PR says they will equip their Arkyd 100 series with a cutting edge Laser Communication system. Will they be able to use multiple Arkyd's as an Interferometer utilizing the Communication system?If they can do that they can exponentially increase their optical resolution.
Quote from: ChefPat on 06/21/2013 03:38 amPR says they will equip their Arkyd 100 series with a cutting edge Laser Communication system. Will they be able to use multiple Arkyd's as an Interferometer utilizing the Communication system?If they can do that they can exponentially increase their optical resolution.I'd say no: to perform optical interferometry requires extremely precise beam combination and extremely precise control over the effective separation of elements of the interferometer which means optical delay lines to compensate for distance variations. And these need to be precise down to (from memory) 1/4 wavelength . . .
But it sounds like a simple strategy. Sit and wait; point and shoot; count and calculate. Repeat.
Indeed. But why be complicated? Spotting objects moving against the background is straight-forward and largely automated (subtract 2nd shot from 1st and anything that isn't zero is moving).
They have not yet told the public sufficient information about the resolution of the camera, nor the strategy for looking, which is why, I suppose, it is being speculated about on this thread.
Yup. Not just resolution but a whole gamut of important things: the per pixel point spread function of the optics, noise floors, dark levels, mapping of pixels onto sky coordinates, what their data release strategy is (will they release FITS files, etc).
Neither the Keck people nor the JPL people (nor Planetary Resources) thought of the bagging idea. If you can guess who, I'll give you a prize (okay, the prize is just satisfaction). As a hint, it's a NASA group. 1 point for guessing the NASA center, 10 points for guessing the group within that NASA center.(And bagging it isn't the only thing considered, either.)
In fact, just the other day, they announced that they want to send up another cubesat, this time to look for planets in other solar systems. So there's that immediate change of plans temporally related to the current rejection of the heist in the halls of Congress.
AcknowledgementsThe authors would like to thank Min Qu and Jon Chrone with Analytical Mechanics Associates, Inc. (AMA, Inc.) for their outstanding trajectory analysis in support the ARM concept. Additionally, we would like to thank the personnel in the Advanced Concepts Laboratory at NASA LaRC, Dave Helton, Josh Sams, Bob Evangelista, Christopher Keblitis, and Kevin Greer (all employees of AMA, Inc.) for the terrific computer-generated graphics included in this paper. We also like to thank Dave North (NASA LaRC), Christopher Keblitis, and KISS for the capture mechanism sketches and drawings, along with Jim Strope for his beautiful photograph of the Murchison CM2 carbonaceous chondrite meteorite fragment. Finally, the authors would like recognize and thank the Keck Institute for Space Studies (KISS). KISS hosted the ARM Study in 2011 and 2012 and was instrumental in advancing the concept of returning a NEA to cislunar space .
Quote from: JohnFornaro on 06/21/2013 01:51 pm In fact, just the other day, they announced that they want to send up another cubesat, this time to look for planets in other solar systems. So there's that immediate change of plans temporally related to the current rejection of the heist in the halls of Congress.You realize these satellites are designed to be multifunctional, right?
Their camera's got to be higher resolution than what you suppose, which would not be able to see the rock that is intended to be retrieved.
Quote from: Robotbeat on 06/21/2013 11:03 pmNeither the Keck people nor the JPL people (nor Planetary Resources) thought of the bagging idea. If you can guess who, I'll give you a prize (okay, the prize is just satisfaction). As a hint, it's a NASA group. 1 point for guessing the NASA center, 10 points for guessing the group within that NASA center.(And bagging it isn't the only thing considered, either.)From the paper I posted in the NEA forum.QuoteAcknowledgementsThe authors would like to thank Min Qu and Jon Chrone with Analytical Mechanics Associates, Inc. (AMA, Inc.) for their outstanding trajectory analysis in support the ARM concept. Additionally, we would like to thank the personnel in the Advanced Concepts Laboratory at NASA LaRC, Dave Helton, Josh Sams, Bob Evangelista, Christopher Keblitis, and Kevin Greer (all employees of AMA, Inc.) for the terrific computer-generated graphics included in this paper. We also like to thank Dave North (NASA LaRC), Christopher Keblitis, and KISS for the capture mechanism sketches and drawings, along with Jim Strope for his beautiful photograph of the Murchison CM2 carbonaceous chondrite meteorite fragment. Finally, the authors would like recognize and thank the Keck Institute for Space Studies (KISS). KISS hosted the ARM Study in 2011 and 2012 and was instrumental in advancing the concept of returning a NEA to cislunar space .
@PlanetaryRsrcs: The A3 will help test the #ARKYD technology! It will launch from the ISS in early 2014. You're the first to know! http://t.co/YIvAtLVYeB
"launch from the ISS" .. that's the first time I've heard that!Good work Planetary Resources.
Ok I'll have one more guess then.GRC COMPASS.
Quote from: JohnFornaro on 06/20/2013 04:57 pmTheir camera's got to be higher resolution than what you suppose, which would not be able to see the rock that is intended to be retrieved. This isn't correct at all. You are confusing the ability to resolve an asteroid with the ability to detect it. You can detect an asteroid, characterize it's orbit and obtain light curves and spectra without being able to resolve it. The vast majority of asteroids and KBOs are only known as point sources.Asteroid surveys favor large FOVs over high resolution.
What about the rate of lazy tumbling?
Diameter?
Mass?
A flickering point of light can only give but so much info.