NEWSALERT: Tuesday, July 11, 2000 @ 0941 GMT
The latest news from Astronomy Now and Spaceflight Now
Space Exploration News From Around the Internet, Updated Every Weekday.
March 3rd, 2000 - Issue #189
http://cnn.com/2000/TECH/space/03/02/venerable.probes/index.html
Space Science News for March 2, 2000
Six billion miles and counting....
Last month NASA received a weak signal from Pioneer 10, twice as far from
the Sun as Pluto and speeding toward the constellation Taurus. The hardy
spacecraft, which is so low on power that it can't transmit and maneuver at
the same time, is still returning data from the outer solar system. This is
also a good time of year to see where Pioneer 10 is heading from your own
back yard.
March 2, 1999
(Launched 2 March 1972)
Distance from Sun (1 March 1999): 72.08 AU
Speed relative to the Sun: 12.24 km/sec (27,380 mph)
Distance from Earth: 10.81 billion kilometers (6.716 billion miles)
Round-trip Light Time: 20 hours 01 minutes
CONGRATULATIONS PIONEER 10! Happy 27th Birthday. Two years into retirement, Pioneer 10 is flying high and still calling home.
The mission formally ended on 31 March 1997 when funding ended in favor of more scientifically productive Heliospheric missions. However, a waiver was given to operate Pioneer 10 as part of the Lunar Prospector controller training program as long as other NASA missions were not interfered with. Pioneer 10 has continued at a much reduced activity level under those guidelines. We are deeply grateful for the gracious way that the Lunar Prospector staff and the DSN have managed this extra burden on their time. The spacecraft is at a distance of >6.7 Billion miles (>72 AU's) and is the farthest out in the opposite direction to which the Sun moves. Voyager 1 passed Pioneer 10 in mileage out of the Solar System on 17 February 1998 but is travelling in the opposite direction.
The low-power Geiger-Tube-Telescope (GTT) instrument still yields valuable scientific data. We also receive data from the Charged Particle Instrument but only for a few hours each week to conserve battery power on Pioneer 10.
Neutron monitors on Earth (e.g., at Climax and Goose Bay) recorded a marked and rapid decrease in cosmic ray intensity of about 4 % during April and early May of 1998. If Pioneer 10 is still inside the heliopause, we can expect a decrease in cosmic-ray intensity at Pioneer 10 to occur during early 1999. The approximate 9 month delay from Earth to Pioneer 10 corresponds to the distance of ~72 AU covered by the solar wind assuming a speed of 450 km/s. If Pioneer10 has passed outside the heliopause into interstellar space, then the decrease in cosmic intensity will not be observed at Pioneer 10.
The battery reading is very low - perhaps at a minimum. Pioneer 10 persists longer than ever conceived or expected. Stay tuned!
Pioneer 10 will continue into interstellar space, heading generally for the red star Aldebaran, which forms the eye of Taurus (The Bull). Aldebaran is about 68 light years away and it will take Pioneer over 2 million years to reach it.
Project Manager: Dr. Lawrence Lasher
STATUS UPDATED: 8 February 1999
Distance from Sun (1 February 1999): 71.88 AU Speed relative to the Sun: 12.24 km/sec (27,380 mph) Distance from Earth: 10.70 billion kilometers (6.646 billion miles) Round-trip Light Time: 19 hours 49 minutes
PIONEER 10 CARRIES ON! One more successful precession maneuver to point the spacecraft to Earth was accomplished on 6-8 February 1999.
The mission formally ended on 31 March 1997 when funding ended in favor of more scientifically productive Heliospheric missions. However, a waiver was given to operate Pioneer 10 as part of the Lunar Prospector controller training program as long as other NASA missions were not interfered with. Pioneer 10 has continued at a much reduced activity level under those guidelines. We are deeply grateful for the gracious way that the Lunar Prospector staff and the DSN have managed this extra burden on their time. The spacecraft is at a distance > 6.6 Billion miles (>71 AU's) and is the farthest out in the opposite direction to which the Sun moves. Voyager 1 passed Pioneer 10 in mileage out of the Solar System on 17 February 1998 but is travelling in the opposite direction.
The low-power Geiger-Tube-Telescope (GTT) instrument still yields valuable scientific data. We also receive data from the Charged Particle Instrument but only for a few hours each week to conserve battery power on Pioneer 10.
