- published: 01 Sep 2012
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Radio astronomy is a subfield of astronomy that studies celestial objects at radio frequencies. The initial detection of radio waves from an astronomical object was made in the 1930s, when Karl Jansky observed radiation coming from the Milky Way. Subsequent observations have identified a number of different sources of radio emission. These include stars and galaxies, as well as entirely new classes of objects, such as radio galaxies, quasars, pulsars, and masers. The discovery of the cosmic microwave background radiation, regarded as evidence for the Big Bang theory, was made through radio astronomy.
Radio astronomy is conducted using large radio antennas referred to as radio telescopes, that are either used singularly, or with multiple linked telescopes utilizing the techniques of radio interferometry and aperture synthesis. The use of interferometry allows radio astronomy to achieve high angular resolution, as the resolving power of an interferometer is set by the distance between its components, rather than the size of its components.
Radio Astronomy in Five Minutes
Understanding Radio Telescopes: Dr John Morgan
Astronomy 101: Introduction to Radio Astronomy
ANITA Lecture - Radio Astronomy and Interferometry Fundamentals – David Wilner
Radio Astronomy - History of Radio Waves, Microwaves and Infrared Waves
Hidden Visions (Radio Astronomy imaging techniques)
BAA Radio Astronomy Group
Basic Radio Telescope system components tabletop test
Radio astronomy: Something Kinda Awesome (SKA) - Presentation by Prof Peter Quinn
Mapping the Galaxy with Radio Astronomy
Anna practicing her Radio Astronomy talk, in preparation for ESP's Firestorm event: three hours of MIT students delivering five-minute talks on any topic of their choice.
http://astronomy.curtin.edu.au/ Curtin University "Super Fellow" John Morgan explains what how radio telescopes are an essential tool for looking into the mysteries of the universe. He talks about the awesome Square Kilometre Array, and the role of Curtin know-how in creating the associated Murchison Widefield Array. This lecture was held on Wednesday 27 August 2014. For more by Curtin Alumni: https://alumni.curtin.edu.au ICRAR: Discovering the hidden Universe through radio astronomy Web: http://www.icrar.org ICRAR's eNewsletter: http://www.icrar.org#subscribe ICRAR on Twitter: http://twitter.com/icrar ICRAR on Facebook: http://www.icrar.org/facebook Curtin Astronomy Club: http://www.facebook.com/curtinastronomyclub
Skynet University: http://skynet.unc.edu/introastro Use Our Telescopes From Anywhere! Astronomy 101: The Solar System Lesson 4: Telescopes Topic: Introduction to Radio Astronomy Next: Space-Based Telescopes (http://youtu.be/oUFTlt7LJB0) Previous: Radio Interferometers (http://youtu.be/7gja8u8kDi4) In Lesson 4, we explore the technologies that astronomers have developed, and continue to develop, to detect light from the universe, at both visible and invisible wavelengths. At visible and near-visible wavelengths, we compare and contrast reflecting and refracting telescope designs, as well as detectors, including spectrographs. We explore why astronomers build bigger and bigger telescopes, and consider both design and atmospheric limitations. We explore technologies that are bein...
Title: Radio Astronomy and Interferometry Fundamentals [Lecture 1/2] Speaker: David Wilner, Harvard-Smithsonian Center for Astrophysics (dwilner at cfa.harvard.edu) Date: 2pm (AEDT) Thursday 19th February 2015 Abstract: Radio astronomy uses observations at radio wavelengths to study celestial objects. This lecture will provide a brief introduction to radio astronomy, including a description of common emission mechanisms and radio telescopes, and why multiple telescopes are linked as interferometers to make high resolution “aperture synthesis” images (a technique recognized by the 1974 Nobel Prize in Physics). We will use pictures to develop intuition about the Fourier transform relationship between the sky brightness and visibility function that underlies radio interferometry. (A com...
Radio astronomy is a subfield of astronomy that studies celestial objects at radio frequencies. The initial detection of radio waves from an astronomical object was made in the 1930s, when Karl Jansky observed radiation coming from the Milky Way. Subsequent observations have identified a number of different sources of radio emission. These include stars and galaxies, as well as entirely new classes of objects, such as radio galaxies, quasars, pulsars, and masers. The discovery of the cosmic microwave background radiation, regarded as evidence for the Big Bang theory, was made through radio astronomy. Radio astronomy is conducted using large radio antennas referred to as radio telescopes, that are either used singularly, or with multiple linked telescopes utilizing the techniques of radio ...
