Most Powerful Solar Telescope on Earth Rises Atop Hawaiian Volcano

by Bob King on May 7, 2014

Construction on the new observatory on the summit of the Haleakala Crater on Maui, Hawaii this February. Credit: National Solar Observatory

Construction on the new observatory on the summit of the Haleakala Crater on Maui, Hawaii this February. The observatory is expected to be completed in 2019. Credit: National Solar Observatory / Ruth Kneale

Rising 10,000 feet above the sunburned faces of 2.2 million tourists a year, the largest solar telescope on the planet is under construction atop Haleakala Crater in Maui, Hawaii. Never mind all those admonitions about never staring at the sun. Astronomers can’t wait for the chance. 

Named for the late Senator Daniel Inouye, the Daniel K. Inouye Solar Telescope or DKIST will be the world’s premier ground-based solar observatory in the world. With its 4-meter (157.5-inch) primary mirror, DKIST is capable of distinguishing features down to 0.03 arc seconds or just 20-70 km (12-44 miles) wide at the sun’s surface. To achieve such fantastic resolutions the telescope will employ the latest adaptive optics technology to cancel the blurring effects of the atmosphere using a computer-controlled deformable mirror. 

capture the evolution of sunspot fine structure and finally understand its physical origin. (Image from the NSO Dunn Solar Telescope, courtesy of Thomas Rimmele.)

Extreme closeup of a sunspot showing the dark, central umbra (top) feathery penumbra and individual granules or hot gas. DKIST will capture the evolution of sunspot fine structure and finally understand its physical origin. Credit: NSO Dunn Solar Telescope, courtesy of Thomas Rimmele

Consider that the smallest features visible in large amateur telescopes are solar granules, columns of hot gas rising up from the sun’s interior. Each spans about 930 miles (1,500 km) and together give the sun’s surface the texture of finely-etched glass. DKIST will resolve features more than 60 times smaller. The current largest sun-dedicated telescope is the McMath-Pierce Solar Telescope , which has kept a steady eye on the home star with its 63-inch (1.6-meter) mirror since 1962 from Kitt Peak, Arizona.

DKIST cutaway showing light entering the top of the dome and gathered by the primary mirror, which is then reflected to a secondary mirror, which reflects the light to a science gallery below. Inset shows the light path in greater detail including the deformable mirror that will cancel the blurring effects of bad atmospheric seeing. Credit: L. Phelps

Observatory cutaway showing light entering the top of the dome and gathered by the primary mirror, which is reflected to a secondary mirror and from there through a series of smaller mirrors to the science gallery below. Inset shows the light path in greater detail including the deformable mirror that will cancel the blurring effects of atmospheric turbulence. Notice that the secondary mirror is offset with no obstructions between it and the primary mirror that would otherwise lessen the telescope’s ability to resolve fine detail. Credit: L. Phelps with enhancements by the author

DKIST will focus on three key areas: What is the nature of solar magnetism; how does that magnetism control our star; and how can we model and predict its changing outputs that affect the Earth? Astronomers hope to clearly resolve  solar flux tubes – magnetic field concentrations near the sun’s surface – thought to be the building blocks of magnetic structures in the atmosphere.

We still lack a complete understanding of how energy in the sun’s turbulent, churning interior is transferred to magnetic fields. Earth’s magnetic field is about 0.5 gauss at the surface. Fields within sunspots can range from 1,500 to 3,000 gauss – about the strength of a bar magnet but across a region several times larger than Earth.

A test of the Visible Broadband Imager (VBI) interference filter that will be used with DKIST

A test of the DKIST Visible Broadband Imager interference filter in 2012 shows material flowing from a sunspot’s outer penumbra into the surrounding solar gases. Credit: NSO

A better understanding of small scale magnetic structures, too tiny to be resolved with current telescopes, will help make sense of broader phenomena like sunspot formation, the heating of the solar corona and why the sun’s energy output varies. The solar constant, the amount of radiation we receive from the sun, increases with an increase in solar activity like spots and flares. Since the smallest magnetic elements are the biggest contributors to this increase, DKIST will be the first telescope able to image and study these structures directly, helping astronomers understand how variations in the sun’s output can lead to climate changes.