Neutron monitors on Earth (e.g., at Climax and Goose Bay) recorded a marked and rapid decrease in cosmic ray intensity of about 4 % during April and early May of 1998. If Pioneer 10 is still inside the heliopause, we can expect a decrease in cosmic-ray intensity at Pioneer 10 to occur during early 1999. The approximate 9 month delay from Earth to Pioneer 10 corresponds to the distance of 71 AU covered by the solar wind assuming a speed of 450 km/s. If Pioneer10 has passed outside the heliopause into interstellar space, then the decrease in cosmic intensity will not be observed at Pioneer 10.
Tracking of Pioneer is expected to continue for several more months under the current pointing arrangements, at which time another repositioning maneuver would be due. The battery reading is very low - perhaps at a minimum. Pioneer 10 persists longer than ever conceived or expected. Stay tuned!
Pioneer 10 will continue into interstellar space, heading generally for the red star Aldebaran, which forms the eye of Taurus (The Bull). Aldebaran is about 68 light years away and it will take Pioneer over 2 million years to reach it.
SUNWARD PULL!?(See the December 1998 issue of Scientific American)
A team of planetary scientists and physicists led by John Anderson (Pioneer 10 Principal Investigator for Celestial Mechanics) has identified a tiny unexplained acceleration towards the sun in the motion of the Pioneer 10, Pioneer 11 and Ulysses spacecraft. The anomalous acceleration - about 10 billion times smaller than the acceleration we feel from Earth's gravitational pull - was identified after detailed analyses of radio data from the spacecraft. A variety of possible causes were considered including: perturbations from the gravitational attraction of planets and smaller bodies in the solar system; radiation pressure, the tiny transfer of momentum when photons impact the spacecraft; general relativity; interactions between the solar wind and the spacecraft; possible corruption to the radio Doppler data; wobbles and other changes in Earth's rotation; outgassing or thermal radiation from the spacecraft; and the possible influence of non-ordinary or dark matter. After exhausting the list of explanations deemed most plausible, the researchers examined possible modification to the force of gravity as explained by Newton's law with the sun being the dominant gravitational force. "Clearly, more analysis, observation, and theoretical work are called for," the researchers concluded. The scientists expect the explanation when found will involve conventional physics.
Dr. Larry Lasher
Pioneer Project Manager
NASA Ames Research Center
NASA Ames Research Center, Mountain View, CA
March 27, 1997
Pioneer 10's last support is being conducted from NASA's Deep Space Station 63, located near Madrid, Spain. The final downlink of the signal begins at 5:25 a.m. PST March 31. Signal acquisition will end at 11:45 a.m PST March 31.
The Geiger Tube Telescope Instrument data from this support will be the last data samples processed for the Principal Investigator Dr. James Van Allen under the Pioneer 10 project. The Pioneer 10 signal, transmitted 6.2 billion miles from Earth, is equal to 2.5 billionth of a trillionth of a watt. The signal strength measurement of Pioneer 10 on the computer screen will visibly drop at 11:45 a.m. and the lights will be symbolically turned off in the control room.
Future support of the Pioneer 10 spacecraft will be on a non-interference basis to other NASA projects and will be used for the purpose of training Lunar Prospector controllers in Deep Space Network coordination of tracking activities.
Intermittant tracking for Pioneers 6, 7 and 8, in Earth-like solar orbits, will also cease on Mar. 31. The briefing will include a brief summary of the entire Pioneer program, United State's longest running spacecraft program, which began in 1958. Speakers are: Dr. Larry Lasher, Pioneer Project Manager, "Overview of Pioneer Program"; Charles Hall, Pioneer Project Manager (1969-80) "Interplanetary, Planetary, Outer Solar System Pioneer Missions"; Dr. David Morrison, Director of Space, NASA Ames, "Pioneer's Relevance to the Future of Space Exploration"; Scott Hubbard, Assoc. Director of Space, Lunar Prospector Mission Manager, NASA Ames, "Transition to Lunar Prospector".
