroids
Comets, meteors, and asteroids are objects that orbit the sun. Comets are small icy bodies that develop tails as they heat up when passing near the sun. Meteors are small particles that burn up as they enter the Earth's atmosphere, sometimes forming meteor showers. Asteroids are rocky remnants from the early solar system and orbit mostly in the asteroid belt between Mars and Jupiter. The moon affects the Earth by providing light at night and influencing ocean tides through its gravitational pull.
Comets, meteors, and asteroids
This document provides information about comets, meteors, and asteroids. It states that comets are small icy masses that orbit the sun and have orbital periods ranging from years to centuries. Meteors are smaller than comets and are made of dust, with meteor showers occurring when cosmic debris enters the atmosphere. Asteroids are rocky remnants from the formation of the solar system and orbit mainly in the asteroid belt between Mars and Jupiter, ranging in size from hundreds of feet to hundreds of miles.
Comets, meteors, and asteroids
This document provides information about comets, meteors, and asteroids. It states that comets are small icy masses that orbit the sun and have orbital periods ranging from years to centuries. Meteors are smaller than comets and are made of dust, with meteor showers occurring when cosmic debris enters the atmosphere. Asteroids are rocky remnants from the formation of the solar system and orbit mainly in the asteroid belt between Mars and Jupiter, ranging in size from hundreds of feet to hundreds of miles.
Comets, meteors, and asteroids
Comets, meteors, and asteroids are objects that orbit the sun. Comets are small icy bodies that develop tails as they heat up when passing near the sun. Meteors are small particles that burn up upon entering Earth's atmosphere, sometimes forming meteor showers. Asteroids are rocky remnants from the early solar system and orbit mostly in the asteroid belt between Mars and Jupiter, ranging in size from hundreds of feet to hundreds of miles wide. The moon affects tides and lunar phases on Earth due to its gravitational pull and position relative to the sun.
Unit D Chapter 9 Space
The document provides an overview of the solar system, including information about the sun, planets, and other celestial bodies. It discusses the inner and outer planets, as well as characteristics of specific planets like Earth, Mars, Jupiter, Saturn, Uranus, and Neptune. It also covers moons, asteroids, comets, dwarf planets, and phases of the moon. The summary focuses on key details about the structure of the solar system and different types of objects within it.
Study of Solar system
What is a solar system?
FORMATION OF SOLAR SYSTEM
Components of the SOLAR SYSTEM
Discovery and exploration
Terminology
Description of the Components of the SOLAR SYSTEM
Farthest Regions
Galactic Context
The Solar System is located in the Milky Way galaxy, a barred spiral galaxy with a diameter of about 100,000 light-years containing about 200 billion stars. Our Sun resides in one of the Milky Way's outer spiral arms, known as the Orion Arm or Local Spur. The Sun lies between 25,000 and 28,000 light years from the Galactic Centre, and its speed within the galaxy is about 220 kilometres per second, so that it completes one revolution every 225–250 million years. This revolution is known as the Solar System's galactic year. The solar apex, the direction of the Sun's path through interstellar space, is near the constellation of Hercules in the direction of the current location of the bright star Vega. The plane of the Solar System's ecliptic lies nearly at right angles (86.5°) to the galactic plane.
Professor’s Questions Set 5Provide comprehensive answers to th.docx
Professor’s Questions Set 5
Provide comprehensive answers to the following questions. Remember to support your arguments where necessary by websites and pictures.
Chapter 7 and 8 Readings
1. Why is Jupiter so much richer in hydrogen and helium than Earth?
2. Why do astronomers conclude that none of the Jovian planets’ rings can be left over from the formation of the planets?
3. How can Jupiter have a liquid interior and not have a definite liquid surface?
4. Why are Uranus and Neptune respectively green-blue and blue?
5. What evidence indicates that catastrophic impacts have occurred in the solar system’s past?
6. Why do astronomers refer to carbonaceous chondrites as unmodified or “primitive” materials?
7. What evidence indicates that the asteroids are mostly fragments of larger bodies?
8. What is the difference between condensation and accretion?
9. Why does the solar nebula theory predict that planetary systems are common?
10. Why is the evidence of “hot Jupiters” puzzling? What is the current hypothesis of how they formed?
Michael Seeds
Dana Backman
Chapter 8
Origin of the Solar System and Extrasolar Planets
*
The solar system is our home in the universe. As humans are an intelligent species, we have the right and the responsibility to wonder what we are. Our kind has inhabited this solar system for at least a million years. However, only within the last hundred years have we begun to understand what a solar system is.
