24 Hours In The Life Of An Astronomer

Posted in Astronomy on November 5th, 2010 by admin

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ESOcast 4: 24 hours in the life of an ESO astronomer.

Have you ever wondered what it must be like to be an astronomer? In this fourth episode of the ESOcast, Dr. J takes us behind the scenes at ESOs Very Large Telescope in Chile to show us what a day in the life of an ESO staff astronomer is like.


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The countdown for an exciting night with an observation run at the world’s most advanced optical telescope, the ESO Very Large Telescope (VLT), has begun …

In this ESOcast episode, were going to follow a day in the life of Dieter Nürnberger. Dieter is a staff astronomer at ESO. His job is to support those scientists that have managed to get observing time on ESOs Very Large Telescope at Paranal Observatory in Chile. Dieter spends most of his working days helping the successful few to make ground-breaking discoveries.

Dieter Nürnberger is on his way to meet the visiting scientists to team up for the night to come. The three have been observing together for several nights, today is their final evening and they are keen to get started. Over dinner they discuss plans for the night ahead.

Well before sunset they leave the Residencia and drive up the desert road to the building housing the VLT control room. At the control building they prepare the observations and check the set up of the telescope. Observing time on these great telescopes is precious and delays must be avoided at all costs.

Like a pilot checking his plane before departure, Dieter goes through a detailed check of his instrument, while the telescope operator does the same for the giant telescope. The astronomers have travelled far for a glorious view of the Universe, and here a glorious view of the sunset is included for free! As usual at Paranal, the conditions are perfect and Dieter and the visiting astronomers return with high expectations.

Read more: http://www.eso.org/public/videos/ESOCAST4/ESOCAST4.pdf

ESOcast is produced by ESO, the European Southern Observatory. ESO, the European Southern Observatory, is the pre-eminent intergovernmental science and technology organisation in Astronomy designing, constructing and operating the worlds most advanced ground-based Telescopes.

• http://www.eso.org/
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Duration : 0:6:0

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Radio Telescopes

Posted in Telescopes on July 15th, 2010 by admin

The Sun and stars emits radio waves — not just visible and infrared light. In the 1930s, Karl Jansky built the first devise to “listen” to the sun, collecting radio waves from far off stars and focusing them onto a detector. This invention provided astronomers with a completely different view of the Universe — prompting the discovery of radio stars, quasars, and black holes.

This video features a model of the Algonquin Radio Observatory (ARO), located in Ontario’s Algonquin Provincial Park. In 1968, astronomers combined signals from the ARO with those from the Dominion Astrophysical Radio Observatory in Penticton, British Columbia forming a new instrument called a Long Baseline Interferometer.

To learn more about Astronomy and Telescopes, visit the Canada Science and Technology Museum.

http://www.sciencetech.technomuses.ca/

Duration : 0:3:7

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NASA Astronomy Pictures Of The Day [Week 5/2010]

Posted in Astronomy on March 13th, 2010 by admin

NASA Astronomy Pictures Of The Day [Week 5/2010]


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► Stardust in Perseus
This cosmic expanse of dust, gas, and stars covers close to three degrees on the sky in the heroic constellation Perseus. Right of center in the gorgeous skyscape is the dusty blue reflection nebula NGC 1333, about 1,000 light-years away. At that estimated distance, the field of view is about 50 light-years across. Next to NGC 1333 is the reddish glow of shocked hydrogen gas created by energetic jets and winds from stars in the process of formation.
• http://antwrp.gsfc.nasa.gov/apod/ap100204.html

► Shepherd Moon Prometheus from Cassini
Another moon of Saturn has been imaged in detail by the Cassini spacecraft. Visible in an unprocessed image from 36,000 kilometers away, Prometheus’ 100-km long surface was revealed to have an interesting system of bulges, ridges, and craters. Cassini’s next major targeted flyby is of the moon Rhea.
• http://antwrp.gsfc.nasa.gov/apod/ap100201.html

► Hong Kong Sky
This remarkable scene combines multiple exposures recorded from a waterside perspective in Hong Kong, China. It follows a young crescent Moon, with brilliant planet Jupiter to its left, as they set together in the western sky. Their two luminous trails are faintly paralleled by trails of background stars.
• http://antwrp.gsfc.nasa.gov/apod/ap100206.html