Ames Research Center, Mountain View, CA
Feb. 27, 1997
Those wishing to participate will be able to attend the conference by Internet hookup. Through the medium of their computers, they will be able to hear eight talks about planets and astronomy by experts, including Dr. James Van Allen, Pioneer 10 Principal Investigator for whom Earth's Van Allen Belt is named. Remote conference attendees also will be able to see graphics on their computer screens illustrating the audio presentations.
The day-long educational conference, co-sponsored by NASA's Ames Research Center, Mountain View, CA, and The Planetary Society, will take place at NASA Headquarters, Washington, DC. "It's going to be attended by as many as 200 DC-area educators and Planetary Society members," said Dr. Larry Lasher, NASA event organizer and Pioneer project manager. The conference is scheduled to begin at 9:30 a.m. and conclude at 4:30 p.m. EST.
"People from all over the world have been following Pioneer 10 developments for decades. This virtual conference will allow them to learn more about the mission," said Andrea McCurdy, one of the NASA Ames K-12 Internet Initiative team members. McCurdy was instrumental in helping to establish the silver anniversary Pioneer web stite.
Internet participants will not only be able to view the conference proceedings, they will also be able to use the world wide web to send typed questions to experts and to receive audio answers.
"We are using an additional technology that will allow the user to receive audio, to send questions via their keyboards and to receive text answers. With this technology, they can also view computer pictures that will automatically change during the talks," McCurdy said.
More than 150 Internet attendees from Australia, Belgium, Canada, Denmark, Italy, Japan, Kenya, the Netherlands, the United Kingdom and the United States have registered to attend the conference. More people are expected to enroll before the virtual conference begins. They will be to participate in advance in practice sessions to learn how to use audio, "chat" and other web tools, according to McCurdy. However, Internet attendees are not required to register in advance, she said.
"We can accommodate up to 200 people during the virtual conference. If the system becomes congested, we have the capability to double that number," she said. Potentially, thousands of people could drop in to the virtual conference and not cause any problems, according to McCurdy.
If attendees miss the live sessions, they will be able to look at a complete Internet archive of the Pioneer event at a later time. "All the audio files, text, transcriptions and graphics will be there. We don't plan to remove them from the Internet," McCurdy said.
Presenters will include Pioneer 10 project manager Dr. Larry Lasher; former Pioneer 10 project managers Richard Fimmel, speaking on "Pioneer Firsts" and Fred Wirth talking on "Operating and Controlling Pioneer;" Planetary Society executive director Dr. Louis Friedman, presenting "Pioneer: Segue to the Future;" and the Jet Propulsion Laboratory's Pioneer 10 principal investigator (PI) Ed Smith talking about "Outer Planets and Magnetospheres."
Other Pioneer 10 PIs scheduled to speak will include Dr. John Simpson from the University of Chicago on "The Heliosphere: Our Laboratory in Space," and the University of Maryland's Dr. Frank McDonald presenting "The Heliosphere: The Barrier to Interstellar Space." In addition, Ames Research Center Director Dr. Henry McDonald will offer remarks and Director of the Space Directorate at Ames, Dr. David Morrison, will speak on "Future Exploration of Outer Space." Dr. Wesley Huntress, NASA Associate Administrator, Space Sciences, will also address participants.
Pioneer 10 was the first artifact to leave the solar system on June 13, 1983, when the spacecraft passed beyond the system's farthest known planet. The spacecraft is now approaching a point 7 billion miles from the Sun. Sunday, March 2, is the official 25th anniversary of the beginning of Pioneer 10's flight.
NASA Headquarters, Washington, DC
Ames Research Center, Mountain View, CA
Feb. 27, 1997
"Pioneer 10 exemplifies the American pioneering spirit of exploration far beyond the frontier," said Dr. Wesley T. Huntress, Jr., Associate Administrator for Space Science at NASA Headquarters, Washington, DC. "Not only has it made many major scientific discoveries in the far reaches of space, we're proud that it has managed to stay alive almost ten times longer than the original mission called for, a tribute to the designers and builders at TRW, and the operators at NASA's Ames Research Center.
"NASA operated the Pioneer 10 mission as long as it had enough power to return science data about the conditions in space as far from Earth as possible. We will end the science mission at the end of March because the power has finally become too weak to do significant science," Huntress said.
