Supernova Imaged by Hubble Telescope 163
Delta Vel writes "First discovered by a Japanese amateur astronomer on July 31, this Type II supernova was imaged by Hubble on August 17th. The newly named SN 2004 dj, the closest supernova to be observed in over ten years, is about 11 million light-years away in the spiral galaxy NGC 2403. Looks like they goofed in one of the images, though--the arrow points to a different bright spot on the before-and-after image than it does on the main and annotated images." Reader Saeed al-Sahaf writes "Today, astronauts Gennady Padalka and Mike Fincke popped open the hatch on the Russian side of the ISS spacecraft and quickly stepped through the fourth and final spacewalk of their six-month mission. Their mission? Install three antennas and replace a 2-foot-square Russian pump panel. But of course, because it isn't a part or our Mission to Mars, it is still too dangerous work on the Hubble Telescope, which after all, is only used for science."
Awesome (Score:5, Funny)
Re:Awesome (Score:1)
That's insane!
Do you have any idea how long it will take for traffic to go up to the space station and back down again?
*whistles*
Re:Awesome (Score:2)
Re:Awesome (Score:2)
Re:Awesome (Score:4, Informative)
It's all there, your browser just doesn't display it.
Try This [216.239.57.104].
Re:Awesome (Score:1)
Re:Awesome (Score:1)
In other news... (Score:5, Funny)
Re:In other news... (Score:2)
The idea of RIAA paying to send lawyers in space is somewhat... funny
Re:In other news... (Score:1)
Re:In other news... (Score:2)
Re:In other news... (Score:1)
Neato (Score:1, Interesting)
PS. No, I didn't rtfa.
Re:Neato (Score:4, Informative)
Who said they could? Lol.
But seriously, I know the dynamic range of CCD's used telescopes can be at least 16 bits grayscale. To display them on a monitor/lcd you have to do some conversion. What basically look like very faint distinctions of shades of grey appear to be a detailed, crisp, starry picture of the sky to us (after conversion by the computer).
End result: They know that this white spec is ~100 times brighter than the white spec next to it, by looking at the raw intensity values observed from the camera.
p.s. Yes, I know that is a color image -- they probably took 3 grayscale images with red,green,and blue filters.
Re:Neato (Score:2, Informative)
Bingo! Hubble takes grayscale pictures and these gets converted to false colour later. The reason? Hubble doesn't shoot with real colour because it would be useless for science. Instead, it uses some filters to pick up radiation from some certaion ionized atoms, hence HII (Hydrogen two) reference in the annoted picture. Now, looking at this picture, certain hue (like red) can represent HII. As a
Re:Neato (Score:3, Interesting)
Re:Neato (Score:2)
Typically there are four, resulting in the four (or 2 depending on how you count) perpendicular diffraction spikes. Many designs exist, some that spread the diffracted light so that it is not obvious to the eye.
I don't think diffraction spikes are useful, other than making bright stars look more 'starry'.
Re:Neato (Score:2)
Re:Neato (Score:5, Informative)
But even if you weren't sure, the "wavelength/frequency" of the light is INCREDIBLY different. A good eye can tell the difference between all the different sorts of supernova spectra in seconds.
Educated guess, my ass.
By the way, I'm one of Filippenko's supernova checkers. Hi everybody!
-Harrison
Re:Neato (Score:2)
Our public schools haven't done a particularly good job of explaining the fascinating detective work required to tease out answers
Re:Neato (Score:4, Interesting)
Sure. Stars are mostly Hydrogen and Helium. A supernova is cascading fusion reaction, and they produce every naturally occuring element in the universe. The spectra reflect this.
I won't google a graph for you, but I'm sure it would only take a few seconds.
Re:Neato (Score:4, Interesting)
Re:Neato (Score:1)
The other thing I wonder is will we be able to see the light echo of this supernova, it would be pretty great to see the surrounding layers of gas.
Re:Neato (Score:3, Informative)
Re:Neato (Score:1)
Re:Neato (Score:3, Informative)
-aiabx
Re:Neato (Score:2)
In another response, someone noted that the nutrinos for SN1987a arrived before the light... though 'C' is the limit of at which things in this universe may travel, folks have to remember that light only travels at 'C' in a perfect vacuum. The s
Re:Neato (Score:3, Informative)
Re:Neato (Score:2)
jk
Re:Neato (Score:2)
That's probably a star in our galaxy
Re:Neato (Score:3, Informative)
Yeah, that's a star. About 11 million light years closer than the supernova. Just to give a hint of a relative brightness...
How exactly can they tell the difference?