18-minute documentary about the evolution of Australian radio astronomy from 1939 to when this movie was made in the early 1990s. Six dishes at Narrabri, one at Coonabarabran, and "The Dish" at Parkes can be hooked up together in such a way as to form a virtual mega-dish with an effective diameter of 300km. This is only possible by perfectly synchronizing the eight signals and by doing complex signal processing (mostly) in real time to filter out random noise. Without such correlation, background noise almost completely masks the weak signal of interest from the distant celestial object under study. Widely dispersed receiving antennas combining their signals in this way is called Very Long Baseline Interferometry, VLBI for short. Final scenes show how the detail available in images bu...
In this video, I'm testing the basic setup for my Radio Telescope: a 1420MHz feedhorn, a LNA gain chain with a passband filter, a IC-R7000 as downconverter and my Afedri SDR as a simple spectrum display on the IF output. I'm using a home built noise generator for the test. The output of the generator is VERY weak, around 12dB above thermal noise floor, but it works just fine with all the gain I have in my system. Sorry for the shakiness - this is shot the 'pragmatic' style, no rehearsal, no list of bullets I need to go through. Just me, my system, my iPhone. That's it! :) Enjoy
Telescopes have allowed us to look beyond our own solar system and make amazing discoveries. Now a new and exciting period approaches through the development of the world's largest telescope, the Square Kilometre Array (SKA). So what is the SKA and what does the remote desert of WA have to do with it? We took a cosmic journey back in time as Professor Peter Quinn discussed the power and potential of this new technology to discover and unravel the mysteries of the universe.
Produced by Danny Ben-David; created May 4, 2015 This video is designed to explore the surprising utility of radio astronomy as a tool for learning more about the universe. The video's vocabulary and content are tuned for high school students and up. Radio astronomy is a fascinating chunk of physics, because it manages to obtain impressive amounts of data with little more than a telescope which looks like a satellite dish and some math. It also ties serendipitously with discoveries such as dark matter, for reasons which will hopefully be clear within the video. This video is part of a group of videos produced by ES.333 (Production of Educational Videos). For more information on radio astronomy, see the National Radio Astronomy Observatory's website (https://public.nrao.edu/radioastronomy...
Ein Vortrag in englischer Sprache von Dott. Filippo Bradaschia Ph. D. am Tag der offenen Tür 2014 bei http://www.astroshop.de Radio telescopes for amateur astronomers and radio astronomy introduction. Filippo Bradaschia, founder of the italian company PrimaLuceLab, introduces the basics concepts of radio astronomy and presents the new innovation in remote sky monitoring technology: the SPIDER230 radio telescope. This is the first complete radio telescope designed to let user perform real radio astronomy, trouble free and with reliable performances. Spider230 radio telescope lets you record radio waves coming from space and convert them in radio-pictures! In his presentation, Filippo covers various aspects of radio astronomy: history, radio waves physics, radio sources in the Universe a...
Astronomy For Everyone is a TV series of monthly TV shows developed by members of the Ford Amateur Astronomy Club (FAAC) targeted to beginner and intermediate audiences as well as all amateur astronomers and sky observers. Please click SHOW MORE. The Ford Amateur Astronomy Club (FAAC) meets monthly in Dearborn, Michigan, provides public outreach sessions, holds night-time observing sessions (Star Parties) in and around South Eastern Michigan, has established observing locations with State and Local park authorities, we share mentoring and more. To see an overview of all of the Astronomy For Everyone programs, please visit: http://www.fordastronomyclub.com/AFE/AFE.html You are welcome to explore our website at: http://www.fordastronomyclub.com This episode covers Radio Ast...
Bob Wilson gave a talk on the history of radio astronomy at Bell Labs, Holmdel, NJ, at CfA 4 June 2015. Topics included the discovery of cosmic radio emission in the 1930s by Karl Jansky, as well as the discoveries of the Cosmic Microwave Background (CMB) and of interstellar carbon monoxide emission.
In this video from the OpenFabrics International Developer Workshop 2014, Dan Werthimer from the UC Berkeley Radio Astronomy group presents: Petaflop Radio Astronomy Signal Processing and the CASPER Collaboration. Learn more: http://insidehpc.com/video-gallery-openfabrics-developer-workshop-2014/
Dr Jasper Horrell (SKA, SA) gives an overview of some of the technical aspects relating to the Square Kilometer Array. Presented at the 2012 ASSA Symposium, SAAO, Cape Town, 2012 October 13. Visit the official symposium website for further details: http://symposium2012.assa.saao.ac.za