Left - Solar photosphere showing bright structures between granules  associated with magnetic fields. RIght - Computer model of a magnetic flux tube rising from the convective  zone into the photosphere. These are believed to be an important  conduit for energy flowing from the solar interior to the hot outer  atmosphere. Flux tubes are below the limit of resolution  in current telescopes. Credit: Paxman, Seldin, Keller / O. Steiner

Left – Solar photosphere showing bright structures between granules associated with magnetic fields bubbling up from below. Right – Computer model of a magnetic flux tube rising from the convective
zone into the photosphere. Flux tubes are believed to be an important
conduit for energy flowing from the solar interior to the hot outer
atmosphere but are below the limit of resolution
in current telescopes. Credit: Paxman, Seldin, Keller / O. Steiner

DKIST will do its work on rapid times scales, taking images once every 3 seconds. For comparison, NASA’s orbiting Solar Dynamics Observatory takes pictures in 8 different wavelengths every 10 seconds, STEREO one image every 3 minutes and SOHO (Solar Heliospheric Observatory) once every 12 minutes. The speedy shooting ability will help DKIST resolve rapidly evolving structures on the sun’s surface and lower atmosphere in a multitude of wavelengths of light from near-ultraviolet to deep infrared thanks to the the extraordinarily clean and dry air afforded by its high altitude digs.

DKIST is under construction in the observatory complex on Haleakala Crater in Maui, Hawaii. The Maui Space Surveillance is the large structure near top center. Photo take Oct. 2013. Credit: Bob King

DKIST is under construction in the observatory complex on Haleakala Crater in Maui, Hawaii. The Maui Space Surveillance Complex is the large structure right of center. Photo take Oct. 2013. Credit: Bob King

The new solar telescope will be in excellent company not far from the current Mees Solar Observatory and a stone’s throw from the Panoramic Survey Telescope and Rapid Response System (Pan-STARRS) telescope, the 79-inch (2-meter) Faulkes Telescope North and Maui Space Surveillance Complex which keeps an eye on man-made orbital debris. Tourists to Mt. Haleakala, a popular destination for tourists, can watch it take shape in the next few years while enjoying a hike in the cool air for which Haleakala is famous.

On August 31, 2012 a long filament of solar material that had been hovering in the sun's atmosphere, the corona, erupted out into space at 4:36 p.m. EDT. The coronal mass ejection, or CME, traveled at over 900 miles per second.

On August 31, 2012 a long filament of solar material erupted out into space as a coronal mass ejection, or CME, traveling at over 900 miles per second. By probing solar gases at high resolution and rapid time scales using DKIST’s high power optics and spectrographs, astronomers hope to better understand the first stirrings of these huge outbursts of solar energy. Credit: NASA

I first heard about the DKIST telescope from a burly stranger with fierce-looking tattoos. My wife and I vacationed in Maui last fall. One afternoon, while watching surfers ride the waves near the beach town of Paia, this big guy overheard us mention Duluth (Minn.), our hometown. He said he’d lived in Duluth for a time before moving to Hawaii and offered us a beer. We got to talking and learned he worked safety inspection at at the “biggest solar telescope in the world”, making the hour-long drive up the mountain 5 days a week.  I checked it out and he was absolutely right.

The Daniel K. Inouye Solar Telescope (formerly the Advanced Technology Solar Telescope) is being developed by a consortium led by the National Solar Observatory and comprising the University of Chicago, the New Jersey Institute of Technology, University of Hawaii, the High Altitude Observatory, NASA, the U.S. Air Force and others. For more details on the project, click HERE.

There’s poetry in building a large solar observatory on an island known for its sunny, warm climate. While vacationers flop out on Kaanapali Beach to vanquish the mid-winter chills, astronomers 50 miles away and 10,000 feet up will be at work coaxing secrets from the fiery ball of light that illuminates surf and scope alike.

About 

I'm a long-time amateur astronomer and member of the American Association of Variable Star Observers (AAVSO). My observing passions include everything from auroras to Z Cam stars. Every day the universe offers up something both beautiful and thought-provoking. I also write a daily astronomy blog called Astro Bob.

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