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red giant - Teacher Pages
red giant - Teacher Pages

... What are the reactants and products in the primary fusion reaction carried out within the sun? What is the widely accepted scientific model that describes the formation of the solar system? ...
Nick Bowden The Final Frontier
Nick Bowden The Final Frontier

... circled the early Sun. Most planets have moons. and they are round but some of them are different circles like ovals.  While there's a group of planets that are made of gas, there are four planets in our solar system that are made of hard rock.  So, some planets are alike by what they're made of. ...
how the Sun impacts the Earth
how the Sun impacts the Earth

... began as a huge cloud of (mainly) hydrogen and helium collapsing under its own gravity. Most of this matter went into the Sun. Some tiny part of it ended up as the rest of the solar system. Leads to the concept of the solar nebula for the cloud of matter that surrounded the “proto-Sun” ...
Light and dark in this magnetic scan of the Sun indicate
Light and dark in this magnetic scan of the Sun indicate

... Through the Photosphere that's the part that we see The light comes out and shines on you and me ...
The Edge of the Solar System The Oort Cloud
The Edge of the Solar System The Oort Cloud

... sun (Kuiper belt ends at 55 AU) Centauri is 270,000 AU from sun ...
The Oort Cloud
The Oort Cloud

... • Distance between Oort Cloud Comets: 50-500 million km (0.33-3.33 AU) • Surface temp. in Oort Cloud ~5-6 K (Kuiper belt 30-60 K) • Named after Jan Oort ...
Name - CHS Room 124
Name - CHS Room 124

... 3. One asteroid belt, located between Mars and Jupiter 4. Dwarf planets, like Pluto (considered to be a planet for about 75 years!) 5. Many moons (Earth has only one, but Saturn, for example, has 25+) C. Planet Facts 1. Mercury- the closest planet to the sun, revolves around the Sun the fastest—once ...
Exam #1 Review
Exam #1 Review

... space at constant velocity. If they fire their rockets at the same time, which of the two ships will speed up faster? • A. The one with the lower mass. • B. The one with the higher mass. • C. They will speed up equally, because they ...
The Universe - Lancaster High School
The Universe - Lancaster High School

... 3 Directions of Death… 1. Release of Outer layers – Sun 2. Nova – Stars bigger than Sun – explosion 3. Supernova – Most massive stars – Chuck Norris of explosions. -can be as bright as an entire galaxy ...
Astronomy 1020 Exam 1 Review Questions
Astronomy 1020 Exam 1 Review Questions

... 19. Whose observations did Kepler use to formulate his 3 laws of planetary motion? Of what planet were these observations made? Why was Kepler so interested in geometric solids? 20. Who is considered the father of experimental physics? Who was the first person to use a telescope to study the cosmos? ...
ASTR0 100 HW #4 – SOLUTIONS – 2 points each
ASTR0 100 HW #4 – SOLUTIONS – 2 points each

... All types of atoms (and also ions and molecules) have their own distinct set of energy levels and a corresponding distinct set of energy transitions when photons are emitted or absorbed by those atoms. These transitions mean that each atom has a unique set of spectral lines, and so when we examine a ...
modeling astronomy concepts with a gps receiver and
modeling astronomy concepts with a gps receiver and

... Students should be encouraged to find the constellation URSA MINOR in the night sky. With their makeshift sextants they should stand in a clear area after night fall and peer through their straws at the star Polaris. They should then record the measurement on the angle ruler. It may be helpful for ...
The Sun
The Sun

... 1. The Sun is a rather normal star ________ 2.The Sun’s average density is less than that of Earth ________ 3.The Sun’s diameter is about 10 times that of Earth ________ 4.Sunspots show that the Sun’s poles spin faster than the equator ________ 5.Convection currents in the Sun involve cool gas risin ...
The Sun - WordPress.com
The Sun - WordPress.com

... It is a giant ball of burning gas. It projects ultra violet rays but our ozone layer protects us from its radiation. It is a source of Vitamin D and we need the Sun to Survive. ...
APOM 2014 April
APOM 2014 April

... This week's issue of Naturefeatures an interesting announcement by Chadwick Trujillo (Gemini Observatory) and Scott Sheppard (Carnegie Institution for Science). These two observers have found an object orbiting the Sun, designated 2012 VP113, that they first spotted 17 months ago with the 4-m Blanc ...
The solar system
The solar system

... objects in space that orbit (go around) it. The Sun is orbited by planets, moons, asteroids, comets and other things. ...
lecture 32 orbits
lecture 32 orbits