Well, dunno, if you don't want to hear anything about doppler and red shift or wavelength, how about the fact that the bright star has been there for as long as we've been looking whereas the supernova just popped to brilliance a few months ago from a location that d
Re:Neato (Score:2)
Must be a slow news day (Score:5, Funny)
I want to know if it will be visible with the... (Score:2, Interesting)
Not visible to the naked eye (Score:1, Informative)
If it were in our own galaxy then it would have a chance of being visible.
Re:I want to know if it will be visible with the.. (Score:3, Interesting)
Re:I want to know if it will be visible with the.. (Score:1, Informative)
If it really appeared as bright as the sun, but was coming from a star-sized pinpoint in the sky, that might be a little hard on the retinas if you looked at it directly.
Now, in the event you notice that the entire upper atmosphere has been turned into an orange smog by the gamma rays, then you know that the supernova was really too close for comfort. In that case,
Re:I want to know if it will be visible with the.. (Score:2)
I wonder what the residents of that now-ex-solar system thought? And perhaps that'd be a good section of the sky to look for messages in? Perhaps they saw it coming, and could only save "themselves" by broadcasting their technology to any civilization that could make use of it.
Re:I want to know if it will be visible with the.. (Score:3, Insightful)
We'd have to go FTL a loooong way to look for any signal.
Re:I want to know if it will be visible with the.. (Score:2, Informative)
If they weren't native, then probably they had the means of travelling between star systems, no contest, it's just like a huge Florida evacuation, only 14 million times larger. :-)
Re:I want to know if it will be visible with the.. (Score:1)
Venus can cast shadows and it is pretty bright but it doesn't make it as it were day. Neither full mooon, which is the brightest object in the sky by far but it makes the terrain visible pretty easily.
Re:I want to know if it will be visible with the.. (Score:5, Informative)
Type Ia supernovae take about a month to reach their peak brightness. While this is a Type II, a different class of explosion, I think the timescale is comparable. Accoring to this page [freeuk.com] the supernova had an apparent visual magnitude of 11.3 in early August. This is a factor of 100 dimmer than the naked eye can see under the best conditions (magnitude 6 is the dimmest the unaided eye can see).
If you're unsure of why a higher number means a dimmer object, or just want more information, czech out the Wikipedia entry on visual magnitudes [wikipedia.org].
By the way, the last supernova that was visible to the naked eye was SN1987A [google.com] in the Large Magellanic Cloud.
Re:I want to know if it will be visible with the.. (Score:2)
-aiabx
Nice Editorializing... (Score:2, Offtopic)
Re:Nice Editorializing... (Score:3, Informative)
When first sighted... (Score:3, Funny)
Article on UC Berkeley's website (Score:5, Informative)
conspiracy alert! (Score:2, Funny)
AHA! CONSPIRACY! This also means we didn't actually land on the moon, and lends credence to my little-green-men-at-roswell theory. Not the alien autopsy though, that was just nonsense.
Re:conspiracy alert! (Score:5, Insightful)
Re:conspiracy alert! (Score:2, Funny)
Re:conspiracy alert! (Score:1)
Mmm, explosions (Score:1)
I'm kind of disappointed though. I was hoping it would be background worthy. [img21.exs.cx]
Re:Mmm, explosions (Score:1)
The image you linked to is a picture of the Cat's Eye Nebula [google.com], a planetary nebula. A planetary nebula is the result of the slow death of a star similar in mass to our sun. A supernova is the result of the explosive death of a significantly more massive star (about 8x more massive).
Supernovae do leave behind pretty glowing nebulae, though. For instance, the Crab Nebula [google.com].
Re:Mmm, explosions (Score:1)
Still very, very beautiful. Makes for a nice and simple but pretty background too (something I have a great difficulty in finding sometimes).
Re:Mmm, explosions (Score:3, Interesting)
Very true- planetary nebulae are some of the most beautiful objects in the universe. Hubble has taken a lot of great pictures of them. If you like the Cat's Eye, but occasionally want a different view, try these planetaries:
Hourglass Nebula [google.com]
Spirograph Nebula [google.com]
Eskimo Nebula [google.com]
They goofed? I think you did (Score:5, Interesting)
I don't think so. Looking at the pics its the same one in both. I think the submitter is confused as there is a large similar looking nebula in the south-east (bottom left, which *is* south-east)
Re:They goofed? I think you did (Score:2)
Not to nit-pick too much, but south east is actually almost directly up in the image, as indicated by the directional arrows on the annotated image.
