STOP THE PRESS: Pres. Clinton just approved Cassini's Launch 10/3/97
IMPORTANT: Pro-Cassini event on sunday Sept 28th in Washington DC. See
'Rallies' below for more details.
CLICK HERE for photos of the event !!! 10/1/97
ALSO 60 Minutes is having a piece about Cassini within the next 2-3
weeks.
Eight of the MOST frequently asked questions about Cassini and its RTGs
THIS SITE HAS THE MOST USEFUL COMPREHENSIVE INFORMATION ABOUT THE RTG,
THEIR NEED, SAFETY, ETC
Yahoos page on Cassini Headlines
Yahoo:Science:Space:Missions:Cassini
National Space Society has a big site on Cassini and the RTG controversy
Cassini : Mission to Saturn Nuclear Safety Issues and Answers
Explaining The Risks of The Cassini Mission
Here is Florida Todays (newspaper) article
about
the RTG's and their safety (sept 14, 97)
SEDS: Space Views - CAST your vote about RTG's
As of February 1997, there have been 20 Titan IV launches, of which 19
have been successful. The only failure was in August 1993 which was due to
a flaw in one of the solid rocket motors, which has been fixed.
I was asked this question in New York City and just found out that its
multiple protective layers of iridium capsules and high-strength graphite
blocks will prevent and fuel from being released as well as shield it from
impacting the ocean or land. Most likely it would land in the ocean since
most of Earth is covered by water. NO, SALT WATER WILL NOT CORRODE
THE RTG OR THEIR PROTECTIVE COVERS.. It wouldnt harm, danger or alter
marine life.
Three. In 1964 there was an accidental re-entry of the SNAP-9A RTG of the Navy's Transit 5BN-2 satellite which burned up in the atmosphere (which was how early RTG'swere designed). Subsequently RTG's were redesigned to contain their plutonium in reentry and launch accidents and have done so in the 1968 Nimbus B-1 mission and also the Apollo 13 mission of which it�s RTG remains in one of the deepest parts of the Pacific Ocean.
SUPPORT Cassini and inform the public about NASA and the safety with
RTG' s in Washington DC in front of the White House on Sept 28th, 1997
around 12 Noon. Members of the National Space Society are organizing this
event.
CLICK HERE for photos of the event !!! 10/1/97
RALLY INFORMATION & LOCATION We will have representatives from NASA and other organizations present.
Local Directions: Take the Metro subway to the McPherson Square Station. Use the White House / Vermont Ave. exit (corner of Vermont Ave and "I" St NW).
Go 1 block west on "I" St to 16th St NW. Turn left, go south on 16th
St to end of block (gold-topped St. John's Church on left). Cross "H" St
to Lafayette Park and look for our pro-Cassini rally.
Radioisotope Thermoelectric Generators (RTGs) are the only sensible source of power for spacecraft to the outer solar system at the present time. To date they have been used on Pioneer 10, Pioneer 11, Voyager 1, Voyager 2, Galileo, Ulysses and Cassini all of which travelled beyond 5 AU from the sun. They have also been used on the two Viking landers as well as by all the Apollo ALSEP experiment packages and numerous military Earth orbiting spacecraft. They all rely on the basic principle that if you take a piece of metal and make one end hot and one end cold then current will flow from the hot end to the cold end. This fact can be used to generate electricity.
Cassini's electrical power source - Radioisotope Thermoelectric Generators (RTGs) - have provided electrical power for some of the U.S. space program's greatest successes, including the Apollo lunar landings and the Viking Landers that searched for life on Mars. RTGs made possible NASA's celebrated Voyager explorations of Jupiter, Saturn, Uranus and Neptune, as well as the Pioneer missions to Jupiter and Saturn. RTG power sources are enabling the Galileo mission to Jupiter and the international Ulysses mission studying the Sun's polar regions.
Extensive studies conducted by NASA's Jet Propulsion Laboratory (JPL)
have shown that NASA's Cassini mission, given its science objectives,
available launch systems, travel time to its destination and Saturn's
extreme distance from the Sun, requires RTGs.
The RTGs power the spacecraft through the radioactive decay of
plutonium-238. This decay emits heat, which is converted into
electricity for the spacecraft to "see, sense, hear, and speak." This
power supplies a reliable, long-lasting source of electricity which is
insensitive to the chilling cold of space and virtually invulnerable to
high radiation fields, such as Earth's Van Allen belts and Jupiter's
magnetosphere.
