Hubble Chronicles Mysterious Outburst
An eruptive star that brightened to 600,000 times its initial intensity and briefly outshone all others in the Milky Way Galaxy has astronomers amazed and puzzled over what happened...The star, named V838 Monocerotis, has suddenly grown so big that if placed in the center of our solar system it would engulf Jupiter.
That's an alien war where one race destroyed the others' solar system.
-- Cheers!
Maybe it's going through puberty? Explosive growth without getting any brighter =;-]
- In the beginning there was nothing, and then it exploded
from the article:
"Oddly, it isn't hot and eruptive in the manner of a supernova or nova, both of which toss off outer layers in explosive fits. Instead, V838 Mon, as astronomers call it, achieved remarkable brilliance while swelling to gargantuan size and remaining cool at its surface."
wierd shit
Get the EULA T-shirt
Courtesy of Astronomy Picture of the day
While I was RTFA, I pretty much expected that this "sudden" event would be revealed as sudden only when measured in geologic or cosmic time; say, a few thousand millenia or so. The fact that this happened over only a few months is fascinating.
http://www.homoexcelsior.com/omega.db/datum/refere nce/star_lifting/177
Sean Ellis
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This event goes contrary to everything what is known about the star life cycle so far. The most strange thing is the luminosity and the fact that resulting object is a big star, and not a collapsed object (like black hole, neutron star or white dwarf)
I doubt that we will ever figure out - and I suspect that even if we did figure out we couldn't do much about it
According to the article, this happened 20,000 years ago...
*yawn*
My father is a blogger.
The collapse of the core of a star as it is about to go supernova takes less than an hour or so, and it is in the shock wave of the exploding star that the really heavy elements are formed from nucleosynthesis. Not everything in astronomy works on gigayear timescales!
Dr Fish
42. Stay the fuck away from "V838 Monocerotis" today.
Check.
Well, that's me done for today. Time to troll Slashdot...
Opportunity knocks. Karma hunts you down.
For those who want a screen filling larger image, 1651x1651, it is the subject of today's Astronomy Picture of the Day (APOD).
-Adam
"In fact, at present it is one of the coolest stars known," Bond told SPACE.com.
Well, it sure looks pretty damn cool.
"In fact, at present it is one of the coolest stars known," Bond told SPACE.com.
The astronomer then proceded to slick back his hair and donned a pair of shades, while rythmically snapping the fingers of his free hand.
"Oh, yeah," added Bond.
The angel in the oatmeal.
For those who don't know what I'm talking about, read The Fourth Profession.
Hubble took a series of 4 photos, and you all have been looking only at the last of them. Also is a link in case you want large versions of each individual photo, and another for links for all the text, images, and video concerning the event. I'm surprised Doctor Fishboy never pointed this out.
"I'm so moist I'm sticking to the leather." -Kermit the Frog on The Late Late Show
Suppose the star is moving towards the earth.
As it periodically swells and casts off a dust nebula, it could move to our side of the past nebulae (assuming that the less dense nebula moves slower than the star).
Now the nebula acts as a reflector, and there is less dust between the star and earth to hide it.
It could be that these effects magnify the apparent brightness, compared to otherwise similar stars that stay within their obscuring nebulae.
They probably have enough data to rule this out, and the orbiting companion theory is more likely, but it would be interesting to know if you could explain some of the 600,000 fold brightness this way.
Free book: Science Toys You Can Make
1. If the star is moving at a certain velocity, then the average velocity of a particle in a cast-off shell of dust will be at the star's velocity. In other words, the star will stay centered in any spherical shell of material it gives off (yes, I know, some neutron stars get kicked out of their nebulae, but that's a far more energetic process). An interstellar wind, if present, would destroy the spherical shape of the nebula.
2. The nebula is acting as a reflector, no doubt, but it is so thin that the star is perfectly visible through it anyway. It's the red star in the photo(s).
3. The only way this could "magnify the apparent brightness" of the star is if the star and nebula were not resolvable as separate objects. Then light reflected from the nebula could be mistaken as light from the star (ignoring spectral techniques). But the photo is of a fully resolved nebula and star. A child could distinguish light from the star vs. reflected light from the nebula.
"I'm so moist I'm sticking to the leather." -Kermit the Frog on The Late Late Show
I was with Mark (Wagner) and Sumner (Starrfield) when we got the spectra. . .now I'm going to be really pissed if I'm not on the paper since I was the one taking the spectra. . .
But anyhow. . .the spectra is really interesting, there are P Cygni profiles for every emission line in the spectra (P Cygni's look like half a gaussian in emission with a sharp cutoff to be half a gaussian in absorption). This object was actually noticed by people looking at variable stars and then was picked up by some other folks in Arizona which showed the light echos even in the relatively low resolution images we got on the ground compared to our HST ACS images.
Their version of SETI @ Home involves manipulating a nearby star in a highly noticable manner. Now that they have our attention, they await our transmitted replies. :-)
(yeah yeah, light travels too slowly, etc...)
While I love the Astronomy Picture Of The Day and the similarly-cool Hubblesite pics of this event, All the good-sized images have that annoying twinkly-crosshairs look to them. The Hubblesite pics include this small image without them, but all of the large-format images that I can find have the "star filter" applied. Does anyone know where I could find a large, unaltered image or images?
--
Brightness we can easily measure but distance for anything but the closest stars is very difficult to determine. They based their conclusion on a guess that this star is 20,000 light years away. While this is definitely an interesting event, if that guess is wrong it might not be nearly as dramatic as they say.
According to the article, they determined the distance by looking at the companion star in the pair, which is of a well-known type, with a well-known temperature/luminosity relation. That gave them a reasonable distance estimate for the companion, and so for the giant.
A proper discussion would have involved momentum. I implicitly assumed the dust particles all had the same mass. It doesn't change the essence of the argument, however.
"I'm so moist I'm sticking to the leather." -Kermit the Frog on The Late Late Show
5. Their distance estimate of 6 kpc was a lower limit. If anything it was even further away and brighter.
"I'm so moist I'm sticking to the leather." -Kermit the Frog on The Late Late Show
Here's a link to Bond's paper in Nature.
"I'm so moist I'm sticking to the leather." -Kermit the Frog on The Late Late Show
A super nova would be the coolest thing ever as it would light up a large area of the sky for about a year. But then again, a supernova might not be to friendly for all the aliens. Damn aliens, making all our fun into a giant guilt trip. Hoch
2*31*37*263