The Maunakea Observatories instrumentation programs are the key to the telescopes’ continued ranking as the most scientifically productive in the world. Each instrument can be fitted onto the telescope of their respective observatory to give scientists new, advanced capabilities for a highly specialized research. SPIRou (SpectroPolarimètre InfraRouge) belongs to the next generation of astronomy instruments with the goal of finding Earth like planets in the habitable zones of nearby red stars. SPIRou uses a technique called radial velocity coupled with polarimetry in the infrared to detect the tiny wiggle in a star, which indicates the presence of planets, to very small levels.
“SPIRou is a giant leap forward for the search for planets” says Claire Moutou, astronomer and SPIRou instrument scientist at CFHT. “With its high precision and ability to look at infrared light, we will discover planets that were undiscoverable before. It’s very exciting.”
Along with professional astronomers, dozens of Hawaii State Department of Education high school students are eagerly anticipating the chance to use SPIRou through the observatories’ Maunakea Scholars program, which gives observing time and mentorship to students statewide. Many of the Scholars’ innovative project proposals have been beyond the boundaries of current technology, until today.
SPIRou looks at the rainbow or spectra of nearby red stars. These stars, called M dwarfs, are very cool, roughly 1000 to 2000 degrees cooler than the Sun. To measure the spectra of these stars, SPIRou operates in the infrared, wavelengths of light longer (thus redder) than the light humans can see with their eyes. As the planet orbits its star, the gravity of the planet pulls the star ever so slightly causing a back and forth motion of the star over a full revolution of the planet. SPIRou will detect the speed of this motion down 2.25 miles per hour. This is technologically very challenging.
“The cameras on SPIRou are cutting edge technology” says Greg Barrick, project engineer for SPIRou at CFHT. “No one else on Earth right now has cameras that can make these measurements.”
After its arrival at the summit, SPIRou will be unpacked and reassembled, a delicate process that will take a several months. Once it is reassembled, the instrument will undergo testing in the lab and on the sky before being declared ready for science. If all goes according to plan, CFHT anticipates SPIRou capturing its first light from an M star in spring 2018.