Rave Radio: Offline (0/0)
Email: Password:
Page: 1 2 3 Next »»Rating: Unrated [0]
I Though Everyone Should Know That...
Good [+1]Toggle ReplyLink» daFTWin replied on Wed Feb 19, 2003 @ 5:19pm
daftwin
Coolness: 277135
DONE AND DONE!!!..
C ya'll in a couple of weeks!!
Good [+1]Toggle ReplyLink» ontheroadagain replied on Wed Feb 19, 2003 @ 6:30pm
ontheroadagain
Coolness: 55035
N: "hahaha, you've been tranced biatch!"

K: "No wonder I didnt realize it.."

HAHAHAHAHAHAHAHAHAHAHAHAHAHAHAHAHAHAHAHAHAH

BEST COMEBACK EVER!!

ohhh shitttt.....fuck.....ok...*sigh*....

...1,2,3,4,5,6,7...
Good [+1]Toggle ReplyLink» Agent_Yogurt replied on Wed Feb 19, 2003 @ 8:59pm
agent_yogurt
Coolness: 134310
heather: u say without hot guys we would die? then y am i still alive??
Good [+1]Toggle ReplyLink» El_Presidente replied on Wed Feb 19, 2003 @ 9:04pm
el_presidente
Coolness: 300025
cyz youre a dyke
Good [+1]Toggle ReplyLink» clown replied on Wed Feb 19, 2003 @ 10:01pm
clown
Coolness: 222465
because hot guys are still out there.. stop looking under rocks..
Good [+1]Toggle ReplyLink» Unknown User replied on Wed Feb 19, 2003 @ 11:23pm
unknown%20user
Coolness: 410
here's some info on the sun in relations to other stars.

B Comparisons with Other Stars

A star is a ball of hot, glowing gas that is hot enough and dense enough to trigger nuclear reactions, which fuel the star. In comparing the mass, light production, and size of the Sun to other stars, astronomers find that the Sun is a perfectly ordinary star. It behaves exactly the way they would expect a star of its size to behave. The main difference between the Sun and other stars is that the Sun is much closer to Earth.

Most stars have masses similar to that of the Sun. The majority of stars’ masses are between 0.3 to 3.0 times the mass of the Sun. Theoretical calculations indicate that in order to trigger nuclear reactions and to create its own energy—that is, to become a star—a body must have a mass greater than 7 percent of the mass of the Sun. Astronomical bodies that are less massive than this become planets or objects called brown dwarfs. The largest accurately determined stellar mass is of a star called V382 Cygni and is 27 times that of the Sun.

The range of brightness among stars is much larger than the range of mass. Astronomers measure the brightness of a star by measuring its magnitude and luminosity. Magnitude allows astronomers to rank how bright, comparatively, different stars appear to humans. Because of the way our eyes detect light, a lamp ten times more luminous than a second lamp will appear less than ten times brighter to human eyes. This discrepancy affects the magnitude scale, as does the tradition of giving brighter stars lower magnitudes. The lower a star’s magnitude, the brighter it is. Stars with negative magnitudes are the brightest of all.

Magnitude is given in terms of absolute and apparent values. Absolute magnitude is a measurement of how bright a star would appear if viewed from a set distance away. By convention, this distance is 10 parsecs, or 32.6 light-years. Apparent magnitude measures how bright a star appears from Earth. The Sun’s absolute magnitude is 4.8. The brightest known stars have absolute magnitudes of about -9 (lower magnitudes mean brighter stars), and the dimmest known stars have absolute magnitudes of about 20. The apparent magnitude of the Sun is -26.72. The apparent magnitude of the brightest star in Earth’s night sky, Sirius, is -1.46. The dimmest stars that can be seen from Earth with unaided eyes have apparent magnitudes of about 6.

Astronomers also measure a star’s brightness in terms of its luminosity. A star’s absolute luminosity or intrinsic brightness is the total amount of energy radiated by the star per second. Luminosity is often expressed in units of watts. The Sun’s absolute luminosity is 3.86 × 1026 watts. The absolute luminosity of stars ranges from one thousandth of the luminosity of the Sun to 10 million times that of the Sun.

Another way of measuring brightness is to measure the amount of light that reaches an observer. This measurement is called apparent brightness or apparent luminosity. Apparent luminosity depends on the absolute luminosity of a star and the distance from the star to the observer. Apparent luminosity becomes smaller as distance from the star to the observer becomes larger. From Earth, the apparent luminosity of the Sun is 10 billion times greater than the apparent luminosity of the next brightest star, Sirius, because the Sun is so much closer to Earth.

