> need to be able to resolve the small details of an object in order to help us get a better understanding of them. Doing this requires building larger and larger light-collecting mirrors
Or an interferometer.
> Basically, the photon sieve is a variation on the Fresnel zone plate, a form of optics that consist of tightly spaced sets of rings that alternate between the transparent and the opaque. Unlike telescopes which focus light through refraction or reflection, these plates cause light to diffract through transparent openings. On the other side, the light overlaps and is then focused onto a specific point – creating an image that can be recorded.
I hadn’t heard of this. It seems that the result would have lower light gathering power than a Fresnel Lens, but potentially higher resolution at a much lower cost. Last time I went to an astronomy lecture, in question time I suggested that the Fresnel Lens would be a good alternative that combines the light weight of the telescope mirror with the wide angle possible with lenses. The Fresnel zone plate would be cheaper and may be as good or better.
> Although such a device would be potentially useful at all wavelengths
But if I understand the optics correctly, different wavelengths would focus at different focal points, so multiple exposures would be needed to build up a coloured image. (Let me check. Looking up https://en.wikipedia.org/wiki/Zone_plate). Not so good. The necessary spacing of rings depends nonlinearly on the wavelength, you can’t get away with using the same zone plate again with a different focus length. So a single zone plate will only work with a single wavelength, you’d need a different zone plate for each wavelength – not an insurmountable obstacle, just slightly annoying to change the lens every time you change the filter.
> However, in the long-run, they hope to create a sieve that will measure 1 meter (3 feet) in diameter. With an instrument of this size, they believe they will be able to achieve up to 100 times better angular resolution in the ultraviolet than NASA’s high-resolution space telescope – the Solar Dynamics Observatory. This would be just enough to start getting some answers from the Sun’s corona.
Nice.