NASA Spacecraft Gets Boost From Jupiter For Pluto Encounter

NASA's New Horizons spacecraft successfully completed a flyby of Jupiter early this morning (Feb. 28), using the massive planet's gravity to pick up speed for its 3-billion mile voyage to Pluto and the unexplored Kuiper Belt region beyond.

"We're on our way to Pluto," said New Horizons Mission Operations Manager Alice Bowman of Johns Hopkins University Applied Physics Laboratory (APL), Laurel, Md. "The swingby was a success; the spacecraft is on course and performed just as we expected."

New Horizons came within 1.4 million miles of Jupiter at 12:43 a.m. EST, placing the spacecraft on target to reach the Pluto system in July 2015. During closest approach, the spacecraft could not communicate with Earth, but gathered science data on the giant planet, its moons and atmosphere.

At 11:55 a.m. EST mission operators at APL established contact through NASA's Deep Space Network and confirmed New Horizons' health and status.

The fastest spacecraft ever launched, New Horizons is gaining nearly 9,000 mph from Jupiter's gravity - accelerating to more than 52,000 mph. The spacecraft has covered approximately 500 million miles since its launch in January 2006 and reached Jupiter faster than seven previous spacecraft to visit the solar system's largest planet. New Horizons raced through a target just 500 miles across, the equivalent of a skeet shooter in Washington hitting a target in Baltimore on the first try.

New Horizons has been running through an intense six-month long systems check that will include more than 700 science observations of the Jupiter system by the end of June. More than half of those observations are taking place this week, including scans of Jupiter's turbulent atmosphere, measurements of its magnetic cocoon, surveys of its delicate rings, maps of the composition and topography of the large moons Io, Europa, Ganymede and Callisto, and a detailed look at volcanic activity on Io.

"We designed the entire Jupiter encounter to be a tough test for the mission team and our spacecraft, and we're passing the test," says New Horizons Principal Investigator Alan Stern from the Southwest Research Institute in Boulder, Colo. "We're not only learning what we can expect from the spacecraft when we visit Pluto in eight years, we’re already getting some stunning science results at Jupiter - and there's more to come."

While much of the close-in science data will be sent back to Earth during the coming weeks, the team also downloaded a sampling of images to verify New Horizons' performance.

The outbound leg of New Horizons' journey includes the first-ever trip down the long "tail" of Jupiter's magnetosphere, a wide stream of charged particles that extends more than 100 million miles beyond the planet. Amateur backyard telescopes, the giant Keck telescope in Hawaii, NASA's Hubble Space Telescope and Chandra X-Ray Observatory and other ground and space-based telescopes are turning to Jupiter as New Horizons flies by, ready to provide global context to the close-up data New Horizons gathers.

New Horizons is the first mission in NASA's New Frontiers Program of medium-class spacecraft exploration projects. The Applied Physics Laboratory, Laurel, Md., manages the mission for NASA's Science Mission Directorate, Washington. The mission team also includes NASA's Goddard Space Flight Center, Greenbelt, Md.; NASA's Jet Propulsion Laboratory, Pasadena, Calif.; the U.S. Department of Energy, Washington; Southwest Research Institute, Boulder, Colo.; and several corporations and university partners.

Astrophysicists Find Fractal Image Of Sun's 'Storm Season' Imprinted On Solar Wind

Plasma astrophysicists at the University of Warwick have found that key information about the Sun’s 'storm season’ is being broadcast across the solar system in a fractal snapshot imprinted in the solar wind. This research opens up new ways of looking at both space weather and the unstable behaviour that affects the operation of fusion powered power plants.

Fractals, mathematical shapes that retain a complex but similar patterns at different magnifications, are frequently found in nature from snowflakes to trees and coastlines. Now Plasma Astrophysicists in the University of Warwick’s Centre for Fusion, Space and Astrophysics have devised a new method to detect the same patterns in the solar wind.

