Relay-Version: version B 2.10 5/3/83; site utzoo.UUCP Posting-Version: version B 2.10.2 11/03/84 (WLS Mods); site astrovax.UUCP Path: utzoo!watmath!clyde!burl!ulysses!allegra!princeton!astrovax!wls From: wls@astrovax.UUCP (William L. Sebok) Newsgroups: net.astro.expert Subject: Re: photons per stellar magnitude Message-ID: <685@astrovax.UUCP> Date: Fri, 15-Nov-85 14:59:38 EST Article-I.D.: astrovax.685 Posted: Fri Nov 15 14:59:38 1985 Date-Received: Sat, 16-Nov-85 09:10:03 EST References: <1863@saber.UUCP> Organization: Princeton Univ. Astrophysics Lines: 46 In article <1863@saber.UUCP> jc@saber.UUCP (John Cincotta) writes: >How many photons per second per square meter are received from a star of >say 10th magnitude on the surface of the earth?? From Allen's "Astrophysical Quantities" (Chapter 10): log f (V) = -0.4m - 8.43 lambda V -2 -1 -1 where f (V) is visual flux in erg cm Angstrom sec outside the Earth's lambda atmosphere near 5500 Angstroms. "This relation is almost unchanged from B to M stars." Therefore (plugging in numbers), for m = 10 V -13 -2 -1 -1 f = 3.72 x 10 erg cm sec Angstrom lambda Now a photon at a wavelength of 5500 Angstrom has an energy of E = h(c/lambda) -27 18 = (6.626 x 10 erg-sec) (2.998 x 10 Angstrom/sec) / (5500 Angstrom) -12 = 3.612 x 10 ergs this yields -2 -1 Flux(5500 Angstrom) = 0.11 photons cm Angstrom -2 -1 = 110 photons meter Angstrom For a 1000 Angstrom bandpass (roughly since I am too lazy now to do the integral and the whole business is approximate anyway) this is about 110,000 photons / square meter for that 10th magnitude star. -- Bill Sebok Princeton University, Astrophysics {allegra,akgua,cbosgd,decvax,ihnp4,noao,philabs,princeton,vax135}!astrovax!wls