*
You are linked through a great chain of origins that leads backward through time to the first instant when the universe began 13.7 billion years ago.The gradual discovery of the links in that chain is one of the most exciting adventures of the human intellect.
The Great Chain of Origins
*
Earlier, you have studied some of that story:Origin of the universe in the big bangFormation of galaxiesOrigin of starsProduction of the chemical elementsHere, you will explore further and consider the origin of planets.
The Great Chain of Origins
*
By the time the universe was three minutes old, the protons, neutrons, and electrons in your body had come into existence. You are made of very old matter.
The History of the Atoms in Your Body
*
Although those particles formed quickly, they were not linked together to form the atoms that are common today.Most of the matter was hydrogen and about
25 percent was helium. Very few of the heavier atoms were made in
the big bang.
The History of the Atoms in Your Body
*
Although your body does not contain helium, it does contain many of those ancient hydrogen atoms that have remained unchanged since the universe began.
The History of the Atoms in Your Body
*
During the first few hundred million years after the big bang, matter collected to form galaxies containing billions of stars. You have learned how nuclear reactions inside stars combine low-mass atoms, su ...
Proficiency #4 for astronomey in science
The document discusses the formation of the solar system. It describes how a large rotating cloud of dust and gas called the Solar Nebula collapsed, forming the sun at the center and flattening particles into planetesimals that became the planets, moons, and other objects in the solar system. It then compares the inner terrestrial planets of Mercury, Venus, Earth and Mars to the outer gas giant planets of Jupiter, Saturn, Uranus and Neptune.
Astronomy unit 2011 SUN EARTH MOON SYSTEM acloutier copyright
The document provides an overview of concepts in astronomy including:
1) It describes Earth's rotation, the moon's effect on Earth, and how this impacts seasons and timekeeping.
2) It explains how the tilt of the Earth's axis and its orbit around the sun cause the seasons and equinoxes and solstices.
3) It discusses technology that has expanded our ability to observe space like telescopes, interferometry, and photography.
Ch08 solar system
The Solar System formed around 4.5 billion years ago from the collapse of a giant cloud of gas and dust. The inner planets are rocky while the outer planets are gaseous. Planets formed from the accretion of planetesimals, which collided and stuck together in the protoplanetary disk surrounding the young Sun. The temperature differences in the disk led to different compositions, with rocky planets in the hot inner region and icy planets in the cold outer region. Over time, planetesimals bombarded planetary surfaces and the planets differentiated into layers. Some planets may have migrated from their initial orbits due to interactions with the gas disk.
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- 6. "Our Solar System - ScienceClass." ScienceClass - Wonderings of science students on science topics. . N.p., n.d. Web. 8 Feb. 2011. <http://scienceclass.ning.com/profiles The solar system and the stars . North American ed. Milwaukee, WI: World Almanac Library., 2001. Print. "Sun." Views of the Solar System . N.p., n.d. Web. 8 Feb. 2011. <http://www.solarviews.com/eng/sun. "NASA - Cosmic Debate: What's Up With the Planets?." NASA - Home . N.p., n.d. Web. 8 Feb. 2011. <http://www.nasa.gov/centers/jpl/news/planetsf-20060815.html>. "Steve Quayle News Alerts." Welcome to the World of Steve Quayle! . N.p., n.d. Web. 10 Feb. 2011. <http://www.stevequayle.com/News "Solar System Earth Moon | Tutorvista.com." Tutorvista.com - Online Tutoring, Homework Help for Math, Science, English from Best Online Tutor . N.p., n.d. Web. 10 Feb. 2011. <http://www.tutorvista.com/physics/solar-system-earth-moon>.