what can I see?
Timothy Collinson
(18 Aug 2014 09:20 UTC)
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Re: [TML] what can I see? Tim (18 Aug 2014 14:22 UTC)
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Re: [TML] what can I see?
Jeffrey Schwartz
(18 Aug 2014 15:13 UTC)
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Re: [TML] what can I see?
Knapp
(18 Aug 2014 17:54 UTC)
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Re: [TML] what can I see?
Timothy Collinson
(19 Aug 2014 07:58 UTC)
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Re: [TML] what can I see?
Jeffrey Schwartz
(19 Aug 2014 13:35 UTC)
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Re: [TML] what can I see?
Timothy Collinson
(19 Aug 2014 17:05 UTC)
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Re: [TML] what can I see?
Timothy Collinson
(18 Aug 2014 20:55 UTC)
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Re: [TML] what can I see?
Tim
(19 Aug 2014 02:14 UTC)
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Re: [TML] what can I see?
Timothy Collinson
(19 Aug 2014 08:03 UTC)
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On Mon, Aug 18, 2014 at 10:20:35AM +0100, Timothy Collinson wrote: > I'm trying to describe the view on a world where this is given as > stellar data: > F7V M1IV > So I know the main star looks yellow-white. Not sure about the other - is > it even visible? I would expect so! It's a subgiant, and likely more luminous than the F7V by a factor of 10-20 or so. The F7 main sequence star is not very much hotter than the Sun; I don't think anybody would notice the difference without measurement or some sort of side-by-side comparison. > The other clue that I have is that the UWP is C565436-5 so I'm > assuming shirt sleeve conditions are possible for at least portions > of the year on some of the planet. For similar temperature to Earth, the primary star would be slightly smaller in the sky, though a little more "dazzling" than our Sun from Earth. Without knowing the orbit of the companion star, it could be anywhere from visually much larger and brighter (if they're a close binary pair inside the planet's orbit), similar or smaller disk with dimmer/yellower light (medium binary), to just a bright pointlike star easily visible during the day (distant binary). The middle case is possibly the most interesting, with substantial light and some heat during the primary's "night" for much of each year. If the companion was about 10 times further out but 20 times as luminous, it would contribute about 5% of the light and 20% of the heat. That 5% light might not seem much in numbers, but indoor lighting is usually less than 1% as bright as daylight, so it would be much brighter than most artificial lighting. Likewise the 20% heat influx would be enough to noticeably reduce heat loss during the (primary) night or add to warming during the day. One other thing to remember is that an F-class star puts out a fair bit more energy into ultraviolet than our Sun does. UV-A in particular would be more intense at the surface of an otherwise Earth-like world, so beings not adapted to such flux would likely need to avoid exposing unprotected skin and eyes for too long. I hope this is a start towards some sort of help. - Tim