What might you discover today? The Faulkes Telescopes (FT) have been built for school children to discover the excitement of looking at stars and galaxies.

Slides:



Advertisements
Similar presentations
Copy and Answer in NB 1.What are the three layers of the suns atmosphere? 2.What produces auroras? 3.What are sunspots and why are they dark? 4.Describe.
Advertisements

It’s 5 times greater. It’s 10 times greater. It’s 20 times greater.
They seem to form a picture in the sky. People use them to find their way around the sky like someone using objects to get from place to place.
Space Science = Astronomy
Earth in Space Notes Part 1. Our Solar System Objects in our solar system move in predictable patterns. The predictable movement of these objects are.
By Emily LaPorte!. this slide show will have information about the universe astrononaghts stars and more!
Part I: A Trip Through the Universe What We Will See STARS AND GALAXIES 1.
Astronomy- The Original Science Imagine that it is 5,000 years ago. Clocks and modern calendars have not been invented. How would you tell time or know.
The Nature of the Stars Chapter 19. Parallax.
The Faulkes Telescopes: A Robotic Telescope Network for School Science Students Dr David Frew Department of Physics, Faculty of Science, Macquarie University.
Part I: A Trip Through the Universe “Our Transportation” STARS AND GALAXIES 1.
Chapter 8: Stars By Sydney Bullock & Abby Swanager.
Stars, Galaxies, and the Universe.  To understand how telescopes work, its useful to understand the nature of the electromagnetic radiation. Light is.
Galaxies.
Discoveries in Planetary Sciencehttp://dps.aas.org/education/dpsdisc/ Dwarf Planet Smaller than Originally Thought Eris is a large icy object orbiting.
Galaxies Hubble Deep Field – taken by the Hubble telescope above the Earth.
Which scientist was the first to use the telescope in astronomy?
Friday, April 16 th Agenda  Quiz over section 18.2: Stars and the Sun  Start Section 18.3: The Solar System  KWL graphic organizer  Movie: “Space.
A Trip Through the Universe Part II. What are binary stars?
Astronomy and the Electromagnetic Spectrum
Happy Birthday Jodrell Bank! From West Mon School’s Astronomy Club and GCSE Astronomy Classes.
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.
OBSERVATION OF THE BINARY STAR NN SER USING THE FAULKES TELESCOPE Anne O ’Leary –Sacred Heart Grammar School Newry This project was carried out at the.
The Universe Chapter 16. Our Universe Only one that exists Includes everything –Stars, planets, galaxies, etc. Commonly accepted to be created by the.
Astronomy- The Original Science Imagine that it is 5,000 years ago. Clocks and modern calendars have not been invented. How would you tell time or know.
What is the Big Bang? The Big Bang theory is an effort to explain what happened at the very beginning of our universe about 15 Billion years ago.
Stars!!!! Galaxies and the Universe too!. Stars are far away! The closest star to Earth is the sun. The next closest is Proxima Centauri If you can travel.
By: Tori and Michelle.  The Andromeda galaxy is a spiral galaxy approximately 2.5 million light-years away.  It is also known as Messier 31, M31, or.
The Nature of the Stars Chapter 19. Parallax.
The Nebula Beginning. So……. What is the evidence???
Tour of the Invisible Universe From the Moon to Beyond.
Astronomy- The Original Science
Voyage Through Space… Artist rendition. Spaceship Earth, Our Home Satellite Composite.
Planets, Solar Systems, and Galaxies…..Oh my!
Methods and materials To calculate the frequencies present in the light curve of KPD , a Fourier transform is needed. However, in order to complete.
Leaning objectives: Explain that: Elements as heavy as iron are formed inside stars by nuclear fusion. Heavier elements are formed in supernovas. Exploding.
Chapter 27 Stars and Galaxies Section 1 Characteristics of Stars Notes 27-2.
© Sierra College Astronomy Department 1 Astronomy 10 Elementary Astronomy COURSE GOALS & OBJECTIVES.
Models of the Universe Highlights of yesterday’s workshop Observations, virtually Todays’ workshop: compare two models E.J. Zita.
Astronomy: The Original Science How did people in ancient times tell time? The studied the movement of stars, planets and the moon. They watched as the.
Objectives Determine how distances between stars are measured. Distinguish between brightness and luminosity. Identify the properties used to classify.
Red Giant Phase to Remnant (Chapter 10). Student Learning Objective Describe or diagram the evolutionary phases from the beginning of stellar formation.
Earth and Space GALAXIES. A long time ago in a galaxy far, far away…
Stellar Evolution Task High Mass Stars How do they evolve.
Exploring the Universe. Big Bang Theory The big bang theory is how the scientist say the universe began. How the Big Bang Started most people believe.
Unit 1: Space 1. Section 10-1 Notes 2 Celestial Bodies Celestial bodies are natural objects out in space including planets, stars, moons, asteroids and.
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.
P1 - Foundation Part 3 – Space Put these in order of smallest to largest. Star, Galaxy, Solar system, Moon, Universe, Planet.
What is in our solar system?. What is the difference between a solar system, a galaxy and the Universe? A solar system is a star and all the objects that.
Globular Clusters Globular clusters are clusters of stars which contain stars of various stages in their evolution. An H-R diagram for a globular cluster.
The Faulkes Telescope Project Dr. Paul Roche and Dr. Sarah Roberts Cardiff University, UK.
© OUP: To be used solely in purchaser’s school or college 7L The Solar System and beyond Time on Earth Views from the Earth Beyond the Earth 7LThe Solar.
Accelerated Reading Time until 1:49.
Stellar Evolution Task
An Introduction to the sky at night
New topic: Space.
25.1 Properties of Stars Objectives:
Learning Goals: I will:
THE SOLAR SYSTEM AND BEYOND
Major features of the Milky Way and the Universe
Observing Planets and Stars
Homework: Due at Midnight
Unit 11- Characteristics of the Universe
Topic 1 Topic 2 Topic 3 Topic 4 Topic 5 $100 $100 $100 $100 $100 $200
The Night Sky What are the patterns in the sky and why do they change throughout the year?
No gum, candy or chewing please! 
The sky at night.
After Bellwork, Read the FYI on the “Cosmological Distance Ladder” then answer the two questions in your science journal.
Science Unit D Review Chapter 2.
Presentation transcript:

