Author Archive
The U.S. Air Force’s robotic space drone, the X-37B, has flown more than 600 days circuiting the Earth.
This craft is labeled Orbital Test Vehicle (OTV-6), also called USSF-7 for the U.S. Space Force, and was launched on May 17, 2020 by an Atlas-V 501 booster.
As for the vehicle’s primary agenda that remains classified, although some of its onboard experiments were identified pre-launch.
Known payloads
One experiment onboard the space plane is from the U.S. Naval Research Laboratory (NRL), an investigation into transforming solar power into radio frequency microwave energy. The experiment itself is called the Photovoltaic Radio-frequency Antenna Module, PRAM for short.
In addition, the X-37B also deployed the FalconSat-8, a small satellite developed by the U.S. Air Force Academy and sponsored by the Air Force Research Laboratory.

Naval Research Laboratory (NRL) has pioneered “sandwich” modules that are used in space solar power experiments.
Credit: NRL/Jamie Hartman
Also onboard are two NASA experiments, one to study the effects of the space environment on a materials sample plate and a payload of seeds.
OTV-6 is the first to use a service module to host experiments. The service module is an attachment to the aft of the vehicle that allows additional experimental payload capability to be carried to orbit.
Track record
There’s no official word on when the military space plane mission will return to Earth, but the craft might be headed for a record-setting duration in orbit, eclipsing 780 days in space.

X-37B breaks record, lands after 780 days in orbit
The Air Force’s X-37B Orbital Test Vehicle Mission 5 successfully landed at NASA’s Kennedy Space Center Shuttle Landing Facility Oct. 27, 2019.
Credit: U.S. Air Force
Originally designed for missions of 270 days, the X-37B has set endurance records during each of its five previous flights.
Earlier flights in the X-37B program are:
OTV-1: launched on April 22, 2010 and landed on December 3, 2010, chalking up over 224 days on orbit.
OTV-2: launched on March 5, 2011 and landed on June 16, 2012, spending over 468 days on orbit.
OTV-3: lofted on December 11, 2012 and landed on October 17, 2014, spending over 674 days on-orbit.
OTV-4: launched on May 20, 2015 and landed on May 7, 2015, spending nearly 718 days on-orbit.
OTV-5: placed into orbit on September 7, 2017 and landed on October 27, 2019, spending nearly 780 days on-orbit.
OTV-1, OTV-2, and OTV-3 missions landed at Vandenberg Air Force Base, California, while the OTV-4 and OTV-5 missions landed at the Kennedy Space Center, Florida.
The unpiloted mini-shuttle has a height of 9.6 feet (2.9 m), a length of 29.3 feet (8.9 m), a wingspan of 14 feet, 11 inches (4.5 meters) and weighs roughly 11,000 pounds (4,990 kg). There are two vehicles that constitute the X-37B program, designed and built by Boeing.
Reusable technologies
According to a Boeing fact sheet, “the X-37B is one of the world’s newest and most advanced re-entry spacecraft, designed to operate in low-Earth orbit, 150 to 500 miles above the Earth. The vehicle is the first since the Space Shuttle with the ability to return experiments to Earth for further inspection and analysis. This United States Air Force unmanned space vehicle explores reusable vehicle technologies that support long-term space objectives.”
According to Boeing, the autonomous vehicle features many elements that mark a first use in space, including:
- Avionics designed to automate all de-orbit and landing functions.
- Flight controls and brakes using all electro-mechanical actuation; no hydraulics on board.
- Built using a lighter composite structure, rather than traditional aluminum.
- New generation of high-temperature wing leading-edge tiles and toughened uni-piece fibrous refractory oxidation-resistant ceramic (TUFROC) tiles.
- Advanced conformal reusable insulation (CRI) blankets.
- Toughened uni-piece fibrous insulation (TUFI) impregnated silica tiles.
“The X-37B has a lifting body-style and landing profile that is similar to the Space Shuttle, but the vehicle is one-fourth the size. The X-37B design combines the best of aircraft and spacecraft into an affordable system that is easy to operate and maintain,” states Boeing.
Space test platform
The X-37B program is flown under the wing of a U.S. Space Force unit called Delta 9, established and activated July 24, 2020.
“Delta 9 Detachment 1 oversees operations of the X-37B Orbital Test Vehicle, an experimental program designed to demonstrate technologies for a reliable, reusable, unmanned space test platform for the U.S. Space Force,” according to a fact sheet issued by Schriever Air Force Base in Colorado.
“The mission of Delta 9 is to prepare, present, and project assigned and attached forces for the purpose of conducting protect and defend operations and providing national decision authorities with response options to deter and, when necessary, defeat orbital threats,” the fact sheet explains. “Additionally, Delta 9 supports Space Domain Awareness by conducting space-based battlespace characterization operations and also conducts on-orbit experimentation and technology demonstrations for the U.S. Space Force.”
Go to this new video of OTV-6 flying overhead on January 11, 2022 by satellite tracker, Kevin Fetter, at:
NASA’s Curiosity Mars rover at Gale Crater is now performing Sol 3351 tasks.
Recent imagery shows the robot’s surroundings:

