With thanks to Orpington AS Honor Wheeler.  Simon Dawes  Martin Crow  Sonia Rubie  Jim Burchell  Kevin Smith  Julian Tworek  David Sheehan & Son.

Slides:



Advertisements
Similar presentations
The York College Radio Telescope Ian OLeary, Tim Paglione, & Waynewright Joseph (York College, CUNY) Introduction Radio telescopes allow us to observe.
Advertisements

 A telescope collects light coming off an object, like the moon, planets, and stars.  It focuses the light and magnifies it, making the object appear.
Astrophysics /07 Technology Responsivity and Risk Mitigation Optimizing the Programmatic S/N Of Future Large Space Telescopes Dan Lester University.
Infrared Telescopes Andrea, Scott, and Martín Visit For 100’s of free powerpoints.
_______________________________________________________________________________ 1400s – 1600s Age of Explorers 1400s – 1600s 1600 – 1700s
The Universe. The Big Bang Theory  Georges Lemaître was the scientist who proposed this theory  He proposed that the universe started as a singularity,
The Dish: Fun things to notice in the movie Parkes tracking Apollo 11 The 6 day old Moon as it appeared from Parkes on 21 July Donna Kubik.
Radio Telescopes Large metal dish acts as a mirror for radio waves. Radio receiver at prime focus. Surface accuracy not so important, so easy to make.
Honors Ch Pg Almost everything we know about the universe (space) comes by studying light from distant sources. Light from what?
Observing the Cosmic Microwave Background 1. Penzias and Wilson with their Horn Antenna. Penzias and Wilson were astronomers, from Bell Labs, who built.
Navigation using pulsars ASTRONOMY AND SPACE SCIENCE George Hobbs Nov 2014.
Ian Cintron and Rebecca Sekban
WHAT ASTRONOMERS LEARN ABOUT THE ELECTROMAGNETIC SPECTRUM.
How do we introduce and demonstrate Radio Astronomy at Tamke-Allan Observatory? Tamke Allan Observatory is located in Rockwood Tennessee and is operated.
Ask the Scientists Questions for Dr. Butner Star Formation 1/29/11.
 Celestial Sphere  Imagine a sphere that surrounds our planet in which all the stars are attached. This sphere is allowed to rotate freely around the.
Unit E: Space Exploration. Heliocentric (Sun-centered) vs. Geocentric (Earth-centered) HeliocentricGeocentric.
Craig Lawrie Advisor: Dr. John Ruhl Abstract Software is developed for the detection of galaxy clusters in data gathered by the South Pole Telescope (SPT).
Warm up question  1. How do you think astronomers can see planets, stars, and galaxies that are so far away?
Telescope Technologies
Astronomy 1020-H Stellar Astronomy Spring_2015 Day-22.
Want to be an astronomer?. A 4000 year old observatory, built by/for astronomers. What is it?
Radio Astronomy: Jansky. Radio Astronomy: Reber Radio Astronomy Jan Oort Hendrik van de Hulst.
Image taken using radiowaves, why can’t we use visible light? Approx diameter of the milky way is 30KPc!
Telescopes Notes.
ELECTROMAGENTIC RADIATION. ELECTROMAGNETIC RADIATION IS A FORM OF ENERGY. IT CAN BEHAVE AS PARTICLES OR WAVES. SOMETIMES, WE USE THE TERM “LIGHT” WHEN.
In the Beginning 1)The Early Universe 2)SETI December 2, 2002 Final Exam will be held in Ruby Diamond Auditorium NOTE THIS!!! not UPL Dec. 11, am-noon.
Non-Optical Telescopes
The theory of the universe. Expanding of our universe In the 1920s, astronomers had the technology to see more Celestial bodies with advance telescope.
Exploring the Universe
Warm-Up Pick up a Big Bang Theory Reading from the front table
The Quiet Skies Project and the IYA Astronomers need dark skies to see the stars, but did you know they also need quiet skies? Learn more about radio astronomy,
Why look at different frequencies of light? Cooler objects are only visible at long wavelengths: radio, microwaves, IR. Hotter objects are only visible.
Looking into space P1b 7.3 What can we see in space?  NASA SLIDE 1.
Spitzer Space Telescope
Radio Astronomy Observing With Your Ears Multi-Wave Centaurus A Galaxy.
Radio Telescopes. Angular resolution Distant objects are separated by an angle. –Degrees, arc-minutes, arc-seconds Angular resolution refers to the ability.
Excursion to Wynnum park By Eh San. At 9:30am, we met other students at South Bank bus stop.
_______________________________________________________________________________ 1400s – 1600s Age of Explorers 1400s – 1600s 1600 – 1700s
Is this photo shopped?. SPACE EXPLORATION UNIT Topic 4 – Bigger, Smarter Telescopes (pages )
We are going to the Intrepid Sea, Air & Space Museum for Family Astronomy Night.
From the Greek:tele = 'far' and skopein = 'to look or see'; teleskopos = 'far-seeing'
P1 - Foundation Part 3 – Space Put these in order of smallest to largest. Star, Galaxy, Solar system, Moon, Universe, Planet.
THE BIG BANG THEORY. HOW IT ALL BEGAN Scientists hypothesize that approximately 13.7 billion years ago, a rapid expansion created the universe, producing.
Wilkinson Microwave Anisotropy Probe (WMAP) By Susan Creager April 20, 2006.
First result with PAF on a big single-dish radio telescope X. Deng, A. Chippendale, S. Johnston, G. Hobbs, D. George, R. Karuppusamy ASTRONOMY AND SPACE.
Photo: Anthony Holloway Public Outreach and Engagement at Jodrell Bank Naomi Smith Events and Participation Programme Manager Jodrell Bank Discovery Centre.
Module 3 – Nautical Science
Microwave/Submillimeter Astronomy
Jodrell Bank Observatory.
April 21, 2016, 7:30pm Hanson Hall, Room 102, Augustana College
Objective Solve problems involving angles of elevation and angles of depression.
Mr. Magner DHSHS Earth Science
LIFE Out There?.
Looking into space P1b 7.3 What can we see in space?  NASA.
Tools of Astronomy Part 2 Notes
BIG BANG THEORY.
LinkedIn Training.
Diffraction and Resolution
Diffraction and Resolution
The Hintze Lecture Series Professor Robert Kennicutt
The distance on the map or drawing or the actual distance.
Probing Metallicity across the Galactic Disk – Dana S. Balser
Author: stefan huber Team Serbia 2
Objective Solve problems involving angles of elevation and angles of depression.
÷ 5 = 29 How many 5s are there in 1? Great!
÷ 2 = 24 How many 2s are there in 4?
BIG BANG THEORY.
P3 1.8 SATELLITES Learning objectives Be able to explain:
I went to the park two weeks _______.
Presentation transcript:

With thanks to Orpington AS Honor Wheeler

 Simon Dawes  Martin Crow  Sonia Rubie  Jim Burchell  Kevin Smith  Julian Tworek  David Sheehan & Son  Janice McClean  Honor Wheeler Members who fell asleep on the coach?…all members except one! Photos/Video Pending!

 06:00 Left Orpington Train Station  11:00 Arrive at Jodrell Bank (we actually arrived at 11:10)  11:15 Free time to explore the Planet Pavilion, Space Pavilion, Telescope and Planet Pathway, Gardens, Cafe and Shop  12:15 – 13:00 Talk in the Space Pavilion (2 groups) at which Kevin Smith asks a very interesting question regarding the Cosmic Microwave Background or the CMB.  13:45 Free time to explore the Planet Pavilion, Space Pavilion, Telescope and Planet Pathway, Gardens, Cafe and Shop  16:30 Depart  21:30 Arrive back at Orpington Train Station

1. Car park 2. Planet Pavilion 3. Galaxy Gardens 4. Space Pavilion 5. Whispering Dishes 6. The Lovell Telescope.

ABOVE: THE LOVELL TELESCOPE CRYOGENIC RECEIVER BELOW: AT 5 METERS IN DIAMETER, THE JODRELL BANK ORRERY IS THOUGHT TO BE THE LARGEST IN THE WORLD

Designed by TV Gardener Chris Beardshaw and Jodrell Astronomer Dr Tim O’Brien

LEFT: A LIVE FEED FROM THE LOVELL TELESCOPE WITH INFORMATION ON AZIMUTH AND ELEVATION AND A SCREEN SHOWING RECENT OBSERVATIONS. ABOVE: A LIVE TELESCOPE SIGNAL WITH A PRINT OUT YOU CAN KEEP. RIGHT: A MODEL IN WOOD

Left: The Mark I in ft (76M) in Diameter. Right: The Mark I in 2013 It was renamed the Lovell Radio Telescope in1987

A great view while having lunch!

RIGHT: THE MARK II TELESCOPE WHICH WAS COMPLETED IN M IN DIAMETER INSET PHOTO: IAN MORISON LEFT: THE 42FT (13M) TELESCOPE