Launched from Cape Kennedy on March 2, 1972, aboard an Atlas Centaur rocket for what had been planned as a two-year mission to Jupiter, Pioneer 10 is now so far away that its radio signal, traveling at the speed of light (186,000 miles per second), takes nine hours and ten minutes to reach the Earth. Currently twice as far from the Sun as Pluto, Pioneer is returning data about the farthest reaches of the Sun's atmosphere.
Now 6.2 billion miles from Earth, Pioneer 10, built by TRW Space and Electronics Group, Redondo Beach, CA, was the first spacecraft to travel through the asteroid belt and explore the outer solar system, the first spacecraft to visit Jupiter, the first to use a planet's gravity to change its course and to reach solar-system-escape velocity, and the first spacecraft to pass beyond the known planets.
Now traveling at 28,000 miles per hour, Pioneer 10 is recording the intensity of galactic cosmic rays in the outer heliosphere (the region of solar wind influence) and searching for the heliopause, the true outer boundary of the solar system where the flow of hot gas from the Sun (the solar wind) bumps into the interstellar medium. The spacecraft is heading in the direction of the long "tail" of the teardrop-shaped heliosphere.
Many scientists rank the first crossing of the asteroid belt between Mars and Jupiter as one of Pioneer 10's major achievements. Before the crossing, no one knew how many rocks, as well as grains of sand, speeding through space at thousands of miles per hour would impact and possibly disable the spacecraft. Pioneer 10 made the crossing nearly unscathed, thus opening the way for other spacecraft to explore beyond Mars, including its sister Pioneer 11, the twin Voyager spacecraft, the Galileo mission to Jupiter and, later this year, the Cassini mission to Saturn.
The spacecraft also survived Jupiter's intense radiation belts when it flew safely by the giant planet in December 1973. Providing the best information of the planet obtained to that date, Pioneer 10's instruments studied ultraviolet and infrared radiation and charged particles, and provided the first "close-ups" of Jupiter and its moons. It also was the first to measure the planet's giant radiation belts, magnetic field and magnetosphere, as well as its atmosphere and interior. The spacecraft measured the exact masses of Jupiter and its four planet-sized moons, Io, Europa, Ganymede and Callisto.
After its Jupiter flyby, the spacecraft continued its mission of exploration for over two decades, and in 1983 became the first spacecraft to travel beyond the outermost planets, Neptune and Pluto. Pioneer 10 will have its first "near-star-encounter" in about 30,000 years when it will pass within approximately three light years of the red dwarf star Ross 248 in the constellation Taurus. In the next million years, Pioneer 10 will pass ten stars at distances ranging from three to nine light years, and will probably still be traveling through the Milky Way galaxy when the Sun becomes a red giant and destroys the Earth five billion years from now.
Pioneer carries a message for any intelligent life forms that it might encounter on its trek across the galaxy. A gold-anodized aluminum plaque designed by Dr. Frank Drake and the late Dr. Carl Sagan is bolted to the spacecraft. The plaque's engraving depicts a man and a woman, a map of Earth's solar system, and other symbols which may help intelligent beings interpret the message and understand something about the spacecraft's creators, and where they lived.
The 570-lb. spacecraft carries 11 instruments that have been used to measure magnetic fields, solar wind, high energy cosmic rays, cosmic and asteroidal dust, and Jupiter's ultraviolet and infrared radiation. Pioneer 10 obtains power from four radioisotope thermoelectric generators that originally supplied 160 watts, but are now two-thirds degraded. The spacecraft is spin-stabilized and has a nine-foot dish antenna. Pioneer's 8-watt signal, equal to the power of a night light, now reaches the 70-meter antennae and sensitive receivers at NASA's Deep Space Network with the strength of .3 billionths of a trillionth of a watt. More information on Pioneer 10 (including an image of the plaque) is available via the Internet at URL:
http://pyroeis.arc.nasa.gov/pioneer/PN10&11.html
The 25th Anniversary of Pioneer 10's launch will be celebrated March 3 in Washington, DC. The events include a day-long Educator's Conference at NASA Headquarters, co-sponsored by the Ames Research Center and The Planetary Society, which will be linked worldwide by the Internet, with a virtual conference featuring RealAudio, WebChat, and E-mail questions for those not attending onsite. Visit the Pioneer 10 web site.
