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#529 | |
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Bamboozled!
"πΊππ·π·π"
May 2003
Down not across
250428 Posts |
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You will end up with a photo of the moon at a distance of 400 thousand km with a camera which has an aperture of a few millimetres and a mass of a gram or so. Further, your camera has not been specifically optimized within those physical parameters to take especially high quality images because a phone camera has to be dirt cheap to be sold by the billion to people who really don't care that much about image quality. All that bullshit in your other post about crashing into the star is just that: bullshit. It would take extremely precise targeting to hit the star and why would anyone want to do that? Unless a decision is made to impact something the odds are overwhelmingly likely that all the probes will just pass clean through the Proxima system. By the time the probes get there we should know the location of the planet to within a thousand km or so. In other words, the photo could be taken from much closer than 400,000 km. Motion blur could be an issue but could be mitigated by scanning the camera field of view or by subsequent deconvolution of the blurred image. Even if the former isn't practical from mass and / or energy considerations, the latter has been standard practice for 20 years or more already. |
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#530 |
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Bamboozled!
"πΊππ·π·π"
May 2003
Down not across
1078610 Posts |
That may be all you are interested in. I can assure you that there are many others who are nowhere near as blinkered in their desire for knowledge and understanding. Why did you think I posted about magnetic fields, chemical composition, thermal structure, and so forth?
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#531 |
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Bamboozled!
"πΊππ·π·π"
May 2003
Down not across
2·5,393 Posts |
I know.
Why do you think I referred to graphene only in the context of the light sail, which needs to have a large area in as small a mass as possible but doesn't need to be rigind, and graphite as a candidate for the probe's structure on which the science instruments are mounted, which needs to be rigid and as small a mass as possible? Please pay attention to what I'm typing and please read the supplementary material to which I have given you an excellent entry point. |
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#532 | |
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Bamboozled!
"πΊππ·π·π"
May 2003
Down not across
2·5,393 Posts |
Quote:
The killer is that we don't yet know how to make big enough single crystals of diamond. Sintered polycrystalline diamond (IMO, I don't know for sure) is likely to have too great a surface roughness for standard semiconductor technology to build reliably working devices on top of it. I agree SiC is a fine candidate material and easy to make in large single crystals but please remember that the diamond proposal is (AFAIK) entirely my own idea and I'm quite prepared to be convinced that it is a bad one. |
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#533 | |
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Sep 2006
The Netherlands
36 Posts |
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a) communication back to the home front b) a good description of what you saw back to the homefront A) you keep ignoring in this. 1 meter light sail in diameter is gonna get lost in all the sounds and noises that the stars make. You need something that points to planet earth. Radio communication goes at light speed. You need a huge parabolic radio antenna to communicat to the homefront. The light sail as you pointed out you want light and very huge. Let's make it 500 meters in diameter ok and very light. No big problem. But then we still need a huge parabolic radio antenna that points back to earth or maybe even to some point far away from the Sun as an 'in between radio station', who will say? B) to take a good picture, regardless at which frequency you want to take it, you need to catch enough light. So the computer chip you use might be very tiny and light - yet the tube and lenses or mirrors used will be significant in diameter. For such expensive mission you definitely do not want some sort of space version of the apple iphone camera. That's not gonna cut it. You're gonna need a big diameter aperture or lenses. For a close pass by of a planet you already will need 10 inch - yet at a speed of 0.05c you can't garantuee a close pass by - even if we do figure out somehow more details like which different planets specific stars might have or do not have and even if we might have some clue where at which moment planets are rotating based upon future telescopes (E-Elt etc). You still are gonna need a far superior camera over other probes to generate enough data for the mission. I'm no expert there but we're soon looking at 16 inches diameter. That's gonna weigh something. That 1 kilo idea is not realistic. 300 is more realistic for the total probe - and that will already require serious design and improvements over anything that was there so far. |
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#534 | ||
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Romulan Interpreter
Jun 2011
Thailand
227008 Posts |
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#535 | |||
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Bamboozled!
