The Sun is no longer the largest object in our solar system.
For some reason, I am very freaked out about this.
(via Lisa)
***
I've learned the same kick at four different schools by four different names: windmill kick, crescent kick, smash kick, and now, at the new school, fan kick.
I get worse at them with each new name.
For some reason, I am very freaked out about this.
(via Lisa)
***
I've learned the same kick at four different schools by four different names: windmill kick, crescent kick, smash kick, and now, at the new school, fan kick.
I get worse at them with each new name.


Comments
(But it's _beautiful._
But I like that in a person.
Edited at 2007-11-16 12:56 am (UTC)
(106 miles/(.05 * 2 miles))3 = (106/10-1)3 = 1021
The density will go down by a corresponding amount, so a factor of 10-21. So now we are down to a density of about 30 molecules per cubic centimeter. I'm having a hard time digging up numbers for bright comet dust-tail particle densities, but this is a pretty typical number for the cold interstellar medium, or the edges of a star-forming region. So, something like the denser (though not the densest) parts of interstellar dust clouds.
Today's solar wind, by comparision, has a local density of 2.6 protons/cm3.
The end is near!
Repent!
(Or get really, really drunk.)
"oh no we are doomed to be struck by a gigantic ball of nothing :/ "
That kind of calmed me down.
And may be concealing a giant Mayan apocalyptic hamster.
Meanwhile, I saw your evil twin today! Minus the glasses. But if we set him loose on Kelleys Island, no local would be able to tell the two of you apart. Swear.
Then again, they can't tell my twin and I apart -- hey, no, wait! That's my darn fellow workshoppers!!!
This is a very press-releasy definition of "object", such that it can include a rapidly dispersing, non-gravitationally-bound puff of dust from a comet but not include other rapidly dispersing, non-gravitationally bound things like the solar wind.
Not that that helps, I'm sure.