Relay-Version: version B 2.10 5/3/83; site utzoo.UUCP Posting-Version: version B 2.10.1 6/24/83; site npois.UUCP Path: utzoo!watmath!clyde!cbosgd!ihnp4!drutx!mtuxo!npois!jay From: jay@npois.UUCP (Anton Winteroak) Newsgroups: net.astro Subject: re how many photons Message-ID: <469@npois.UUCP> Date: Tue, 3-Dec-85 15:42:02 EST Article-I.D.: npois.469 Posted: Tue Dec 3 15:42:02 1985 Date-Received: Thu, 5-Dec-85 05:35:31 EST Organization: ATTIS, Neptune, NJ Lines: 37 A few weeks ago, someone asked how many photons per square meter per second did we receive for objects of various stellar magnitudes. I have computed that from the following facts: 1. The sun is at apparent magnitude -26 to us. 2. The sun is 1.5 e11 meters away from us. 3. The sun gives off 4.0 e33 ergs per second. 4. The average energy of a photon from the sun is 2.1 eV. 4a. Therefore there are 2.9 e11 photons per erg. 5. I counted photons of all wavelengths (including ir, uv, etc.) 5a. For visable light, divide by about two. Apparent Mag. Photons/meter square per sec comments. -26 4e21 this is what we get from the sun. -25 2e21 -20 2e19 -15 2e17 as bright as a half moon. -10 2e15 Comet Kohoutek was supposed to get this bright. -5 2e13 Venus gets this bright now and then. Halley's Comet was this bright in 867. 0 2e11 Several Stars look this bright. 5 2,000,000,000 dimmest naked eye stars. 10 20,000,000 dim stars in big binoculars. 15 200,000 the planet Pluto, on a good night. 20 2,000 visable on photographs and image intensifiers only. 25 20 near the limit of what can be photographed from through our atmosphere. remember to divide by two to get visable photons, and by two again for atmospheric absorbtion.