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Mapping the universe at 30 Terabytes a night

Jeff Kantor, on building and managing a 150 Petabyte database

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Interview It makes for one heck of a project mission statement. Explore the nature of dark matter, chart the Solar System in exhaustive detail, discover and analyze rare objects such as neutron stars and black hole binaries, and map out the structure of the Galaxy.

The Large Synoptic Survey Telescope (LSST) is, in the words of Jeff Kantor, LSST data management project manager, "a proposed ground-based 6.7 meter effective diameter (8.4 meter primary mirror), 10 square-degree-field telescope that will provide digital imaging of faint astronomical objects across the entire sky, night after night." Phew.

When it's fully operational in 2016, the LSST will: "Open a movie-like window on objects that change or move on rapid timescales: exploding supernovae, potentially hazardous near-Earth asteroids, and distant Kuiper Belt Objects.

"The superb images from the LSST will also be used to trace billions of remote galaxies and measure the distortions in their shapes produced by lumps of Dark Matter, providing multiple tests of the mysterious Dark Energy."

In its planned 10-year run, the LSST will capture, process and store more than 30 Terabytes (TB) of image data each night, yielding a 150 Petabytes (PB) database. Talking to The Reg, Kantor called this the largest non-proprietary dataset in the world.

Data management is one of the most challenging aspects of the LSST. Every pair of 6.4GB images must be processed within 60 seconds in order to provide astronomical transient alerts to the community. In order to do this, the Data Management System is composed of a number of key elements. These are:

  • the Mountain/Base facility, which does initial data reduction and alert generation on a 25 TFLOPS Linux cluster with 60PB of storage (in year 10 of the survey)
  • a 2.5 Gbps network that transfers the data from Chile (where the telescope itself will be based) to the U.S. and within the US
  • the Archive Center, which re-reduces the data and produces annual data releases on a 250 TFLOPS Linux cluster and 60PB of storage (in year 10 of the survey)
  • the Data Access Centers which provide access to all of the data products as well as 45 TFLOPS and 12 Petabytes of end user available computing and storage.

So what's a time-critical system of this magnitude written in?

The data reduction pipelines are developed in C++ and Python. They rely on approximately 30 off-the-shelf middleware packages/libraries for parallel processing, data persistence and retrieval, data transfer, visualization, operations management and control, and security. The current design is based on MySQL layered on a parallel, fault-tolerant file system.

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Latest Comments

Big piccies

Well, my maths will probably get flamed but what the hey.

Doing some rough numbers and assuming JPEG's, low compression and 32-bit colour depth then these pictures have a resolution of about 120000 x 90000 pixels.

That would give a photo-quality print that was approimately 8 meters by 6 meters.

Crikey!

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No JPEG....

They have to use non-lossy compression for this, so the figures won't be that great (compared with JPEG or whatever we are using in 10 years time), but still a good percentage I would think.

Not lossy because you may compress out something faint but important. Which is most of what astronomy is about.

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Why is this wrong?

150 Petabytes over 10 years is closer to 42 Terabytes per 24 hours. Not 30.

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