An RTG consists of two parts: a source of heat and a system for
converting the heat to electricity. The heat source contains a
radioisotope, such as plutonium-238, that becomes physically hot from
its own radioactive decay. This heat is converted to electricity by a
thermoelectric converter which uses the Seebeck effect, a basic
principle of thermoelectricity discovered in 1822. An electromotive
force, or voltage, is produced from the diffusion of electrons across
the joining of two different materials (like metals or semiconductors)
that then form a circuit when the ends of the converter are at different
temperatures.
Each RTG contains 18 separate heat source modules, and each module
encases four plutonium-238 pellets. The modules are designed to survive
a range of postulated accidents: launch vehicle explosion or fire,
reentry into the atmosphere followed by land or water impact, and
post-impact situations. An outer covering of graphite provides
protection against the structural, thermal, and eroding environments of
a potential reentry. Additional graphite components provide impact
protection, while iridium cladding of the actual fuel cells provides
post-impact containment. The fuel is in the form of plutonium-238
dioxide, a ceramic material which is resistant to fracturing.
After the Challenger accident, a study considered additional shielding.
Additional shielding was not adopted, even though it would offer some
protection near the launch area, because the great complexity of such a
design significantly increased the risk of mission failure. If a failure
on orbit occurred, additional shielding would significantly increase the
consequences of a ground impact. The two close flybys of Earth had
raised questions about the possible inadvertent reentry of Galileo into
Earth's atmosphere.
Exhaustive studies were made by JPL and were independently reviewed
regarding the safety of the Venus-Earth-Earth Gravity Assist (VEEGA)
mission. The Department of Energy, as required
by law, completed a mission risk analysis, with full disclosure of those
results to State and local governments. The Interagency Nuclear Safety
Review Panel completed an independent Safety Evaluation Report and the
Office of Science and Technology Policy approved the mission. As a
result of the Project's testing and rationale for the Galileo mission,
the Court found in the Project's favor and the launch was a splendid
success. The United States has an outstanding record of safety in using
RTGs on 23 missions over the past three decades. While RTGs have never caused a
spacecraft failure on any of these missions, they have been on-board
three missions which experienced malfunctions for other reasons. In all
cases, the RTGs performed as designed.
More than 30 years have been invested in the engineering, safety
analysis and testing of RTGs. Safety features are incorporated into the
RTG's design, and extensive testing has demonstrated that they can
withstand physical conditions more severe than those expected from most
accidents.
First, the fuel is in the heat-resistant,
ceramic form of plutonium
dioxide, which reduces its chance of vaporizing in fire or reentry
environments. This ceramic-form fuel is also highly insoluble, has a low
chemical reactivity, and primarily fractures into large, non-respirable
particles and chunks. These characteristics help to mitigate the
potential health effects from accidents involving the release of this
fuel. Second, the fuel is divided among 18
small, independent modular units, each with its own heat shield and impact
shell. This design reduces the chances of fuel release in an accident because all modules would not be
equally impacted in an accident. Third,
multiple layers of protective materials, including iridium capsules and
high-strength graphite blocks, are used to protect the fuel and prevent
its accidental release. Iridium is a metal that has a very high melting
point and is strong, corrosion resistant and chemically compatible with
plutonium dioxide. These characteristics make iridium useful for
protecting and containing each fuel pellet. Graphite is used
because it is lightweight and highly heat-resistant.
Potential RTG accidents are sometimes mistakenly equated with accidents
at nuclear power plants. It is completely inaccurate to
associate an RTG accident with Chernobyl or any other past radiation accident
involving fission. RTGs do not use either a fusion or fission process and could
never explode like a nuclear bomb under any accident scenario. Neither
could an accident involving an RTG create the acute radiation sickness
similar to that associated with nuclear explosions.
NASA places the highest priority on assuring the safe use of plutonium
in space. Thorough and detailed safety analyses are conducted prior to
launching NASA spacecraft with RTGs, and many prudent steps are taken to
reduce the risks involved in NASA missions using RTGs. In addition to
NASA's internal safety requirements and reviews, missions that carry
nuclear material also undergo an extensive safety review involving
detailed verification testing and analysis. Further, an independent
safety evaluation of the Cassini mission will be performed as part of
the nuclear launch safety approval process by an Interagency Nuclear
Safety Review Panel (INSRP), which is supported by experts from
government, industry and academia.
Information about radioisotope thermoelectric generators can be
located via the DOE Reports Bibliographic Database at Select the link "Search The DOE Reports Bibliographic Database." perform a search using the keywords radioisotope thermoelectri
generators in the "Enter Search Terms Here" area. By selecting a report
link you will reach information about that report. For each report,
availability information can be found by selecting the link "Report
Ordering and Retrieval
More information from the Dept of Energy (DOE)
http://apollo.osti.gov/html/dra/dra.html