Re:They goofed? I think you did (Score:2)
High Rez Goodness (Score:5, Informative)
http://imgsrc.hubblesite.org/hu/db/2004/23/images
Re:High Rez Goodness (Score:3, Funny)
OMFG (Score:1)
11oneeleven (Score:2)
uNF
What a stupid filename (Score:2, Funny)
Re:High Rez Goodness (Score:3, Interesting)
Re:High Rez Goodness (Score:3, Interesting)
Re:High Rez Goodness (Score:2)
Super Novas & Nebulas are different critters (Score:3, Interesting)
Re:Super Novas & Nebulas are different critter (Score:5, Informative)
Crab Nebula Info [seds.org]
The star went supernova almost a thousand years ago, and that is whats left.
During the actual event of a supernova, though, the star (from so far away) only seems to go from being a normal star to an amazingly bright one, and then slowly dimming down over a few months (or years). The reason is because stars are so huge they cannot simply explode like in the movies, after all they are in a constant state of nuclear fusion!!
The arrows are correct!!!! (Score:5, Informative)
Almost lost my bearings.. (Score:5, Funny)
Nearby galaxy (Score:4, Interesting)
Re:Nearby galaxy (Score:5, Informative)
There are plenty of stars just itching to blow, though. Eta Carinae [nasa.gov] is about ready to pop, and Betelgeuse [nasa.gov] isn't far off. Either of these stars blow, we'll have a hell of a show.
Here's historically one up close and personal (Score:2)
In turn that (A) allowed UV radiation from the sun to cook a lot of organisms. Yes, including those under water. _And_ (B) affected the climate so massively, that the Earth was turned into a cosmic ball of ice for an awfully long time. _And_ (C) must have caused
Re:Here's historically one up close and personal (Score:2)
Efficient?
The photon radiation from a supernova is utterly trivial; supernovae emit monstrous amounts of energy in neutrinos, but only a tiny amout as gamma. Since it's the gamma you want if you're planning to cook the Earth, that's inefficient enough right there. Not to mention the fact that the Earth will only intercept a tiny fraction
Re:Here's historically one up close and personal (Score:3, Funny)
But even if we talk efficiency as in physics: compare it to rising the ocean level that much. Even completely melting the polar caps won't do. We're talking either:
A. bringing a helluva lot of water from somewhere else. Which ought to cost a helluva lot of energy. Or
B. just creating more water. Which means even more energy. Think: E=m*c^2.
Re:Nearby galaxy (Score:3, Informative)
Still waiting... (Score:4, Funny)
Re:Still waiting... (Score:4, Funny)
Re:Still waiting... (Score:4, Informative)
According to current theory, our sun at the end of its lifetime (5 billion years from now) will become a red giant and throw off its outer layers forming a planetary nebula, and then turn into a white dwarf.
If, by chance the sun as a white dwarf is captured by another star's gravitation, it could draw off mass from that star and then go supernova.
If the sun were to turn into a variable star or nova between now and white dwarf stage, it could very easily boil away the oceans. Some scientists think that the sun will gradually increase in luminosity and that earth will be unhabitable in a billion years.
Alternatively, if a nearby star (25 light years away) were to go supernova, that would pretty much kill the ozone layer and the sun's UV would fry us.
Some scientists think that there is no life in the universe because supernova are such large events in galaxies that as life gets started somewhere it probably gets wiped out by a nearby star going supernova.
Re:Still waiting... (Score:5, Informative)
Close: it's the Chandrasekhar Limit.
It's not the star, but the core of the star that needs to exceed 1.4 solar masses. The Sun will eventually run out of hydrogen in its core, and fusion will end. The core will then be unsupported against its weight, and will contract and heat up dramatically. The increased heat will trigger nuclear fusion of helium, then the Sun switches on again. While the core's heating up, the increased temperature makes the outer layers balloon out to a huge volume, forming the red giant.
It's the core that's interesting, though. Eventually the helium runs out too, and we have a very dense gas of carbon. It contracts and heats up, but the Sun isn't big enough to reach carbon-burning temperatures. So the core can't support itself by burning to produce heat, and instead collapses until it's supported by 'degeneracy pressure' resulting from the fact that in quantum mechanics, no two electrons can occupy the same state.
The Chandrasekhar limit is the maximum mass that can be supported this way, and it's 1.4 solar masses. Get above that mass, the core of the dead star collapses, FAST. The next state down is the neutron star, held up by degeneracy between neutrons rather than electrons. All that matter falling at very high speed hits a core of hard neutronium and the fun starts. Lots and lots and lots of energy has got to go somewhere... the result being a star-shattering kaboom.