What might you discover today? The Faulkes Telescopes (FT) have been built for school children to discover the excitement of looking at stars and galaxies far out in space. With one in Hawaii (FTN) and one in Australia (FTS), where it is night during daytime in Europe, classes can take control of a fully equipped 2-metre telescope and choose their own objects to explore. Pupils can also obtain images offline for more extended research projects. Together with the Faulkes Telescope Project, the Armagh Observatory and Planetarium are developing pupil- researcher partnerships to encourage young people of today to become the scientists of tomorrow. Schools can get involved directly by booking time on the telescopes. Students can pursue individual projects, either through their schools or during the summer at the Armagh Observatory. This poster illustrates just some of the projects that might be pursued. Further details can obtained from the contact addresses below. Contacts The Faulkes Telescope Project: Schools co-ordinator for Ireland: Robert Hill, Armagh Planetarium, , Pupil-researcher partnerships: Simon Jeffery, Armagh Observatory, , Nuffield Science Bursaries: Sentinus, Photo Credits Astronomical images obtained with Faulkes Telescopes by Anne O’Leary, Ciara Quinn, Sharon McClure and Louise Jeffery: 2000 PH5, NGC6826, NGC6543, NN Ser, M9 The Faulkes Project Team: Faulkes Telescope North, Jupiter, Crab Nebula, Sunflower Galaxy Three projects were funded under the Nuffield Science Bursary scheme administered by Sentinus Background: False colour image of M9. Solar system Take a closer look at our neighbours in the universe. Are there any asteroids on collision course with Earth? The sequence below shows the motion of the near-earth asteroid 2000 PH5 across the sky. The picture to the right shows Jupiter with one of its moons. Binary stars Disappearing stars! What happens when two stars orbit each other? The sequence below shows the eclipse of NN Ser, a binary star. The graph shows data of its magnitude (brightness) against phase of orbit. Star clusters Find out about the colours of stars and stellar evolution. This is a false colour image of the globular cluster M9 and a graph of brightness against colour for a selection of the stars it contains. Planetary Nebulae Experiment with different filters and combine the images to give false colour pictures. The image on the left is NGC 6826 or the ‘blinking planetary’ and the nebula on the right is NGC 6543, also known as the ‘cat’s eye’ nebula. Other possibilities Other topics for study might include pulsating stars, stellar evolution, galaxies, cosmology. It’s your choice! Below are images of the Crab Nebula and the Sunflower galaxy. Second level students making observations with FTN at Armagh Observatory. Cosmic explosions Nova Sco 2004/2 appeared in the constellation of Scorpio on 6 August It is an explosion on the surface of a white dwarf star. As you can see from the pictures, what had been a very faint star, invisible on the left hand image quickly became the brightest object in this area of the sky. A close up of the nova is shown above right. Poster Design © 2004: Louise Jeffery, Armagh Observatory