Curiosity Mast Camera Right imagery taken on Sol 3350, January 8, 2022
Credit: NASA/JPL-Caltech/MSSS

Curiosity Mast Camera Left image taken on Sol 3349, January 7, 2022.
Credit: NASA/JPL-Caltech/MSSS

Curiosity Mast Camera Left image taken on Sol 3349, January 7, 2022.
Credit: NASA/JPL-Caltech/MSSS

Curiosity Mast Camera Left image taken on Sol 3349, January 7, 2022.
Credit: NASA/JPL-Caltech/MSSS

Curiosity Mast Camera Left image taken on Sol 3349, January 7, 2022.
Credit: NASA/JPL-Caltech/MSSS

Curiosity Mast Camera Left image taken on Sol 3349, January 7, 2022.
Credit: NASA/JPL-Caltech/MSSS

Landing leg of Chang’e-5 lander.
Credit: CNSA/CLEP
China’s Chang’e-5 lunar lander has provided the first on-location detection of water on the Moon.
The finding was published in Science Advances on January 7, written by a joint research team led by Lin Yangting and Lin Honglei from the Institute of Geology and Geophysics of the Chinese Academy of Sciences (IGGCAS).
Data acquired by the Chang’e-5 observed water signals in reflectance spectral data from the lunar surface.

China’s Chang’e-5 robotic sample return mission.
Credit: CNSA/CLEP
Spectral reflectance
China’s Chang’e-5 spacecraft landed in the Northern Oceanus Procellarum basin on the Moon on December 1, 2020 and successfully returned to Earth 1.731-kilograms of lunar collectibles on December 17, 2020.
The spacecraft landed on one of the youngest mare basalts, located at a mid-high latitude on the Moon.

Chang’e-5 descent stage seen just before sunset on Februray 7, 2021.
Credit: NASA/GSFC/Arizona State University
Before sampling and returning the lunar specimens to Earth, the lunar mineralogical spectrometer onboard the lunar lander performed spectral reflectance measurements of the regolith and of a rock, thereby providing the extraordinary opportunity to detect lunar surface water.
Parts per million (ppm)
A quantitative spectral analysis indicates that the lunar soil at the landing site contains less than 120 ppm of water – mostly attributed to solar wind implantation. This is consistent with the preliminary analysis of the returned Chang’e-5 samples.

Context images and water content at the Chang’e-5 landing site
Credit: Lin Honglei
In contrast, however a light and vesicular rock — a light-colored and surface-pitted rock (named as CE5-Rock) — that was also analyzed revealed an estimated roughly 180 ppm of water, thus suggesting an additional water source from the lunar interior.
According to the research, “the results of compositional and orbital remote sensing analyses show that the rock may have been excavated from an older basaltic unit and ejected to the landing site of Chang’e-5. Therefore, the lower water content of the soil, as compared to the higher water content of the rock fragment, suggests that degassing of the mantle reservoir beneath the Chang’e-5 landing site took place.”

Chang’e-5 return capsule holding lunar specimens.
Credit: National Astronomical Observatories, CAS
Researchers from the National Space Science Center of CAS, the University of Hawaiʻi at Mānoa, the Shanghai Institute of Technical Physics of CAS and Nanjing University were also involved in the study.
To view the research paper – “In situ detection of water on the Moon by the Chang’E-5 lander” – go to:

Curiosity Left B Navigation Camera photo taken on Sol 3348, January 6, 2022.
Credit: NASA/JPL-Caltech
NASA’s Curiosity Mars rover at Gale Crater is now performing Sol 3349 duties.
Lucy Thompson, a planetary geologist at University of New Brunswick; Fredericton, New Brunswick, Canada, reports another successful drive on Mars by the robot.