► The Einstein Cross Gravitational Lens
Most galaxies have a single nucleus — does this galaxy have four? The strange answer leads astronomers to conclude that the nucleus of the surrounding galaxy is not even visible in this image. The central cloverleaf is rather light emitted from a background quasar. The gravitational field of the visible foreground galaxy breaks light from this distant quasar into four distinct images. The quasar must be properly aligned behind the center of a massive galaxy for a mirage like this to be evident. The general effect is known as gravitational lensing, and this specific case is known as the Einstein Cross.
• http://antwrp.gsfc.nasa.gov/apod/astropix.html

► Mars and a Colorful Lunar Fog Bow
Even from the top of a volcanic crater, this vista was unusual. For one reason, Mars (on the far upper left) was dazzlingly bright when this picture was taken, as it was nearing its brightest time of the entire year.
• http://antwrp.gsfc.nasa.gov/apod/ap100202.html

► P/2010 A2: Unusual Asteroid Tail Implies Powerful Collision
First discovered on ground based LINEAR images, the object appeared unusual enough to investigate further with the Hubble Space Telescope. What Hubble saw indicates that P/2010 A2 is unlike any object ever seen before. At first glance, the object appears to have the tail of a comet. Close inspection, however, shows a 140-meter nucleus offset from the tail center, very unusual structure near the nucleus, and no discernable gas in the tail. Knowing that the object orbits in the asteroid belt between Mars and Jupiter, a preliminary hypothesis that appears to explain all of the known clues is that P/2010 A2 is the debris left over from a recent collision between two small asteroids. If true, the collision likely occurred at over 15,000 kilometers per hour — five times the speed of a rifle bullet — and liberated energy in excess of a nuclear bomb.
• http://antwrp.gsfc.nasa.gov/apod/ap100203.html

► Dust Storm on Mars
It’s spring for the northern hemisphere of Mars and spring on Mars usually means dust storms. So the dramatic brown swath of dust (top) marking the otherwise white north polar cap in this picture of the Red Planet is not really surprising.
• http://antwrp.gsfc.nasa.gov/apod/ap100205.html

► The Colors of IC 1795
This colorful cosmic portrait features glowing gas and obscuring dust clouds in IC 1795, a star forming region in the northern constellation Cassiopeia. The nebula’s colors were created by adopting the Hubble false-color palette for mapping narrow emission from oxygen, hydrogen, and sulfur atoms to blue, green and red colors, and further blending the data with images of the region recorded through broadband filters.
• http://apod.nasa.gov/apod/ap091210.html

► The International Space Station Over the Horizon
The STS-129 crew of the Space Shuttle Atlantis undocked from the International Space Station (ISS) and returned to Earth. As the shuttle departed the space station, they took the above image. The ISS continues to be home for five astronauts of Expedition 21.
• http://apod.nasa.gov/apod/ap091207.html
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Duration : 0:3:29

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Hubble Space Telescope Directly Observes Exoplanet

Posted in Telescopes on March 6th, 2010 by admin

Hubblecast 22: Hubble Space Telescope Directly Observes Exoplanet Orbiting Fomalhaut.

The NASA/ESA Hubble Space Telescope has discovered an extrasolar planet, for the first time using direct visible-light imaging. The strange world is far-flung from its parent star, is surrounded by a colossal belt of gas and dust, and may even have rings more impressive than Saturn’s.


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Credit:
- ESA/Hubble (M. Kornmesser & L. L. Christensen)
- Visual design & Editing: Martin Kornmesser
- Animations: Martin Kornmesser & Luis Calçada
- Web Hosting: Leibniz-Rechenzentrum (LRZ)
- Web Technical Support: Lars Holm Nielsen & Raquel Yumi Shida
- Written by: Lee Pullen & Lars Lindberg Christensen
- Host: Dr. J
- Narration: Bob Fosbury
- Cinematography: Peter Rixner
- Music: movetwo
- Footage and photos: A. Fujii, Digitized Sky Survey 2, NASA, ESA, and P. Kalas (University of California, Berkeley). Acknowledgment: Davide De Martin (ESA/Hubble)
- Directed by: Lars Lindberg Christensen

Dr. J is a German astronomer at the ESO. His scientific interests are in cosmology, particularly on galaxy evolution and quasars. Dr. J’s real name is Joe Liske and he has a PhD in Astronomy.

Hubble European Space Agency Information Centre
Garching/Munich, Germany
• http://www.eso.org
• http://www.spacetelescope.org
• http://hubblesite.org
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Duration : 0:5:2

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Telescope Basics (Reflector, Refractor, Schmidt-Cassegrain)

Posted in Telescopes on February 20th, 2010 by admin

Understanding Reflector, Refractor, and Schmidt-Cassegrain Telescopes, Alt-Azimuth and Equatorial mounts, benefits, and comparisons.

Duration : 0:7:39

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