This is a composite image showing a small region of the Chandra Deep Field North. Shown in blue is a deep image from the Chandra X-ray Observatory and in red is an image from the Multi-Element Radio Linked Interferometer Network (MERLIN) an array of radio telescopes based in Great Britain. An optical image from the Sloan Digital Sky Survey (SDSS) is shown in white, yellow and orange.
Imagine getting a picture of some random patch of the Earth. This picture has some features on it - maybe a mountain or a river or even a city - but from the altitude it was taken, you can't be exactly sure what's what. And then imagine if someone asked you to place it exactly where it should lie on the Earth. Really hard, right?
It's New Hampshire - USA
Well, of course, it gets a lot easier if someone were to give you the exact longitude and latitude. While this seems like an obvious thing to do, it's not so simple for astronomical images. When astronomers create their images for scientific purposes, these images retain certain coordinate information - like longitude and latitude - but for space. Unfortunately, when these images get processed further to make them attractive for the public, this information gets stripped out. In other words, we're back to having no clue where this image matches up with anything else.
Many of this week's blogs focused on that little-known telescope that's being invaded by a spaceship. In case you missed it, the telescope is called "Hubble" and the spaceship is our Space Shuttle Atlantis. Naturally, the astro-blogosphere took notice. In his "Dynamic of Cats" blog, Steinn Sigurdsson talks about the last pretty picture to come out of that workhorse instrument with the stubborn screw -- Wide Field/Planetary Camera 2.
Take a look at "The Bigger Picture," a blog produced by the Smithsonian Photography Initiative (SPI). It aims to present an inside look at the Smithsonian's photography collections and invites audiences to engage in an online discussion about photography's powerful impact on our world. We contributed a post on "Seeing the Invisible (part I)" that you might enjoy: http://blog.photography.si.edu/2009/05/11/seeing-the-invisible/
-Kim Arcand, CXC
(update on 06/01/09: Part II is also available: http://blog.photography.si.edu/2009/06/01/seeing-the-invisible-part-2/)
Activity from a supermassive black hole is responsible for the intriguing appearance of this galaxy, 3C305, located about 600 million light years away from Earth. The structures in red and light blue are X-ray and optical images from the Chandra X-ray Observatory and Hubble Space Telescope respectively. The optical data is from oxygen emission only, and therefore the full extent of the galaxy is not seen.
This week, the Space Shuttle Atlantis will return to the Hubble Space Telescope for a fifth and final time. The mission will bring the telescope new instruments, batteries, and gyroscopes that will extend its lifetime for hopefully several years or more.
This year marks the 10th anniversary that the Shuttle launched and deployed Chandra . There haven't been any visits since and none will ever take place. That's because Chandra was designed to be different than Hubble -- in more ways than just the type of radiation it detects.
An extremely deep Chandra X-ray Observatory image of a region near the center of our Galaxy has resolved a long-standing mystery about an X-ray glow along the plane of the Galaxy. The glow in the region covered by the Chandra image was discovered to be caused by hundreds of point-like X- ray sources, implying that the glow along the plane of the Galaxy is due to millions of such sources.
In this latest installment of our series, we sit down with Eli Bressert. Eli is responsible for making the Chandra images for the public that appear in press releases, on the website, in posters, etc. While we won't get into the technical details of how that gets done in this video blog, we did want to point out that this an important -- if lesser known -- job in the world of space science.
We've been publicizing and distributing Chandra results for nearly ten years now. One interesting trend we've watched over this time is how much things have changed in how people get their information. Back in the day, we would write a press release â€“ sometimes even printing on paper! â€“ and this would go to science reporters, who, in turn, would write articles for their newspapers, radio programs, or TV reports. The public would generally learn about our results by seeing them through these outlets.
This composite image shows the massive galaxy cluster MACSJ0717.5+3745 (MACSJ0717, for short), where four separate galaxy clusters have been involved in a collision, the first time such a phenomenon has been documented. Hot gas is shown in an image from NASA's Chandra X-ray Observatory and galaxies are shown in an optical image from NASA's Hubble Space Telescope. The hot gas is color-coded to show temperature, similar to a temperature map of the Earth given in a weather forecast.
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