... that Earth is located at the center of the universe. The stars were fixed to the outermost shell. There are 7 concentric spherical shells, each containing one object: Sun, Moon, or a planet (5 planets were known then). The shells rotate uniformly around Earth. ...
Our Earth and Other Planets Lessons
Our Earth and Other Planets Lessons

... Lively and colorful illustrations provide a fun introduction to the solar system. Fictitious postcards from each planet can give children a creative impetus for their own reports. Keep in mind that since the book was written, Pluto has been reclassified as a dwarf planet and additional moons have be ...
The Sun: center of the Solar System
The Sun: center of the Solar System

... million years ago, similar in size to Chicxulub) • Barringer Crater (Arizona; one of the bestpreserved on Earth) • Ries and Steinholm (Germany; same age, probably binary asteroid) ...
Earth in Space
Earth in Space

... areas are swept out in equal time. • This area is equal to • This area ...
Lecture 27 (pdf from the powerpoint)
Lecture 27 (pdf from the powerpoint)

... fp = 0.5 (half of all stars formed will have planets) ne = 2 (2 planets per star will be able to develop life) fl = 1 (100% of the planets will develop life) fi = 0.01 (1% of which will be intelligent life) fc = 0.01 (1% of which will be able to communicate) L = 10,000 years (which will last 10,000 ...
The Sun
The Sun

... The Sun Unit 6: Astronomy ...
20.1 A Solar System is Born
20.1 A Solar System is Born

... The Solar Nebula Nebula – a large cloud of gas and dust in interstellar space • Where stars are born or explode at the end of their lives • Hydrogen, helium, carbon, iron • Two forces that interact with nebulas to create planets and stars – Gravity & Pressure ...
Chapter 11
Chapter 11

... Served Us Nachos (Mercury, Venus, Earth, Mars , Jupiter, Saturn, Uranus, Neptune) ...
ppt
ppt

... All of them are bright compared with the majority of the stars. Some – Venus, Mars, and Jupiter – can outshine the brightest stars in the sky. ...
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Solar System



The Solar System comprises the Sun and the planetary system that orbits it, either directly or indirectly. Of those objects that orbit the Sun directly, the largest eight are the planets, with the remainder being significantly smaller objects, such as dwarf planets and small Solar System bodies such as comets and asteroids. Of those that orbit the Sun indirectly, two are larger than the smallest planet.The Solar System formed 4.6 billion years ago from the gravitational collapse of a giant interstellar molecular cloud. The vast majority of the system's mass is in the Sun, with most of the remaining mass contained in Jupiter. The four smaller inner planets, Mercury, Venus, Earth and Mars, are terrestrial planets, being primarily composed of rock and metal. The four outer planets are giant planets, being substantially more massive than the terrestrials. The two largest, Jupiter and Saturn, are gas giants, being composed mainly of hydrogen and helium; the two outermost planets, Uranus and Neptune, are ice giants, being composed largely of substances with relatively high melting points compared with hydrogen and helium, called ices, such as water, ammonia and methane. All planets have almost circular orbits that lie within a nearly flat disc called the ecliptic.The Solar System also contains smaller objects. The asteroid belt, which lies between Mars and Jupiter, mostly contains objects composed, like the terrestrial planets, of rock and metal. Beyond Neptune's orbit lie the Kuiper belt and scattered disc, populations of trans-Neptunian objects composed mostly of ices, and beyond them a newly discovered population of sednoids. Within these populations are several dozen to possibly tens of thousands of objects large enough to have been rounded by their own gravity. Such objects are categorized as dwarf planets. Identified dwarf planets include the asteroid Ceres and the trans-Neptunian objects Pluto and Eris. In addition to these two regions, various other small-body populations, including comets, centaurs and interplanetary dust, freely travel between regions. Six of the planets, at least three of the dwarf planets, and many of the smaller bodies are orbited by natural satellites, usually termed ""moons"" after the Moon. Each of the outer planets is encircled by planetary rings of dust and other small objects.The solar wind, a stream of charged particles flowing outwards from the Sun, creates a bubble-like region in the interstellar medium known as the heliosphere. The heliopause is the point at which pressure from the solar wind is equal to the opposing pressure of interstellar wind; it extends out to the edge of the scattered disc. The Oort cloud, which is believed to be the source for long-period comets, may also exist at a distance roughly a thousand times further than the heliosphere. The Solar System is located in the Orion Arm, 26,000 light-years from the center of the Milky Way.
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