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Interface Region Imaging Spectrograph (IRIS) - Frequently Asked Questions (FAQs)
June 12, 2013
 

Artist's concept of the IRIS satellite in orbit. › View larger
Artist's concept of the Interface Region Imaging Spectrograph (IRIS) satellite in orbit.
How big is the IRIS satellite?

IRIS is approximately 7 feet (2.1 meters) long and about 12 feet (3.7 meters) across with its solar panels deployed.

How much does IRIS weigh?

The IRIS observatory weighs 403 pounds.

Where will IRIS launch and what launch vehicle will be used?

IRIS will launch from Vandenberg Air Force Base in Calif. It will be deployed from an Orbital Sciences L-1011 aircraft aboard a Pegasus XL rocket at an altitude of 39,000 feet over the Pacific Ocean about 100 miles Northwest of Vandenberg Air Force Base.

When will IRIS launch?

IRIS is scheduled to launch on June 26, 2013. Deployment from the Pegasus XL rocket is targeted for 7:27 pm PDT in the middle of a five-minute launch window.

How long is the IRIS mission?

Two years.

Hinode views the lower regions of the sun's atmosphere, the interface region, which a new mission called the Interface Region Imaging Spectrograph will study in exquisite detail. › View larger
This image from the joint NASA-Japan Aerospace Exploration Agency's Hinode mission shows the lower regions of the sun's atmosphere, the interface region, which a new mission called the Interface Region Imaging Spectrograph, or IRIS, will study in exquisite detail. Credit: NASA&JAXA/Hinode
What is IRIS going to study? Why?

IRIS is a NASA Small Explorer Mission that will observe a region that lies between the sun's 10,000 degree, white-hot, visible surface, the photosphere, and the much hotter multi million-degree outer atmosphere of the sun, the corona. The sun's dynamically changing chromosphere and transition region make up the key "interface region" that IRIS will study that lies between the photosphere and corona.

IRIS will observe how solar gases move, gather energy, and heat up through the interface region, information that is key to understanding what heats the sun's corona. IRIS improves our understanding of the interface region where most of the sun's ultraviolet emission is generated that impacts the near-Earth space environment and Earth's climate.

All the energy that drives solar activity travels through the interface region and IRIS observations will help our understanding of what causes the ejection of solar material – from the steady stream of the solar wind to larger, explosive eruptions such as coronal mass ejections, or CMEs – that travels toward Earth and causes space weather, which can disrupt human technology.

Graphic of IRIS satellite with components labeled. › View larger
An artist rendition of the Interface Region Imaging Spectrograph (IRIS), with major components labeled. Credit: NASA/LMSAL
What instrument is on IRIS? What will it study?

IRIS carries a single instrument, an ultraviolet telescope that feeds an imaging spectrograph. The telescope's primary mirror has a diameter of about eight inches. The images from IRIS's telescope will record observations of material at specific temperatures, ranging from 5000 K to 65,000 K (and up to 10 million K during solar flares) in order to observe material on the sun's surface and in the chromosphere and transition region.

The high-resolution images and spectra provided by IRIS will make it possible for scientists to use advanced computer models to unravel how matter, light and energy move fro the sun's 6,000 Kelvin surface to its million Kelvin corona.

Why can't NASA just use its existing fleet of solar spacecraft to study this mysterious region on the sun?

IRIS is unique in that it's the first mission designed to simultaneously observe the range of temperatures specific to the chromosphere and transition region not only at very high resolution, as small as 150 miles across the sun, but also at the quick rate of once every few seconds. Such capability does not exist on other NASA missions.

IRIS will join the Solar Dynamics Observatory (SDO) mission and the joint NASA/JAXA's Hinode mission. Together they will explore how the solar atmosphere works and impacts Earth, with SDO and Hinode monitoring the solar surface and outer atmosphere and IRIS watching the region in between.

Diagram of sun synchronous polar orbit. › View larger
IRIS will travel in a polar, sun-synchronous orbit. This means it will travel around Earth, crossing nearly directly over the poles, in such a way that it crosses the equator at the same local time each day.
What orbit will IRIS operate in and why?

IRIS will travel in a polar, sun-synchronous orbit. This means it will travel around Earth, crossing nearly directly over the poles, in such a way that it crosses the equator at the same local time each day. The spacecraft's orbit will place it at about 390 miles (620 km) above the Earth's surface at its closest point, and at 420 miles (670 km) at the farthest. This orbit allows for eight months of continuous observations each year and maximizes eclipse-free viewing of the sun.

Who are the major contributors to the IRIS mission? What are their roles?

Lockheed Martin Space Systems ATC in Palo Alto, Calif., designed and built the IRIS observatory with support from the company's Civil Space line of business and major partners, the Smithsonian Astrophysical Observatory and Montana State University.

NASA's Goddard Space Flight Center in Greenbelt, Md., manages the Explorers Program.

NASA's Ames Research Center in Moffett Field, Calif., is responsible for mission operations and the ground data system.

The Norwegian Space Centre and NASA's Near Earth Network will provide the ground stations to support the IRIS mission using antennas at Svalbard, Norway, Fairbanks, Alaska, McMurdo, Antarctica and Wallops Island, Virginia.

The Joint Science Operations Center, run by Stanford University and Lockheed Martin, is responsible for managing the science data.

NASA's Launch Services Program at Kennedy Space Center, Fla., is responsible for launch management.
IRIS Mission logo
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IRIS Mission Logo. Credit: LMSAL
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Page Last Updated: July 28th, 2013
Page Editor: NASA Administrator