The radius of the Sun is about average among stars. The radii of most stars fall between 0.2 and 15 times the Sun’s radius, although some giant stars are hundreds of times larger than the Sun. Larger stars usually have larger absolute luminosities.

We receive much more energy from the Sun than from other stars, because the Sun is so nearby. The Sun’s proximity also allows scientists to study its face in detail. A modest telescope can resolve solar structures that are 700 km (400 mi) across—about the distance from Boston, Massachusetts, to Washington, D.C. That level of detail is comparable to seeing the features on a coin from 1 km (0.6 mi) away. Other stars are so distant that the details on their surfaces remain unresolved with even the largest telescopes.
Good [+1]Toggle ReplyLink» mindset replied on Sat Feb 22, 2003 @ 10:57pm
mindset
Coolness: 53245
how many atoms in the universe = metaphysics

the application of a theory of knowledge (like: hey, i know how many atoms there are) on metaphysics implies a circular formula, a loop.

stars to galaxies to universes to dimensions to stars.

we're all gonna die.
Good [+1]Toggle ReplyLink» El_Presidente replied on Sun Feb 23, 2003 @ 6:13am
el_presidente
Coolness: 300025
were all gonna die my friend. were all gonna die

*hits on his tam tam, beatnick stylez*
Good [+1]Toggle ReplyLink» mdc replied on Sun Feb 23, 2003 @ 5:27pm
mdc
Coolness: 149515
wrong
Good [+1]Toggle ReplyLink» neoform replied on Mon Feb 24, 2003 @ 12:48am
neoform
Coolness: 340365
who's wrong?
Good [+1]Toggle ReplyLink» mdc replied on Mon Feb 24, 2003 @ 9:56am
mdc
Coolness: 149515
everyone!! mwahahaha!
Good [+1]Toggle ReplyLink» neoform replied on Mon Feb 24, 2003 @ 10:11am
neoform
Coolness: 340365
oh yeah? well your friends DON'T call you ejack! bitch! (that's what they call you)
Good [+1]Toggle ReplyLink» Screwhead replied on Mon Feb 24, 2003 @ 10:12am
screwhead
Coolness: 686290
I call him Spike.
Good [+1]Toggle ReplyLink» El_Presidente replied on Mon Feb 24, 2003 @ 2:23pm
el_presidente
Coolness: 300025
boozay!
Good [+1]Toggle ReplyLink» daFTWin replied on Mon Feb 24, 2003 @ 3:20pm
daftwin
Coolness: 277135
BOOZAY!!!!
Good [+1]Toggle ReplyLink» PitaGore replied on Mon Feb 24, 2003 @ 4:12pm
pitagore
Coolness: 472505
Afro Mafioso back inside da place !!
Woot Woot !!
Good [+1]Toggle ReplyLink» mindset replied on Mon Feb 24, 2003 @ 5:14pm
mindset
Coolness: 53245
IT'S NOT boozay, or BOOZAY, it's boozAY!
Good [+1]Toggle ReplyLink» mdc replied on Mon Feb 24, 2003 @ 10:58pm
mdc
Coolness: 149515
spike??
how do you know about spike??
why you call me spike fred?
Good [+1]Toggle ReplyLink» Screwhead replied on Tue Feb 25, 2003 @ 12:02am
screwhead
Coolness: 686290
Because you're SPIKE!

Right Spike?
Good [+1]Toggle ReplyLink» neoform replied on Tue Feb 25, 2003 @ 12:13am
neoform
Coolness: 340365
djneoform: haha spooky = assholishman
SpOOkY: yup yup
SpOOkY: w4rd to yo m0tha BEYOTCH
djneoform: my mother biotch? i thought that was a pie or something
djneoform: oh i get it
SpOOkY: no, you're thinking a brioche.
SpOOkY: damn you
djneoform: haha
djneoform: *sticks penis in fred*
SpOOkY: don't make the person who just smoked think about food!
SpOOkY : damn.
SpOOkY : I want pastry.
djneoform: *laughes* that wasn't my dick
djneoform: hahaha
djneoform: sucka
SpOOkY: what?
SpOOkY: dude
SpOOkY: wtf are you talking about?
djneoform: i just stuck someone else's dick in you!!
djneoform: *laughes some more*
SpOOkY: yay!
I Though Everyone Should Know That...
Page: 1 2 3 Next »»
Post A Reply
You must be logged in to post a reply.