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Subject:
sun
Category: Science > Astronomy Asked by: kr54-ga List Price: $5.00 |
Posted:
29 Dec 2005 07:07 PST
Expires: 28 Jan 2006 07:07 PST Question ID: 610884 |
Why does the Sun not give off radiation uniformly all through the solar system? | |
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Subject:
Re: sun
Answered By: hedgie-ga on 02 Jan 2006 05:20 PST |
Hello kr54-ga and welcome to Google Answers. Thank you for asking this interesting question about out Solar System. As commenters tried to say, there are two possible meanings, so I will answer both: Meaning 1: Venus is hot, Mars is cold Neptun is very cold .. In general: Father from the Sun, the colder it gets This link shows how Temperature goes down with distance from the Sun http://www.lwr.kth.se/Grundutbildning/1B1292/Applets/Climate/T-effective/T-effective.htm Question is :why? Answer : All isotropic sources of energy are like that, It is called Inverse Square law. http://en.wikipedia.org/wiki/Inverse-square_law Meaning 2: Does Sun shine the same in all directions? in other words: Is sun radiation isotropic? Answer is: Yes. "We all know the Sun radiates energy in all directions. The energy radiated from the Sun measured at any fixed distance and from any angle will be approximately the same..." http://www.itnu.de/radargrundlagen/antennen/at08-en.html Please, feel free to ask for clarifications. Rating appreciated. Hedgie |
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Subject:
Re: sun
From: leoj-ga on 29 Dec 2005 14:17 PST |
Because like anything else in a configuration like this, it follows a 1/r^2 law. |
Subject:
Re: sun
From: kottekoe-ga on 29 Dec 2005 17:53 PST |
KR54, Like Silicon Samurai, I'm still perplexed. Please clarify the question. To my knowledge sunlight is radiated quite uniformly. Of course, there are small nonuniformities like sunspots that give some variability, but these are on such a small angular scale that they are irrelevant unless you are in a spacecraft very near the surface of the sun, in which case you're getting cooked either way. I suppose there is some nonuniformity associated with solar latitude. Certainly there will be small effect due to the solar oblateness so I would expect a slightly different flux directly above one of the sun's poles than directly above the solar equator. The solar wind is quite variable and is strongly influenced by the sun's magnetic field, which is roughly aligned with the poles. Large magnetic storms on the sun give rise to solar flares which cause large directional bursts in the solar wind, but have very little effect on "sunlight". As both commenters have noted, there is a strong variation in the amount of light that reaches you depending on how far you are away from the sun. This is a simple geometrical fact since the uniformily radiated light gets spread more and more thinly as you get further away. Since the area of a sphere grows quadratically with its radius, the intensity of the sunlight must fall as the inverse square of the distance. |
Subject:
Re: sun
From: siliconsamurai-ga on 30 Dec 2005 06:01 PST |
Sorry, that's certainly not a clarification of any sort so I'll pass on this question. |
Subject:
Re: sun
From: qed100-ga on 30 Dec 2005 07:25 PST |
Hello kr54-ga. Perhaps you should provide some examples of what you mean by the non-uniformity of sunlight. |
Subject:
Re: sun
From: siliconsamurai-ga on 31 Dec 2005 03:31 PST |
Inverse square distribution is still "uniform." Also, it applies precisely only to sunlight and other electromagnetic fields, not all "radiation" so, without more information we don't know if this is an obvious and elementary question or one about some obscure aspect of astrophysics. |
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