Veloce uses precision pressure control for the Veloce echelle spectrograph

by Dr. James Gilbert

This “Alicats in the Wild” blog post comes courtesy of our Australian distributor, Duff & Macintosh Pty Ltd. Veloce integrates a highly-customized Alicat closed-volume pressure controller for stable precision pressure control of air inside the instrument.

Precision pressure control for the Veloce echell spetrograph

Interior of the Veloce echelle spectrograph, where precision pressure control is critical.

Veloce echelle spectrograph interior – James Gilbert (ANU)

Veloce was built primarily to detect stars that are ‘wobbling’ due to the gravitational tug of one or more orbiting planets. Veloce is based on a technique called Precision Radial Velocity Spectroscopy – we measure the spectral content of starlight and look for minuscule colour shifts (Doppler shifts) caused by the periodic motion of the star.

Anglo-Australian Telescope at Siding Spring Observatory

Anglo-Australian Telescope at Siding Spring Observatory, NSW, Australia – Angel Lopez-Sanchez (AAO-MQU)

It is absolutely critical to control the measurement errors of the instrument, because the signal we are looking for is so small. We are looking for changes of 1/1500 pixels on our image detector, which is a physical distance of something like ten nanometers on the detector surface. This corresponds to a radial velocity measurement of around 1 m/s, meaning we can measure the speed of a star’s motion down to slow walking pace.  This is sufficient to detect planets not too dissimilar to Earth, that may be in the so-called ‘habitable zone’ of the host star.

We approached Alicat because we needed industrial-grade reliability as well as science-grade performance.

AAT Dome at Siding Spring Observatory

AAT Dome at Siding Spring Observatory, NSW, Australia – Angel Lopez-Sanchez (AAO-MQU)

If the air pressure in the instrument changes, then the refractive index at the surface of the optics changes, and our signals are completely drowned out.  We decided to shield the instrument from atmospheric pressure variations by keeping it at a fixed positive pressure at all times. We needed a stability of 5 mbar, with a goal of 1 mbar, in an 1800-litre volume with significant leaks. We approached Alicat because we needed industrial-grade reliability as well as science-grade performance. Alicat rose to the challenge and modified one of their standard products to provide an affordable solution to our requirements. The instrument has been operating for several months already, and its internal pressure has not ventured beyond 0.3 mbar of our setpoint, which is fabulous.

Veloce is now fully commissioned and has already observed its first planetary systems. Initially, we are looking at known candidates found by NASA’s Transiting Exoplanet Survey Satellite (TESS). Veloce is currently the best instrument in the world for some of these targets, and may be the first to confirm the existence and accurately measure the mass of planets we previously didn’t know existed.

While there are many factors that have made the Veloce project a success, we would certainly not be able to fulfill our science goals without the tight pressure regulation provided by our Alicat pressure controller.

Alicat dual-valve pressure controller

Alicat dual-valve precision pressure controller

Alicat supplied Veloce with a dual-valve pressure controller that can detect the smallest deviation from the chosen pressure setpoint within 5 ms.

When the pressure controller detects such deviations, it the setpoints of both its inlet and outlet valves in order to return the volume to setpoint within 50 ms. This ensures that Veloce never sees more than 0.3 mbar total pressure deviation across its 1800-liter volume.

To prevent unwanted thermal disturbances, the sensor for precision pressure control was physically isolated from the valve and flow path, so that the controller itself could be mounted outside the spectrograph chamber.

 

Background

Dr. James Gilbert was the technical lead for the Australian National University’s development of the Veloce echelle spectrograph, which is now installed on the 3.9-meter Anglo-Australian Telescope at the Siding Spring Observatory in New South Wales, Australia.