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Tools of Astronomy
Tools of Astronomy

... Spectrum: the different colors and wavelengths of light. ...
Astronomy review - Petal School District
Astronomy review - Petal School District

... Infrared Telescopes • Can be on the ground or above atmosphere. • Used to measure temperature of celestial objects, their composition and to locate planets around other stars. Exoplanets Infrared telescopes on Mauna Lea in Hawaii ...
Solar space instrumentations and techniques
Solar space instrumentations and techniques

... percentage of photons that are actually detected is known as the Quantum Efficiency (QE). • Wavelength range: CCDs can have a wide wavelength range ranging from about 400nm (blue) to about 1050nm (Infra-red) with a peak sensitivity at around 700nm. However, using a process known as backthinning, it ...
File
File

... What are Telescopes? A telescope is an instrument designed for the observation of remote objects by the collection of Light  A telescope’s diameter is measured in inches, meters or centimeters  Eg: A 6inch Telescope is bigger than a 4inch Telescope because it can collect more light ...
Astronomy PowerPoint - Petal School District
Astronomy PowerPoint - Petal School District

... large stars. Can be seen without a telescope. Neutron star: extremely small, dense leftovers from a supernova supernovae shrink into neutron stars ...
Telescopes January 31 −
Telescopes January 31 −

... • With tip-tilt correction • Detail become visible • Fainter stars become visible ...
Stars and galaxies Intro
Stars and galaxies Intro

... to focus X-rays and produce an image • The first X-ray telescopes were used to observe the sun. FYI: The Chandra X-ray Observatory ...
SPACE EXPLORATION UNIT
SPACE EXPLORATION UNIT

... Using computers to combine images from >1 telescope Acts like telescope the size of the distance between telescopes (greatly improves resolving power) The Very Large Telescope (VLT) is operated by the European Southern Observatory in Chile ...
pptx
pptx

... The Square Kilometer Array will be an array of thousands of radio dishes with a total collecting area of 1 km2 and a baseline of 3000 km. It will be built in Australia and Africa and will be 100 times more sensitive than the VLA. ...
Chapters 5,12
Chapters 5,12

... Advantages of reflecting telescopes include the fact that the light does not have to pass through any glass, there is no chromatic abberation, they can be made larger, and their weight is easier to support. ...
Everything YOU wanted to know about Teaching High School
Everything YOU wanted to know about Teaching High School

... http://stardate.org/nightsky/bguide/view.html  Important points: ...
Tools of Modern Astronomy:
Tools of Modern Astronomy:

... Read pages 784-790 in the textbook to find the answers to the question below. Use the back of this page or a sheet of binder paper if you need more room for the answers. 1. What did enslaved African Americans follow as they moved north to the Free States? What are constellations? 2. What are stars? ...
PHY2083 ASTRONOMY
PHY2083 ASTRONOMY

... • An advantage of working at such long λ  is that small deviations from an ideal parabolic shape are not crucial. ...
Lecture 12 - Empyrean Quest Publishers
Lecture 12 - Empyrean Quest Publishers

... Reflecting or Newtonian telescope (reflector): A large curved objective mirror focuses an image, a small eyepiece lens magnifies it. The image is inverted. Refracting telescope (refractor): A large objective lens (usually converging) focuses an image and a small eyepiece lens magnifies it. The image ...
vision technology reaches for the stars
vision technology reaches for the stars

... You’ve probably heard of the Hubble Telescope, which is world-famous for its ability to see billions of light years into space. But you might not know about its next-generation successor. The James Webb Space Telescope, planned to launch in 2018, will boast a magnifying power 100 times that of the H ...
NASA Missions
NASA Missions

... Launched in 1990. Has a huge optical telescope, a wide field camera, an infrared spectrometer and a spectrograph ...
Using the Electromagnetic Spectrum
Using the Electromagnetic Spectrum

... from B&W images. The images were recorded on 2 types of photographic plates, one sensitive to red light and the other to blue, and then digitized. Credit: David De ...
Telescopes - ESS I. Uses for telescopes-
Telescopes - ESS I. Uses for telescopes-

... i. Detects the smallest waves Electromagnetic Spectrum- know the order from long to short wavelength a. Radioi. Longest wavelength b. Microwavei. used by cell phones c. Radari. good for tracking objects (speed, weather…) ...
Document
Document

... • The Sun is a million times larger than the Earth. • The Moon is a fourth the size of the Earth. • The distance from the Earth determines their ANGULAR SIZE. ...
Astronomy Tools
Astronomy Tools

...  Video clip links are not working. You will see them at some point during class.  Other underlined links work and you may explore them. ...
THE MISSION THE SCIENCE BEHIND CHEOPS ROLE OF ADMATIS
THE MISSION THE SCIENCE BEHIND CHEOPS ROLE OF ADMATIS

... be launched into low Earth orbit to measure transits of Exo-planets. CHEOPS is the first Small mission from ESA and was selected in October 2012 with a launch target for 2017. ESA is the Mission Architect and in charge of the spacecraft development and launcher procurement. The Member States contrib ...
fors_office2007 - Departament d`Astronomia i Meteorologia
fors_office2007 - Departament d`Astronomia i Meteorologia

Mega Telescopes of the 21st Century
Mega Telescopes of the 21st Century

... Credit: Clip from European Southern Observatory Press Release ...
No Slide Title
No Slide Title

InStrumentS
InStrumentS

... the Great Observatories to make astronomical studies over many different wavelengths (visible, gamma rays, X-rays and infrared) to provide a greater understanding of the universe. ...
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XMM-Newton



The XMM-Newton, also known as the X-ray Multi-Mirror Mission and the High Throughput X-ray Spectroscopy Mission, is an orbiting X-ray observatory launched by ESA in December 1999 on an Ariane 5 rocket. It is named in honor of Sir Isaac Newton. The telescope was placed in a very eccentric 48 hour elliptical orbit at 40°; at its apogee it is nearly 114,000 kilometres (71,000 mi) from Earth, while the perigee is only 7,000 kilometres (4,300 mi).
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