OP is my Sun
M(v) - M(V) = -2.5Log[ F(λ)(V) / F10λ(V) ]
Quote from: Connor on February 07, 2016, 05:15:15 PMM(v) - M(V) = -2.5Log[ F(λ)(V) / F10λ(V) ]stop that
Quote from: N'awoo on February 07, 2016, 05:16:58 PMQuote from: Connor on February 07, 2016, 05:15:15 PMM(v) - M(V) = -2.5Log[ F(λ)(V) / F10λ(V) ]stop thatA star has a parallax angle of 10", what is its distance?
Quote from: Connor on February 07, 2016, 05:18:10 PMQuote from: N'awoo on February 07, 2016, 05:16:58 PMQuote from: Connor on February 07, 2016, 05:15:15 PMM(v) - M(V) = -2.5Log[ F(λ)(V) / F10λ(V) ]stop thatA star has a parallax angle of 10", what is its distance?FUCK uh uh uh uh uh uh uh uh uh uh uh uh uh uh uh uh 1 / 5
Quote from: N'awoo on February 07, 2016, 05:19:16 PMQuote from: Connor on February 07, 2016, 05:18:10 PMQuote from: N'awoo on February 07, 2016, 05:16:58 PMQuote from: Connor on February 07, 2016, 05:15:15 PMM(v) - M(V) = -2.5Log[ F(λ)(V) / F10λ(V) ]stop thatA star has a parallax angle of 10", what is its distance?FUCK uh uh uh uh uh uh uh uh uh uh uh uh uh uh uh uh 1 / 50.1pc. d(in pc) = 1/p(in arcseconds)I realized afterwards that distance didn't make much sense but huehuehue, I should've put 0.1"
if a sun made of lava collided with a sun made of ice, what would happen?
yea, this lesson kind of throws me off since i get mixed up with parallax and arcseconds ad which to invert.
Quote from: N'awoo on February 07, 2016, 05:21:53 PMyea, this lesson kind of throws me off since i get mixed up with parallax and arcseconds ad which to invert.Astronomy can be t r i c k y I think the hardest part is fucking determining where everything goes in the equations. And then unit cancellations. That stuff can be annoying if it's likeHEY GIVE ME THE FLUX DENSITY IN ERGS PER SECOND PER SQUARE CENTIMETER BUT CONVERT IT TO FUCKING MKS UNITS BECAUSE FUCK YOU
yea, like weins law and the other one.. i forgot the name.just wait until you get to cosmology
if the sun is a star