Curiosity Chemistry & Camera RMI taken on Sol 3349, January 7, 2022.
Credit: NASA/JPL-Caltech/LANL
The drive resulted in a dusty bedrock workspace with nodules and small raised ridges in front of the rover, Thompson adds. “Curiosity also has a view towards larger scale, dark, resistant ridges that we have noticed within the more subdued and lighter colored, more typical bedrock in this area.”

Curiosity Mast Camera Left image acquired on Sol 3347, January 5, 2022.
Credit: NASA/JPL-Caltech/MSSS

Curiosity Mast Camera Left image acquired on Sol 3347, January 5, 2022.
Credit: NASA/JPL-Caltech/MSSS
Small, raised ridges
Thompson notes that the science team decided to investigate the chemistry and texture of one of the small, raised ridges in the workspace (“El Fosso”) with the Alpha Particle X-Ray Spectrometer (APXS) and the Mars Hand Lens Imager (MAHLI).

Collection of Mast Camera Right and Left imagery taken on Sol 3347, January 5, 2022.
Credit: NASA/JPL-Caltech/MSSS
“Is the ridge there because of the presence of a harder, more resistant mineral that might have formed as fluid flowed through the rock? Determining the chemistry of the feature could help to figure out why the ridge is there,” Thompson explains.
To complement this observation, the bedrock target “Kamarkawarai” will be analyzed with the Chemistry and Camera (ChemCam) Laser Induced Breakdown Spectroscopy (LIBS) and imaged with the rover’s Mastcam.
Movement of sand
Looking further afield, Curiosity is slated to image one of the larger scale, dark, resistant ridges with a ChemCam Remote Micro-Imager (RMI) mosaic.
A planned drive is expected to take Curiosity closer to one of these ridges, which Mars researchers hope to investigate in future plans.
Mastcam is scheduled to document an area that may have been the site of recent movement of sand around a block (“The Pit”), as well as an area of a butte that may contain cross bedding (“Maringma”).

Curiosity Mast Camera Right image acquired on Sol 3347, January 5, 2022.
Credit: NASA/JPL-Caltech/MSSS
Increase in dust
“Our plan was also full of atmospheric and environmental observations, particularly as we are expecting an increase in dust within the atmosphere as a regional storm passes by. We planned Mastcam basic tau, crater rim extinction and sky survey observations as well as a Navcam line of sight observation and suprahorizon movie,” Thompson reports.

Curiosity Mast Camera Right image acquired on Sol 3347, January 5, 2022.
Credit: NASA/JPL-Caltech/MSSS
After the rover’s drive, the plan calls for acquiring a DAN active measurement and a MARDI observation to document the terrain beneath the rover. Standard Dynamic Albedo of Neutrons (DAN), Rover Environmental Monitoring Station (REMS) and Radiation Assessment Detector (RAD) activities round out the plan.
“Today was one of those planning days when everything went smoothly. It is not always easy to place the APXS and MAHLI instruments (situated on the end of the robotic arm) on the rocks that we want to investigate,” Thompson points out. “We have to ensure the safety of our instruments and the rover,” and it was relatively easy to place APXS and MAHLI on a target of interest.

