he wasn't even looking at me and he found me

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@astronomystuff
A Nova erupts in the constellation Centaurus and is visible to the naked eye!
Nova Centauri 2013 was found by John Seach from Australia on December 2, 2013.
Astronomy Picture of the Day: http://apod.nasa.gov/apod/ap131207.html
A Laser Strike at the Galactic Center
Discarded rockets of the Apollo 11 voyage. Found at the bottom of the Atlantic Ocean
ISON update: It (probably) didn’t (completely) disintegrate
As ISON approached the Sun, astronomers – both professional and amateur – from all over the world got very excited. ISON started to flare up and get very bright, and then it vanished.
The comet started to dim and “smear” as it entered the occulter guarding NASA’s Solar and Heliospheric Observatory’s (SOHO) cameras, the Solar Dynamic Observatory caught some glimpses of “bright pixels,” but it wasn’t an astonishingly bright event. The early speculation was that ISON had completely disintegrated as it passed the Sun.
But, that’s not where the story ends…
As Phil Plait says, “It’s still possible that the initial reports of ISON’s death were somewhat exaggerated.” New images from SOHO show that ISON might still be fighting, just barely.
The “Comet of the Century” has had a lot of hype over the last year and a half, since it’s discovery in 2012. ISON is a new visitor to the inner solar system and it was set to pass within 1.2-million kilometers (730,000 miles) of the Sun. The potential to study both the origins of the Solar System and the structure of the Sun’s corona – all in the same event – was to good to pass up.
As I stated before, as the comet approached the Sun, something happened and ISON started to smear. It looked like the comet fizzed out before it even got started. Even if ISON disintegrated, scientists were suppose to see debris left over (which would be better for professional study, though not so good for amateur astronomy), but everything, the comet, the tail, everything, just vanished. Dean Pesnell, a project scientist with SDO summarized it most eloquently by saying “I’d like to know what happened to our half a mile of material that was going around the sun. Now’ it’s broken up and I didn’t see anything.”
Currently, material has reemerged from the other side of the Sun’s Corona. This is either a continuation of the tail that ISON left behind, or the comet itself. Current speculation is the dust that we see is simply dust, orbiting exactly as it should. The nucleus is probably lost.
So, what did we learn from this comet?
We learned a lot about the original conditions of the solar system.
Because the comet fizzed out so spectacularly, we learned that our models for comets and their composition has some serious problems; we need to figure out what those are so we can fix them.
As with all good celestial events, we are also left with a mystery… What happened to ISON while it was in SOHO’s occulter and invisible to SDO’s vision? As always, there is more than one possible answer to this mystery…
**UPDATE: 11/28 22:10 Eastern** It looks like part of ISON might have survived. We are seeing some brightening of ISON as it leaves the Sun. According to Phil Plait, comet astronomers are baffled and he is refusing to predict the comet’s actions any further. It keeps brightening, smearing, and vanishing without warning or a discernible pattern. We’ll keep you informed as the event continues to unfold.
Image credit: NASA/SOHO
Carl Sagan
Receiving the Galactic Beam
Image Credit: Wayne England
Gif collection from my latest video. See it here: http://www.youtube.com/watch?v=gPw8C1fID80
Witch’s Head Nebula,Wired Space Photo of the Day. Image: NASA/JPL-Caltech [high-resolution]
High noon analemna over Azerbaijan
Is the Sun always straight up at noontime? No. For example, the Sun never appears directly overhead from locations well north or south of the Earth’s equator. Conversely, there is always a place on Earth where the Sun will appear at zenith at noon — for example on the equator during an equinox. Turning the problem around, however, as in finding where the Sun actually appears to be at high noon, is as easy as waiting for midday, pointing your camera up, and taking a picture. If you do this often enough, you find that as the days march by, the Sun slowly traces out a figure eight on the sky. Pictured above is one such high noon analemma – a series of pictures always taken at exactly noontime over the course of a year. The above fisheye image, accumulated mostly during 2012, also shows some buildings and trees of Baku, Azerbaijan around the edges.
Image credit & copyright: Tunç Tezel (TWAN)
A special spiral galaxy for over 200,000 Facebook fans
This Hubble Picture of the Week is dedicated to the over 200,000 Facebook fans of ESA/Hubble, who share our passion for the NASA/ESA Hubble Space Telescope and the discoveries it brings. We thank you for staying in touch with us!
The image, captured by the NASA/ESA Hubble Space Telescope, shows part of NGC 3621, an unusual spiral galaxy located over 20 million light-years away in the constellation of Hydra (The Water Snake).
The small, bright nucleus on the right of the image does not have the significant bulge of older stars that is common in spiral galaxies, marking NGC 3621 as a “pure-disc” galaxy. Many luminous clumps of blue young stars are scattered along the loose spiral arms, which are partially obscured by the dark dust lanes snaking across the frame. This galaxy is very useful for astronomers; some of its brightest stars can be used to estimate extragalactic distances, allowing us to measure the vast scale of the Universe. - ESA/Hubble & NASA
Desert Sky
Photograph courtesy Thomas Sullivan, APOY/Royal Observatory
Milky Way and Mashed Potato Mountain
Milky Way Reflections
Photograph courtesy Luc Perrot, APOY/Royal Observatory
M78: Stardust and Starlight Interstellar dust clouds and bright nebulae abound in the fertile constellation of Orion. One of the brightest, M78, is just left of center in this colorful telescopic view, covering an area north of Orion’s belt. At a distance of about 1,500 light-years, the bluish nebula itself is about 5 light-years across. Its blue tint is due to dust preferentially reflecting the blue light of hot, young stars in the region. Dark dust lanes and other nebulae can easily be traced through this gorgeous skyscape. The scene also includes the remarkable McNeil’s Nebula — a newly recognized nebula associated with the formation of a sun-like star, and the telltale reddish glow of many Herbig- Haro objects, energetic jets from stars in the process of formation. Image Credit & Copyright: Tony Hallas