I'm wondering about how the 'java objects' of Cache will be used for the GAIA data.
I suppose the raw data is the billion pixel images but the science happens when those pixels move when you take subsequent pictures at a different phase of orbit.
The moving pixels become the java objects, with a record on which images and where they appear, current best estimate of location.
Then there spectroscopy data, for detecting a star's composition and velocity relative to GAIA and doppler spectroscopy which can detect the wobble of the star which may indicate planets.
I assume the spectroscopy is not collected for all billion target stars and not as often as the optical images.
A good match for the MV model, irregular repeating or even absent sets of data.
Billion star survey, I just love this 21st century tech.
Jeremy Thomson