The targeted landing zone for Ingenuity’s Flight 19 can be seen in this Return-To-Earth (RTE) camera image from Flight 9. The targeted landing spot is in the center of the image, just below the rover tracks.
Credit: NASA/JPL-Caltech
NASA’s Ingenuity rotorcraft is slated to take place no earlier than today, Friday, January 7.
Martin Cacan, Ingenuity Pilot at NASA’s Jet Propulsion Laboratory, reports the scout vehicle will fly out of the South Séítah basin, across the dividing ridge, and up onto the main plateau.
The precise landing target for Flight 19 is near the landing site of Flight 8.
Fault protection parameters
“While short, the flight has a challenging start due to featureless sandy terrain that the helicopter currently sits on,” Cacan explains. “Initially chosen for the lack of rocks to land safely, the area is actually so devoid of rock that warnings were reported during Flight 18 landing due to insufficient features to track in the vision navigation. As a result, fault protection parameters will be updated to mitigate the risk of a premature landing mid-ascent.”
This 19th flight is set to last about 100 seconds at a groundspeed of 2.2 mph (1 meter per second) and altitude of 33 feet (10 meters) while taking 9 new, high-resolution Return-To-Earth (RTE) images.
“The final act of the flight is to turn nearly 180 degrees to flip the RTE camera to a forward-facing orientation for future flights toward the river delta,” Cacan adds.
China has tested a key step in completing its space station by the end of this year.
A mechanical arm of China’s Tianhe core module shifted the Tianzhou-2 cargo spacecraft, then re-docked and locked the hardware to the core cabin.
The China Manned Space Agency (CMSA) said early Thursday morning that the experiment will be applied in the subsequent assembly and construction of the space station in orbit.
The process took about 47 minutes and was the first time that China has used the space station robotic arm to operate a large spacecraft in orbit for a “transposition” test. It is the first such maneuver of the robotic arm that measures 33-feet (10-meters) long and that’s able to lift objects weighing up to 20 tons.
Breakthrough technology
After being unlocked and separated from the Tianhe core module, the Tianzhou-2 cargo spacecraft was dragged by the mechanical arm, taking the sphere center of the core module’s node cabin as the center of the circle for plane transposition.
Then, a reverse operation was performed until the cargo spacecraft re-docked and locked with the core cabin, reports China Central Television (CCTV). The robotic arm is installed on the Tianhe core module.
The precursor evaluation will be utilized when China launches two lab modules – the Wentian and Mengtian lab modules — to the station construction site later this year.
“If transposition fails or is unavailable, the whole scale will probably be limited. This is a technology in which we must make breakthrough in the course of building the entire space station,” Shi Jixin, deputy chief designer of the space station at the Fifth Academy under the China Aerospace Science and Technology Corporation (CASC) told CCTV. “The entire space station can be built on schedule only when we make the technological breakthrough,” Shi said.
First, the robotic arm crawled to its berth port near the node cabin of the core module two days ahead of schedule in preparation for the transposition test. After that, the Tianzhou-2 cargo spacecraft was grabbed by the robotic arm.
“I use a robotic arm to push the cargo spacecraft to unlock, and then reverse it and make it return to re-dock, and finally complete the lock,” said Shi.
Trial testing
Shi said that during the transposition test, one end of the robotic arm was connected to the core module and the other end to the Tianzhou-2 cargo spacecraft, which is unstable and might cause damage to the robotic arm just like a pole carrying two elephants. Therefore, technical researchers have carried out a dedicated design for the transposition test.
“First, I set it upright, and then reverse it at a 90-degree angle, so that the windward side is the smallest and the operation in orbit has a minimal aerodynamic disturbance. It stands up like a pendulum, and the module is actually gradient-stable, which means that no matter which way I flip it, it will stay on its vertical axis,” Shi told CCTV.
Xu Xiaoping, deputy chief designer of the cargo spacecraft system of the Fifth Academy of China Aerospace Science and Technology Corporation (CASC) added: “Before carrying out the test in space, we had conducted trial tests on the ground to simulate the space test.”
Xu noted that he mechanical arm of the space station has assisted astronauts in four extravehicular activities. The test conducted Thursday was a test of the mechanical arm’s capability of transposition of the cargo spacecraft.
Large load
“The mechanical arm has never carried such a large load. In the past, an astronaut out of the spacecraft plus the space suit carried by a mechanical arm usually weighed about 300 kilograms. This time the load weighs nearly nine tons. Such a heavy load is also a test to the mechanical arm,” said Shi.
Shi said that the space station system is in good condition, and the maneuver will also prepare Tianhe to dock the Wentian and Mengtian lab modules.
“It is a joint validation of multiple systems,” Shi explained. “First, in the process of docking, the speed of the mechanical arm in fact is not high enough. Thus, the GNC [guidance, navigation and control] subsystem is needed to accelerate the speed, so that docking could be successfully completed. After docking, the cargo spacecraft needs to be re-docked and captured, and then the mechanical arm will withdraw after the locking [is] completed. Therefore, multiple systems involved in this process will be verified in the test.”
Two modes
“Astronauts control the cargo spacecraft in the core module, and carry out manual remote operation to conduct withdrawal and docking tests. At present, there are two modes of cargo spaceship rendezvous and docking. The automatic rendezvous and docking would be carried out if everything goes well. If any abnormality occurs, we also have the backup means of manual remote operation. So this operation in fact is mainly for the in-orbit verification of the backup means,” said Yang Sheng, general chief of the cargo-freighter system, Fifth Academy of CASC.
After completing all missions, Tianzhou-2 will separate from the space station core module, taking away stored waste and human excrement before eventually departing from orbit and burning up upon re-entry into the Earth’s atmosphere. This is also one of the key technologies of the space station construction.
“Depending on its overall consumption and lifespan, Tianzhou-2 will choose the proper time to separate from the space station core module and burn up the waste upon re-entry into the Earth’s atmosphere. So, Tianzhou-2 is entrusted with the most and hardest tasks, and thus will stay relatively longer in orbit,” said Yang.
China sent the cargo craft Tianzhou-2 into space on May 29 last year from the southern island province of Hainan, to deliver life support supplies for astronauts, spacesuits for extra-vehicular activities, and space-science equipment among other supplies, and also to replenish Tianhe’s propellant.
On September 18 of last year, the Tianzhou-2 cargo craft separated from the rear docking port of Tianhe and docked with its front docking port.
The space station core module Tianhe was launched on April 29, 2021.
Busy year
Upon its completion at the end of this year, Tiangong (Heavenly Palace) will consist of three main components; a core module attached to two space labs, and will have a combined weight of nearly 70 tons.
China’s station is scheduled to operate for 15 years in a low-Earth orbit about 250-miles (400-kilometers) above the planet.
Six launches this year involve Shenzhou-14 and Shenzhou-15 crewed missions to the Tiangong orbiting outpost, the Tianzhou-4 and 5 robotic cargo spaceships and the two large space labs that will be docked to the facility.
China Daily reports that the first of the six to be launched will be Tianzhou-4, which will be followed by the Shenzhou-14 piloted spacecraft. Then the two space labs — Wentian (Quest for the Heavens) and Mengtian (Dreaming of the Heavens) — will be launched to complete the station. The fifth launch will be Tianzhou-5 and the final will be the Shenzhou-15 crew.
To watch newly released videos of this testing phase of China’s space station construction and life onboard the facility, go to:
An alliance of experts in space, sports and the entertainment industry are designing and developing original games exclusively for zero or micro-gravity playing fields.
The group has already singled out a number of prospective game concepts, from guiding a magnetic ball through hoops in space to space dodge ball between opposing teams, as well as racing the clock to tie an increasingly-complicated series of knots while tethered to a teammate.

