Astronomy By Claire Andrues THE ORION NEBULA (M42)

Slides:



Advertisements
Similar presentations
By Gayla Burrage. The Hubble Telescope was launched in 1990.
Advertisements

Stars.
Chapter 19: Between the Stars: Gas and Dust in Space.
Space Science = Astronomy
DO NOW QUESTION Yesterday we talked about the future of the universe. What do you think will happen to the universe?
By Kain and Ian. What is it? Orion Nebula (also known as Messier 42, M42, or NGC 1976) NEBULA - an interstellar cloud of dust, hydrogen gas, helium gas.
Stellar Evolution: The Life Cycle of a Star. Stellar Nurseries All stars start out in a nebula (large cloud of dust and gas). All stars start out in a.
Copyright © 2010 Pearson Education, Inc. Clicker Questions Chapter 11 The Interstellar Medium.
Astronomical Imaging: Overview When you think of a clear, dark night sky, what do you think of? –The human visual system is fine-tuned to focus, detect,
Microwave: The Cosmic Microwave Background (CMB). Shortly after the Big Bang, the Universe cooled enough to allow atoms to form. After this point in time,
Types of Stars Life Cycle of Stars Galaxies
OUR SOLAR SYSTEM Our solar system is nearly 5 billion years old.
Stars & Constellations D. Crowley, Stars & Constellations G To know what a star and constellation is Thursday, August 13, 2015.
Stars, Galaxies, and the Universe
Astronomy Stars, Galaxies, and the Universe Tools of Ancient Astronomy.
The Universe Chapter 20.
STAR BIRTH. Guiding Questions Why do astronomers think that stars evolve? What kind of matter exists in the spaces between the stars? Where do new stars.
TOPIC: Astronomy AIM: What are stars?
Place in Space By Taylah Williams. What is a light year? Q1:The fastest thing that we know of is light which travels at a speed of 186,000 miles or 300,000.
Stars, Galaxies, and the Universe.  To understand how telescopes work, its useful to understand the nature of the electromagnetic radiation. Light is.
STARS. For most of recorded history the Earth was thought to be the center of the universe and never moved. The constellations were named and stories.
Galaxies & Star Systems Astronomy 2. Star Systems Our solar system only has one star (our sun); however, most are grouped together to groups of two or.
STARS BY SEYMOUR SIMON. Stars are huge balls of hot gases Our sun is a star, and it is the star nearest our planets Earth and our solar system Other stars.
Stars are born from a large collection of dusts and gasses that compress under the pressure of gravity, and eventually these dusts and gasses clump in.
The Universe. The Universe is….. All matter, including earth, galaxies, and intergalactic space.
1 Stars, Galaxies & Universe Chapter 3. 2 Tools of Astronomy Constellations are groups of stars that form a pattern. The electromagnetic spectrum is made.
The Milky Way Galaxy.
Nebulae. “Nebula” comes from the Latin word for cloud. “Nebulae” is the plural. It is loosely applied to anything that looks fuzzy or extended in a telescope.
Astronomy and the Electromagnetic Spectrum
STARS Amy Johnson. In General Stars are always in the sky, but can only be seen at night when the atmosphere is not so bright The Sun is the closet star.
Astronomy Part 1 General Science I Spring ‘09. History of the Universe Earth = 1 of 9 planets Sun= 1 of 100 billion stars in the Milky Way, 1 of infinite.
The Universe Chapter 16. Our Universe Only one that exists Includes everything –Stars, planets, galaxies, etc. Commonly accepted to be created by the.
Copyright © 2010 Pearson Education, Inc. Life Cycle of the Stars.
Galaxies of Stars.  By far the nearest star to earth.  A star is a large self-luminous body in space that creates its own radiant energy.  It gets.
What are stars? Glencoe: Chapter 26-2 Outline. Astronomy The study of objects and matter outside the Earth’s atmosphere and of their physical and chemical.
Stars By: Sana Gill. Characteristics Stars are spheres of plasma kept together by gravity. An example of a star is our sun. Are sun is one of at least.
Stars. Astronomy The study of space How astronomers measure distance 1. Light years– The distance light travels in one year 9.461x km.
All stars form in clouds of dust and gas. Balance of pressure: outward from core and inward from gravity.
STARS  Stars form when clouds of gases (mainly hydrogen) are pulled together by gravitational forces.  Atomic explosions occur inside stars. –They are.
Galaxies GALAXIES Stars are not randomly sprinkled throughout the universe. Most astronomers agree that there are about 100 billion galaxies in the universe,
The Life Cycle of a Star The Horsehead Nebula – one of the most famous pictures in astronomy.
11.1 Stars A star is a) a massive sphere of gases with a core like a thermonuclear reactor. b) the most common celestial body in the universe. c) It is.
A nebula is an interstellar cloud of dust, hydrogen gas and plasma. It is the first stage of a star's cycle. dusthydrogenplasmastar.
The Interstellar Medium. Red, White, and Blue : Nebulae.
Astronomy Review. What 3 pieces of evidence supports the Big Bang Theory? 1) Doppler Effect 2) Microwave Radiation 3) Quasars.
Nebulas by Brian Charlesworth. Long Exposure Photography Long exposure photography of the universe is an incredible mix of art and science.
Earth and Space GALAXIES. A long time ago in a galaxy far, far away…
Astronomy 2 Overview of the Universe Spring Lectures on Star Formation.
Emily Linden & Fiona Ward
Spring 2012 Astronomy Course Mississippi Valley Night Sky Conservation The Sky Around Us Program developed by Mississippi Valley Conservation Authority.
Study of the universe (Earth as a planet and beyond)
STARS AND GALAXIES The Life Cycle of a Star: Stars have a life cycle and evolve over time. The mass of a star controls its Evolution Lifespan Ultimate.
1 Chapter 12 Objectives: 1)List the major objects that can be seen in our night sky. 2)Define a light year and be able to convert it to distances. 3) Define.
The Lifecycle of Stars. Introduction Did you know that, just like us, stars are born, grow older and die? This presentation will guide you through some.
Stars Huge spheres of very hot gas that emit light and other radiation. They are formed from clouds of dust and gas, or nebulas, and go through different.
STARS Earth and Space. INTRODUCTION When you look at the sky on a clear night, you can see dozens, perhaps even hundreds, of tiny points of light. Almost.
Warmup How would you explain the concepts of a year, a month, and a day to a small child?
Study of the universe (Earth as a planet and beyond)
Astronomy. Astronomy Vocabulary Big Bang Theory: the tremendously powerful explosion of an incredibly dense mass about billion years ago that produced.
Stars and Galaxies Chapter 12. Stars Definition: a large ball of gas that emits energy produced by nuclear reactions in the star’s interior Planets, comets,
Introduction to Astronomy
Galactic Structure.
STARS Visual Vocabulary.
What do you see in the photographs of the sky?
14.2 Galactic Recycling Our Goals for Learning
Chapter 15 Preview Section 1 Stars
Constellations The Night Sky.
Pan-STARRS & Nebulae Briana Gonzalez.
The Interstellar Medium
Presentation transcript:

Astronomy By Claire Andrues THE ORION NEBULA (M42)

WHERE IS IT LOCATED IN OUR SKY? The Orion Nebula is located in the constellation Orion. It can be located with the naked eye by first finding Orion’s belt, a visible curved path of three stars, and then finding the two stars Betelgeuse and Rigel, which are among the brightest stars in our sky. Find the midpoint between the stars and then look under the belt of Orion. The Orion nebula is close to earth, which makes it a visible fluffy ball in our night sky.

WHERE IS IT LOCATED IN SPACE? The Orion nebula is located, like Earth, in the Milky way Galaxy. The Orion nebula is very close to Earth compared to other objects in the constellation Orion. While the star Betelgeuse is 640 light years away and the star Rigel is 800 light years away, the Orion Nebula is only 35 light years away from Earth. Its close proximity makes it one of the only nebulas that the human eye can examine in the sky.

WHAT IS A NEBULA? A nebula is an interstellar cloud of dust in space. It contains hydrogen, helium, and other gases. A nebula is a region where stars are born. Gases and space dust come together under a gravitational collapse and form large masses. These new masses attract other matter in space and eventually form stars like our Sun.

THE ORION NEBULA The nebula is about 24 light years across and is 2000 more times massive then the mass of our sun. It is at least two million years old and has been creating stars for that same amount of time. The Orion nebula is still active today. Loose clusters of 700 newly formed stars are seen in the nebula. Stars that are thought to have formed in the Orion nebula from two million years agao include: AE Aurigae, 53 Arietis and Mu Columbae Stars that are very young in the nebula are the open cluster Trapezium, which contains four main stars, two of which are binary systems which contain two more stars equaling six in the cluster.

HISTORY The Orion Nebula can be seen in the night sky with a sharp eye and so its discovery goes far back in our history. The Mayans are thought to have noticed the nebula and use it in stories such as their “Three Hearthstones” myth that compared the nebula to the area of Orion’s belt. It is not known whether Early Astronomers such as Ptolemy and Galileo noticed the nebula because it is not mentioned in any of their writings about the sky. The first recorded observation on the nebula was by Nicolas-Claude Fabri de Peiresc, a French astronomy in 1610 using a refracting telescope. Later the first publication was by Johann Baptist Cysat in 1619 Nicolas-Claude

FIRST PHOTOGRAPH In 1880 Henry Drape, a professor in Astronomy, captured the first photograph of the Orion Nebula. The photograph is overexposed and shows the surrounding stars much brighter than the nebula.

SO MANY COLORS Like many other nebulae, M42 has areas of red and blue-violet coloration. The visible red is created by a hydrogen emitted wavelength, while the blue is created by the reflected radiation from O-class stars found in the nebula. The difference in the Orion Nebula from others is the large amount of green coloration. In the early 20 th century when not many other nebulae had been observed by astronomers. The green color was thought to be a new unknown element. Spectral lines had not been distinguished and so the color could not be identified. It is now known that the green spectral lines come from an electron transition in ionized oxygen that is considered “low-probable”

THE ORION NEBULA

SOURCES