Far cheaper and plausible than the Hubble satellite-telescope, no?Heiwa wrote: I wonder what clowns waste tax payers money with this.

Far cheaper and plausible than the Hubble satellite-telescope, no?Heiwa wrote: I wonder what clowns waste tax payers money with this.
I will thus just visually check, again, weather permitting, how anything, incl. the ISS, can appear and disappear SW during 2 minutes above me. When NASA told me earlier, several times, that the ISS was passing above I watched and ... sometimes some strange thing up in the sky passed. I really wonder what it could be? A diameter 100 meters lightweight satellite?Time: Sun Apr 07/10:05 PM, Visible: 2 min, Max Height: 82 degrees, Appears: SW, Disappears: SW
Source: http://www.jwst.nasa.gov/faq.html#whatkindThe best example of weight reduction is the primary mirror, which takes up a considerable fraction of the total mass budget. The mirror has to be very accurately shaped. Any variations from the perfect shape of the mirror have to be less than a fraction of the observing wavelengths, which start at about 0.1 micrometer (in the ultraviolet) for Hubble and 0.6 micrometer (gold light) for Webb. (For comparison, the average thickness of a human hair is about 100 micrometers.) To keep the mirror in such a perfect shape, Hubble has a thick, solid glass mirror with a mass around 1000 kg (2200 lbs on Earth).
Webb's mirror will consist of 18 thin, lightweight beryllium mirror segments, which will be kept in the right shape and place by a large number of adjustors attached to a stiff backing frame. Including the backing frame, the 18 segments of the Webb primary mirror total about 625 kg. These kinds of technologies, which were not available at the time Hubble was built, will be used throughout Webb.
There is apparently also a big sunshade, i.e. parasol to protect the telescope from the sun:The James Webb Space Telescope includes four scientific instruments: the Near Infrared Camera (NIRCam), the Near-Infrared Spectrograph (NIRSpec), the Mid-Infrared Instrument (MIRI), and the Fine Guidance Sensor/ Near InfraRed Imager and Slitless Spectrograph (FGS-NIRISS).
I really wonder what the space parasol will look like and what it is made of. I cannot see it on the picture of the James Webb Space Telescope:The large sunshade will protect the telescope from heating by direct sunlight, allowing it to cool down to a temperature below 50 Kelvin (-223° C or -370° F) by passively radiating its heat into space. The definition of the Kelvin temperature scale is that 0 K is "absolute zero," the lowest possible temperature. Water freezes 32 degree F, 0 degree C or about 273 K. The near-infrared instruments (NIRCam, NIRSpec, FGS/NIRISS) will work at about 39 K (-234° C or -389° F) through a passive cooling system. The mid-infrared instrument (MIRI) will work at a temperature of 7 K (-266° C or -447° F), using a helium refrigerator, or cryocooler system.
Cool, Heiwa!Heiwa wrote:So today with the right astrophotography equipment installed on my roof terrasse close to Nice, France, I could easily make a picture of the ISS that according below message from NASA just received will pass above my house:
Time: Sun Apr 07/10:05 PM, Visible: 2 min, Max Height: 82 degrees, Appears: SW, Disappears: SW
I'm excited!NASA wrote:Time: Sun Apr 07/10:06 PM, Visible: 1 min, Max Height: 44 degrees, Appears: WSW, Disappears: W
Brian,
From Wikipedia on BerylliumHeiwa wrote:The James Webb Space Telescope 18 segments mirror is fanta(sy)stic!
Each segment weighs only 35 kgs!
Source: http://www.jwst.nasa.gov/faq.html#whatkindThe best example of weight reduction is the primary mirror, which takes up a considerable fraction of the total mass budget. The mirror has to be very accurately shaped. Any variations from the perfect shape of the mirror have to be less than a fraction of the observing wavelengths, which start at about 0.1 micrometer (in the ultraviolet) for Hubble and 0.6 micrometer (gold light) for Webb. (For comparison, the average thickness of a human hair is about 100 micrometers.) To keep the mirror in such a perfect shape, Hubble has a thick, solid glass mirror with a mass around 1000 kg (2200 lbs on Earth).
Webb's mirror will consist of 18 thin, lightweight beryllium mirror segments, which will be kept in the right shape and place by a large number of adjustors attached to a stiff backing frame. Including the backing frame, the 18 segments of the Webb primary mirror total about 625 kg. These kinds of technologies, which were not available at the time Hubble was built, will be used throughout Webb.
http://en.wikipedia.org/wiki/BerylliumBeryllium is a steel gray and hard metal that is brittle at room temperature and has a close-packed hexagonal crystal structure.
I was pretty surprised at how realistic it all can look.