Visionary artist, Pat Rawlings, sees the moon’s one sixth gravity as an excellent environment for athletic competitions that are hampered by Earth’s stifling and ever-tugging gravity.
Credit: NASA/Pat Rawlings

Watch this space! The International Space Station has prompted an array of “sporting ideas” for fun and relaxation.
Credit: NASA
For more information, go to my new Space.com story — “Let the space games begin! Ideas for off-Earth sports move to center court – Space dodge ball would be pretty fun,” at

Curiosity’s location as of Sol 3345. Distance driven 16.71 miles/26.89 kilometers.
Credit: NASA/JPL-Caltech/Univ. of Arizona
NASA’s Curiosity Mars rover at Gale Crater has just entered Sol 3348.
Curiosity has entered a new mapping quadrant, Roraima, viewing flat-topped hills and some steep slopes.
“As we head southward, we will likely be parking near some of these tall hills and cliffs in order to get close-up images,” reports Ashley Stroupe, a mission operations engineer at NASA’s Jet Propulsion Laboratory.

Curiosity Left B Navigation Camera image taken on Sol 3347, January 5, 2022.
Credit: NASA/JPL-Caltech
“Parking near such tall terrain can sometimes block our view of the orbiters if they are low in the sky, impacting the amount of data we may receive,” Stroupe adds. “We saw this kind of an effect when we parked near the tall steep cliff of Maria Gordon notch, where there was a significant reduction of data on one of our communication passes with the Trace Gas Orbiter (TGO). We will take this into account to make sure we will still get down the data we need for planning.”