The researchers, led by Professor Sandra Chapman, have also been able to directly tie these fractal patterns to the Sun’s ‘storm season’. The Sun goes through a solar cycle roughly 11 years long. The researchers found the fractal patterns in the solar wind occur when the Sun was at the peak of this cycle when the solar corona was at its most active, stormy and complex – sunspot activity, solar flares etc. When the corona was quieter no fractal patterns were found in the solar wind only general turbulence.

This means that fractal signature is coming from the complex magnetic field of the sun.

This new information will help astrophysicists understand how the solar corona heats the solar wind and the nature of the turbulence of the Solar Wind with its implications for cosmic ray flux and space weather.

These techniques used to find and understand the fractal patterns in the Solar Wind are also being used to assist the quest for fusion power. Researchers in the University of Warwick’s Centre for Fusion, Space and Astrophysics (CFSA) are collaborating with scientists from the EURATOM/UKAEA fusion research programme to measure and understand fluctuations in the world leading fusion experiment MAST (the Mega Amp Spherical Tokamak) at Culham. Controlling plasma fluctuations in tokamaks is important for getting the best performance out of future fusion power plants.

The research by K.Kiyani, S. C. Chapman, B. Hnat, R. M. Nicol, is entitled "Self- similar signature of the active solar corona within the inertial range of solar wind turbulence" and was published on May 18th 2007 in Phys. Rev. Lett.

The researchers received support and data from STFC (previously PPARC), EPSRC, and the NASA WIND, ACE and ULYSSES teams.

Spaceship Force Field Makes Mars Trip Possible

According to the international space agencies, "space weather" is the single greatest obstacle to deep space travel. Radiation from the sun and cosmic rays pose a deadly threat to astronauts in space. New research shows how knowledge gained from the pursuit of nuclear fusion research may reduce the threat to acceptable levels, making humanity's first mission to Mars a much greater possibility.

The solar energetic particles, although just part of the 'cosmic rays' spectrum, are of greatest concern because they are the most likely to cause deadly radiation damage to the astronauts.

Large numbers of these energetic particles occur intermittently as "storms" with little warning and are already known to pose the greatest threat to man. Nature helps protect the Earth by having a giant "magnetic bubble" around the planet called the magnetosphere.

The Apollo astronauts of the 1960's and 70's who walked upon the Moon are the only humans to have travelled beyond the Earth's natural "force field" – the Earth's magnetosphere. With typical journeys on the Apollo missions lasting only about 8 days, it was possible to miss an encounter with such a storm; a journey to Mars, however, would take about eighteen months, during which time it is almost certain that astronauts would be enveloped by such a "solar storm".

Space craft visiting the Moon or Mars could maintain some of this protection by taking along their very own portable "mini"-magnetosphere. The idea has been around since the 1960's but it was thought impractical because it was believed that only a very large (more than 100km wide) magnetic bubble could possibly work.

Researchers at the Science and Technology Facilities Council's Rutherford Appleton Laboratory, the Universities of York, Strathclyde and IST Lisbon, have undertaken experiments, using know-how from 50 years of research into nuclear fusion, to show that it is possible for astronauts to shield their spacecrafts with a portable magnetosphere - scattering the highly charged, ionised particles of the solar wind and flares away from their space craft.

Computer simulations done by a team in Lisbon with scientists at Rutherford Appleton last year showed that theoretically a very much smaller "magnetic bubble" of only several hundred meters across would be enough to protect a spacecraft.

Now this has been confirmed in the laboratory in the UK using apparatus originally built to work on fusion. By recreating in miniature a tiny piece of the Solar Wind, scientists working in the laboratory were able to confirm that a small "hole" in the Solar Wind is all that would be needed to keep the astronauts safe on their journey to our nearest neighbours.

Dr. Ruth Bamford, one of the lead researchers at the Rutherford Appleton Laboratory, said, "These initial experiments have shown promise and that it may be possible to shield astronauts from deadly space weather."