Re:Still waiting... (Score:2)
Uninhabitable!? Oh my god, oh my god! What will we do?!
Wait, wait... whew, a billion years. I thought you said a million years.
Re:Still waiting... (Score:2)
Coming to a town near you! (Score:2, Informative)
Re:Coming to a town near you! (Score:1)
Something doesn't sound right... perhaps I am misinterpretting "remnants".
But if SN 2004 dj is 11 million light years away, would not the event have happened 11 million light years ago? Not just a million?
Did you mean Suprnova? (Score:5, Funny)
Re:Did you mean Suprnova? (Score:1)
Goofed images? (Score:1)
Look better. The two last images point to the same place. See the "small" galaxy or whatever at the bottom of the pointed supernova on the two last photos pointed on the quote. They're the same as the big one pointed on the first one, the photo has only been zoomed to that area.
I don't think people realize... (Score:2, Troll)
Re:I don't think people realize... (Score:2)
I'm assuming you refer to 1987A, though it was not in Monoceros. No, it was not the last real supernova. It was the last one that was near enough to be visible to the naked eye, there have been lots since then, they just tend to be rather far and so dim.
This is brighter than most, which is why it's interesting, but nowhere
Keep patching up Hubble? (Score:2)
Stop Whining and Get it Right (Score:2)
ISS spacewalk vs. Hubble repair mission (Score:1)
OK, pay attention people. The ISS spacewalk presents very little risk of a dead (astro|cosmo)naut - at worst the guy turns around and goes back into the ISS.
A shuttle mission to the ISS has a fallback position if the shuttle is found to
Neutrinoes and 1987A (Score:2)
No humans to Hubble (Score:2)
Does anyone in our industry still have an opinion or i
Re:Political Comments not Nesissary (Score:1, Insightful)
>still too dangerous work on the Hubble Telescope, which after all, is
>only used for science."
>
Everybody excoriated NASA for not flying to the station, not paying attention to safety, not getting the Air Force to look, etc, etc. They came up with the safe haven plan to address those concerns, way to go NASA. Then someone noticed it was going to end up not saving Hubble. All of a sudden, what the hell, take a chance, don
Re:Political Comments not Nesissary (Score:5, Informative)
1) Age isn't necessarily a bad thing with a telescope. Lots of telescopes are a lot older than that - witness the Anglo-Australian Telescope, the UK Schmidt Telescope, and the recently burned-down Great Melbourne Telescope (aka MSSSO 50") which provided evidence that the universe is accelerating.
oh yeah, and hubble was launched on April 24, 1990 [hubblesite.org] - you do the maths.
2) The replacement, the James Webb Space Telescope is optimised for the Infra-Red and can NOT operate in the blue/UV like hubble. Nor will it be launched until 2012, 4-5yrs *after* the prospective hubble death date.
JWST will also be at the L2 lagrange point, meaning that there is NO possibility of any servicing mission. here [nasa.gov] is info on the orbit.
3) There are NO better telescopes on the ground for imaging. Hubble has a *diffraction-limited* resolution of about 0.05" - 0.1" (0.05 - 0.1 arcsec). The BEST sites in the world (Mauna kea, cerro paranal) get seeing as good as 0.3-0.4" at the best of times, and that isn't too often.
No, adaptive optics do NOT help because they limit the field-of-view. Hubble has a diffraction limited FOV across the entire chip.
4) Hubble does not have to contend with atmospheric absorption, which makes observations in some bands (like the aforementioned UV) nigh on impossible.
Re:Political Comments not Nesissary (Score:2)
None of it, obviously, and such emotive appeals don't further your point, but thanks for the info. It still doesn't invalidate my point that 20 years is not particularly "old" for a telescope. Especially when it cost $US1.5billion. Hence all the servicing missions so far.
Is there any reason to believe JWST/NGST will cost significantly less than hubble? So lets estimate $US1-1.5billion all up. How much does a servicing mission cost to hubble (ignoring the fact that JWST
Re:Political Comments not Nesissary (Score:3, Insightful)
Shuttle launches run to around US$500M (the actual cost is unclear, sin
question (Score:1, Interesting)
how hard would it be to actually replace hubble with a similar yet much more modern instrument? And just how long would it take. Lets say we kept with the hubble design and just upgraded everything. Can you put a new hubble into orbit without a shuttle launch and if so, why not do that. It can't be that expensive to build a clone and this time they know what to generally expect. I'm no genius on this stuff but I was wondering if anyone had any reliable information on the prospects of
Re:Grainy Image? (Score:1, Interesting)