Looking back, Curiosity can see all the way to the Torridon quadrant and see Mars’ “Scottish highlands” with the attached beautiful view of the Maria Gordon notch; you can also see the rim of Gale crater in the distance.
This image was taken by Left Navigation Camera on Sol 3345.
Credit: NASA/JPL-Caltech.
Touch-and-go
A recent plan had the robot perform a “touch-and-go” which includes some contact science, targeted science, and a drive.
“Our contact science target, “Verde,” is a small piece of bedrock with nodules in it, similar to many of the other rocks we have investigated recently,” Stroupe points out. “The science team will be able to compare its composition with those prior targets to continue to build up a picture of the changing geology and chemistry preserved in the region. The rover planners will then leave the arm stowed again in preparation for driving and to leave a clear view of the target for the cameras.”

Curiosity Front Hazard Avoidance Right B Camera image acquired on Sol 3347, January 5, 2022.
Credit: NASA/JPL-Caltech
The targeted science in the plan also investigates the nodules by looking at “Maurak,” another nearby target, with Curiosity’s Chemistry and Camera (ChemCam) and its Mastcam.
Distant butte
ChemCam was also to take Remote Micro-Imager (RMI) images of a distant butte named “Mirador,” both its top and its face, which has an interesting and significant textural transition, Stroupe points out.

Curiosity Left B Navigation Camera image taken on Sol 3347, January 5, 2022.
Credit: NASA/JPL-Caltech
Once ready to drive away, Curiosity will head nearly 50 feet (roughly 15 meters) southward.

Curiosity Left B Navigation Camera image taken on Sol 3347, January 5, 2022.
Credit: NASA/JPL-Caltech
“Due to some significant rocks and the uphill climb ahead of us, this is only as far as the rover planners can see. Even if that distance, the rover is going to need to wind around to skirt some more significant rocks so that we don’t add damage to the wheels,” Stroupe reports. “The drive should leave us parked where we have a better view of the road ahead, as well as leave bedrock within the rover’s workspace for the next plan.”

Curiosity Right B Navigation Camera photo taken on Sol 3347, January 5, 2022.
Credit: NASA/JPL-Caltech
Engineering maintenance
After the drive, Curiosity will do some evening environmental observations, Navcam suprahorizon and zenith movies, to look at the atmosphere. Overnight, the Sample Analysis at Mars (SAM) Instrument Suite will be doing an engineering maintenance activity to check out the optics on the tunable laser spectrometer (TLS).
On the second sol of the plan, Sol 3348, after the drive, Curiosity will do some untargeted science using AEGIS (Autonomous Exploration for Gathering Increased Science) – a software suite that permits the rover to autonomously detect and prioritize targets.
Also on tap is a long Navcam dust devil movie, Stroupe concludes.
Just-issued images show NASA’s Ingenuity Mars Helicopter observations on Sol 292, acquired on December 15, 2021.
This was the date of Ingenuity’s 18th flight. Imagery from the aerial machine was taken using its high-resolution color camera.
This camera is mounted in the helicopter’s fuselage and pointed approximately 22 degrees below the horizon.
50 Years of Solar System Exploration: Historical Perspectives has been issued by NASA Office of Communications/NASA History Division.
Divided into 12 chapters, this free volume is expertly edited by Linda Billings, a consultant to NASA’s Astrobiology Program and Planetary Defense Coordination Office in the Planetary Science Division of the Science Mission Directorate at NASA Headquarters in Washington, DC.
“What readers will find in this volume is a collection of interesting stories about money, politics, human resources, commitment, competition and cooperation, and the ‘faster, better, cheaper’ era of solar system exploration,” explains Billings.
The volume features a diverse array of scholars that address the science, technology, policy, and politics of planetary exploration. This volume offers a collection of in-depth studies of important projects, decisions, and milestones of this era.
This volume is based on a symposium — “Solar System Exploration @ 50” — held in Washington, D.C. on October 25-26, 2012. The purpose of this symposium was to consider, over the more-than-50-year history of the Space Age, what we have learned about the other bodies of the solar system and the processes by which we have gained new knowledge.
The symposium commemorated the 50th anniversary of the first successful planetary mission, Mariner 2 sent to Venus in 1962, organized by the NASA History Program Office, the Division of Space History at the National Air and Space Museum, NASA’s Science Mission Directorate, and the Jet Propulsion Laboratory.
For information on accessing this free publication, go to:
https://www.nasa.gov/connect/ebooks/50-years-of-solar-system-exploration.html
NASA webcast the entire symposium, archived here:



