"πΊππ·π·π"
May 2003
Down not across
101010001000102 Posts |
Quote:
Quote:
You persist in ignoring what others have to say. You keep making bald assertions about what you believe to be necessities which you fail to justify and ignore alternatives. Where did I say that the information sent back to earth had to be by radio? Please read this You are correct that there is background noise, primarily from the star. Please do a little bit of reading and calculate the power per unit bandwidth to be expected from Proxima Centauri. The formulae are straightforward and the raw data on Proxima are easily available. I'll even make it easy for you by pointing you at https://en.wikipedia.org/wiki/Planck's_law and https://en.wikipedia.org/wiki/Proxima_Centauri Then consider the power per unit bandwidth of a diode laser. Assume, say, 1W with a bandwidth of 30GHz operating at a frequency of 300THz (a wavelength of about a micron) which are fairly typical values for easily obtainable lasers. Compare that with the blackbody radiation from the star. To optimize your design, choose the diode's operating frequency (red-shifted of course) to be the same as a deep absorption line in the stellar spectrum and compare once again. It should go without saying that the detector at earth should also be tuned to the (red-shifted) laser wavelength and have an equally narrow bandwidth. I obliged your curiosity and calculated fthe size of an imaging telescope for you. Please do your own computations from now on. I'll give you pointers, as above, if you need the raw data but you ought to be able to use a search engine for yourself by now. BTW, do you still think it would be cheaper to build a 10-20km diffraction-limited optical telescope in earth orbit? Cheaper than even your (IMO excessive) $300G estimate for an interstellar mission? I estimated $20G in total and $1M per probe. My estimates are 2-4 times larger than those at https://breakthroughinitiatives.org/News/4 Quote:
Added in edit: My apologies, I was naively assuming that the camera optics needed to be localized to a small area of the spacecraft, leading to an incorrect view that the aperture would be of order one cm or less. There is no need for such a restriction and the effective aperture could be essentially the size of the spacecraft itself, or 10cm. My assumption was that a filled aperture telescope would be necessary. It quite clearly is not. Once more: please read http://www.breakthroughinitiatives.org/Initiative/3 and links therein. Another excellent resource is http://arxiv.org/abs/1604.01356 (referenced from the Breakthrough Initiatives site) which goes into very precise detail about the light sail propulsion mechanism for spacecraft of all sizes, from sub-kilogram probes reaching 0.2c to 100-ton human-rated spacecraft for solar-system travel at 0.0026c (760 km/s). A 100kg craft (Voyager-class) would reach Mars in about a day at a speed of 0.015c. Note that we are considering only fly-by and/or long duration missions here so don't need to consider how to slow down again at the destination. (Incidentally a 100kg probe would reach Proxima in around 280 years, which is substantially longer than I believe we are currently willing to contemplate. Figure 13 in that paper addresses communication back to earth from a sub-kg probe. The scenario considers a 1g spacecraft structure 10cm in diameter and does not use any other optical component such as the 1 metre sail for comms. When you can back up your claims with sound and detailed physics and engineering computations I will be inclined to take them seriously. Until then you give every appearance of spouting ill-informed nonsense. Last fiddled with by xilman on 2016-09-01 at 10:31 Reason: Fix accidental omission |
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#536 |
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"/X\(β-β)/X\"
Jan 2013
2·5·293 Posts |
Explosion at SpaceX launch site: http://www.bbc.com/news/world-us-canada-37247077
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#537 | |
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"Kieren"
Jul 2011
In My Own Galaxy!
1015810 Posts |
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Last fiddled with by kladner on 2016-09-01 at 15:52 |
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#538 | |
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Nov 2004
10348 Posts |
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Norm |
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#539 | |
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Bamboozled!
"πΊππ·π·π"
May 2003
Down not across
2·5,393 Posts |
Quote:
I had hoped that those interested would have found it by themselves --- it's not difficult given the heavy hints I'd already posted --- but it became clear that diep at least had failed to do so. |
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