First all-sky map of the edge of the solar system
The map will provide a deeper understanding of the Sun's interaction with the galaxy.
January 13, 2009
Provided by the Southwest Research Institute, Boulder, Colorado
January 13, 2009
This IBEX data image shows a dark sky map with the first orbit’s coincidence counts from hydrogen atoms at speeds from about 100,000 (161,000 km) to 36 million miles (58 million km) per hour. The IBEX team is collecting additional orbit data to expose adjacent swaths of the sky to reveal the edge of our solar system.
Photo by SWRI, San Antonio, Texas
Following two months of commissioning, during which the spacecraft and sensors were tuned for optimum mission performance, the Interstellar Boundary Explorer (IBEX) spacecraft began gathering data to build the first maps of the edge of the heliosphere, the region of space influenced by the Sun.
IBEX is using energetic neutral atom (ENA) imaging to create the first global maps of interactions between the million miles per hour (1,609,000 km/h) solar wind blown out in all directions by the Sun and the low-density material between the stars, known as the interstellar medium.
The maps are built by two ENA cameras, which collectively measure energetic neutral atoms coming in from the edge of the solar system with speeds from about 100,000 miles per hour (161,000 km/h) to some 36 million miles per hour (58 million km/h). Each sensor uses a charge-exchange process that converts incoming neutral atoms into charged ions so they can be analyzed and detected.
The sensors look out from opposite sides of the spacecraft in directions perpendicular to the Sun-pointed spin axis. As the spacecraft spins at four revolutions per minute, the measured ENAs fill in the pixels to build a circular swath that appears as a crescent on the map. As the spacecraft's spin axis tracks the Sun, the swaths move across the sky to complete the image.
"We are seeing fabulous initial results from IBEX, but, just as artisans use looms to build up colorful textiles by weaving one thread at a time, the IBEX sensors also need time - six months - to build up a complete map of the sky," said Dr. David McComas, IBEX principal investigator and senior executive director of the Space Science and Engineering Division at Southwest Research Institute in San Antonio, Texas. "So far, the intricate pattern of this fascinating interaction is only just beginning to disclose itself to us."
IBEX will enable researchers to examine the structures and dynamics of the outer heliosphere and to investigate the acceleration and propagation of charged particles in this complex and important region. IBEX also will address a serious challenge facing manned exploration by studying the region that shields Earth from the majority of galactic cosmic ray radiation.
"The space physics community is holding its collective breath waiting for these maps, which will provide a much deeper understanding of the Sun's interaction with the galaxy," said McComas. "We expect the first complete image, due this summer, to tell us a great deal about the heliosphere's fundamental nature."