The Pioneer 10 mission is managed by the Ames Research Center, Mountain View, CA, for the Office of Space Science, NASA Headquarters, Washington, DC.
SKY & TELESCOPE NEWS BULLETIN
FEBRUARY 28, 1997
Incredibly, Pioneer 10 maintains contact with Earth using just an 8- watt transmitter, but the electricity supplied by the plutonium-fueled generators on board is weakening. Even so, the spacecraft is still returning data on the intensity of galactic cosmic rays, using the instrument developed by space pioneer James Van Allen. Some 30,000 years from now the spacecraft will pass in the general vicinity of Ross 248, a 15th-magnitude star in the constellation Taurus.
REDONDO BEACH, Calif. - 1972 was a good year for launching careers: Hewlett Packard introduced the world's first hand-held scientific calculator; Jimmy Connors and Chris Evert became professional tennis players; and NASA launched the TRW-built Pioneer 10 spacecraft.
The venerable HP-35 electronic calculator, priced at $395 per copy, replaced the faithful slide rule, transforming complete industries almost overnight. The Connors/Evert duo brought celebrity and a new, innovative style of play to center court, helping to transform professional tennis into one of the world's richest-paying spectator sports.
And Pioneer 10, the first man-made object to leave the solar system, proved that travel to the outer solar system was possible, paving the way for a generation of successful NASA interplanetary space missions including Pioneer 11, Voyagers 1 and 2 and Galileo.
On Sunday, March 2, Pioneer 10 will celebrate its 25th birthday in space. Still operating, it is now more than 6.1 billion miles from the Earth, making it NASA's most distant spacecraft. Like Connors, Evert and the hand-held calculator, it owes its success to innovation -- and rugged, well-designed packaging.
And like those other pioneers, its career has produced new ways of thinking about the world that have fundamentally altered the course of history.
"Pioneer 10 is a wonderful example of the engineering excellence and superior mission performance that TRW has delivered to its space customers since 1958," said Tim Hannemann, executive vice president and general manager of TRW Space & Electronics Group.
"The spacecraft's innovative, low-risk design allowed it to remain in service 15 times longer than its intended mission life, giving NASA and scientists worldwide an unprecedented look at Jupiter and the outer reaches of our solar system."
To succeed in the job, Pioneer 10 would have to overcome two significant hurdles: an asteroid belt of rock and space debris between the orbits of Mars and Jupiter considered to be a barrier to interplanetary space travel; and several belts of radiation near Jupiter feared strong enough to render the spacecraft inoperable.
Just in case their "new hire" didn't reach Jupiter safely on the first try, NASA asked TRW to build an identical back-up spacecraft, Pioneer 11.
TRW's Ed Wheeler, a member of Pioneer 10's original design team, recalled, "Since no other spacecraft had ever made this trip, we knew we had to make it extremely reliable and ensure, as best we could, that it could survive a harsh radiation environment." Wheeler and his colleagues completed design, production and integration of the 570-pound spacecraft in about two-and-a-half years.
Pioneer 10 was launched on March 2, 1972 from Cape Kennedy aboard an Atlas/Centaur launch vehicle. A year later, it began its trek across the uncharted asteroid belt. To the amazement of NASA scientists, it emerged seven months later, virtually unscathed.
In December 1973, Pioneer 10 became the first spacecraft to fly by Jupiter, snapping the world's first close-up photos of the giant planet. That's when TRW's foresight in designing a simple, rugged spacecraft began to pay off.
"We designed many of Pioneer 10's components with proven, radiation-hardened medium-scale integrated circuits, instead of the newer, but riskier very large-scale integrated circuits available in the late '60s," explained Wheeler.
"When the spacecraft flew by Jupiter, it was exposed to radiation levels 100,000 times stronger than a lethal dose for a human being. The glass on its star tracker, a navigation instrument, turned black, but the spacecraft suffered only minor damage."
Before it left Jupiter's neighborhood, Pioneer gathered the first definitive set of data about the solar system's largest planet. Among its findings:
Fortunately, Pioneer 10's design team had planned for this situation by equipping it with a self-contained nuclear power system. Its four radioactive isotope thermoelectric generators (RTGs), which produce energy from the radioactive decay of plutonium, each provided 40 watts of power at 4 volts.
As Pioneer 10 passed by Jupiter, its career received the first "interplanetary jump start." A TRW engineer calculated that if the spacecraft were targeted for a "near miss" with Jupiter (fly within 80,000 miles), the immense gravitational attraction of the planet would boost the satellite's velocity to more than 82,000 miles per hour, the escape velocity of the solar system.
The successful "slingshot" maneuver around Jupiter, which allowed NASA to retarget Pioneer 10 for a spot outside the solar system, is now standard operating practice for interplanetary space travel.
On June 13, 1983, more than 11 years after launch, Pioneer 10 became the first man-made object to leave the solar system. With seven of its instruments still sending back data about interstellar space, though, its career was far from over.
By the time Pioneer 10 crossed Pluto's orbit for the last time, however, the Sun had become too distant a star to provide useful navigational clues.
Today, Pioneer 10 orients itself with the aid of a strong beacon-like signal sent out about twice a year from NASA's Deep Space Network. Using the beacon as a reference point, Pioneer 10's programmable processor - one of the first ever flown in space - commands the spacecraft's attitude control thrusters to turn the spacecraft toward the Earth.
The single most important factor behind the success of these on-orbit "steering" maneuvers - NASA successfully performed the latest one just last month - is Pioneer 10's hydrazine-based propulsion system. In 25 years, the spacecraft's four tiny one-pound attitude control thrusters - the "oars" that turn the spacecraft during the pointing maneuvers - have never missed a day of work.
TRW credits this performance, in part, to the tiny electric heaters that insulate the thrusters and their liquid propellant lines against the extreme cold of space. Design variations on these units have been the standard for TRW spacecraft attitude control systems since the early '70s.
As the world's ambassador to the universe, Pioneer 10 also carries with it the world's first "interstellar postcard," a 6-inch by 9-inch anodized gold plaque bolted to the spacecraft's main frame.
Designed by the late Dr. Carl Sagan, the plaque is inscribed with symbols, binary numbers and drawings meant to communicate the nature and the location in the universe of the civilization that launched the Pioneer 10 spacecraft.
Six of its original 11 instruments are still functional, but its power generators are running out of fuel. The energy produced by the satellite's RTGs is now barely sufficient to operate just two instruments: a Geiger tube telescope and an ultraviolet photometer.
Still, Pioneer 10's durable 8-watt transmitter, the power equivalent of a home night light, continues to transmit its findings about the outer reaches of the heliosphere, that portion of space affected by the solar wind.
By the time the signals reach the football-field-sized antennas of NASA's Deep Space Network - a one-way trip takes more than 9 hours, 10 minutes at the speed of light - they measure less than one-billionth of a trillionth of a watt (.2 x 10-21 watts).
Like the power in Pioneer 10's generators, though, the scientific value of Pioneer 10 data - and the availability of NASA resources to continue tracking the spacecraft - is rapidly dwindling. On March 31, 1997, the funding needed to continue mission operations will cease. But Pioneer 10's faint signal will continue to serve the cause of space exploration.
Its real-time tracks will still be used to train spacecraft controllers and data archivists at NASA's Deep Space Network and other NASA tracking facilities as they prepare for upcoming NASA Discovery missions such as Lunar Prospector.
As it sails into eternity, Pioneer 10 will be remembered not only as "NASA's trailblazer to the stars," but also, in Wheeler's words, as an "innovative little spacecraft that found a cheap, simple way to perform an extraordinary mission."
And who knows, maybe one day someone in a distant universe will discover Pioneer 10's interstellar post card, figure it out -- and send it back.
The TRW-built Pioneer 11 spacecraft, twin sister to Pioneer 10, was launched on April 5, 1973 following Pioneer 10's successful trek across the feared Mars-Jupiter asteroid belt. It followed Pioneer 10's same trajectory to Jupiter, then headed for Saturn, where it made the first direct observations of the ringed planet in 1979.
After continuing its studies of energetic particles, it too exited the solar system. Pioneer 11's mission ended in September 1995. Its electrical power source exhausted, the spacecraft could no longer operate any of its scientific instruments, nor point its antenna toward Earth. The spacecraft is now headed toward the constellation of Aquila, northwest of the constellation of Sagittarius. It may pass near one of the stars in the constellation in about 4 million years.