Image Credit: NASA/JPL/University of Arizona - “PSP_003086_2015: Color Image of Nili Fossae Trough, Candidate MSL Landing Site“

[Disclaimer: Richard Leis, Jr. is an Operations Specialist for HiRISE.]

The High Resolution Imaging Science Experiment (HiRISE) team today released a slew of new false color images of the surface of Mars to the public, the culmination of many months of software and automation development. Color products are now expected to be released at regular intervals, matching the previous release rate of black and white images. The images selected are of potential Mars Science Laboratory (MSL) landing sites, the upcoming rover mission planned for launch in 2009. Now that these images have been released, researchers suggesting landing sites for the mission will have new data to work with while developing their proposals.

Creating useful color products from HiRISE data has proven to be a difficult task that has involved many people. Sarah Mattson applied her continuing University of Arizona mathematics education to help develop algorithms for registering and stitching the various color products together, based on manual procedures developed by HiRISE Principal Investigator Alfred McEwen. Guy McArthur, a software developer for HiRISE, created a series of automated “pipelines” for turning calibrated image products into beautiful final color products. Eric Eliason, HiRISE Operations Center (HiROC) Manager oversaw the software development effort and participated in validation efforts. Operations Specialist Táhirih Motazedian reprocessed MSL image data through calibration, geometry, and the new color pipelines, after also conducting thorough testing of the pipelines, all while managing the HiROC systems resources that are pushed to their limits during such intense reprocessing efforts. Student Validators Alaina de Jong and Bryan Cardwell raced to validate new color products fresh out of the pipelines to ensure they were ready for today’s scheduled public release. Database Manager Rod Heyd ensured the database and procedures for releasing products were updated to handle the new color products. Finally, Website Guru Yisrael Espinoza updated the web backend and public site to include color images in an attractive and user-friendly way.

Image Credit: NASA/JPL/University of Arizona - “PSP_004052_2045: Layers Exposed in Crater Near Mawrth Vallis”

The HiRISE camera is currently in orbit around Mars on board the Mars Reconnaissance Orbiter (MRO). The camera is returning the highest resolution images of the surface ever taken from Mars orbit, with images reaching resolutions of nearly 25 centimeters per pixel. This equates to objects about one meter in size on the surface of Mars, since the human eye needs about three or four pixels to pick out an object in an image. The new color images are in enhanced and false color. Everyone knows well that the surface of Mars is a study in red, so choosing color filters that can pull out subtle differences between compositions was a priority when developing the camera. Red, near infrared, and blue-green filters down the center of the instrument’s CCD array create a false color swath in HiRISE images of about 1.2 kilometers in width. The remaining red CCDs create a black and white image 6 kilometers across.

The prospective landing sites targeted by HiRISE include materials like clays, sulfates, and other materials with high water content. MSL is expected to explore just such a location to determine the past and current role of water on Mars and whether or not the environment ever supported microbial life.

More Information

• High Resolution Imaging Science Experiment (HiRISE)
  • October 10, 2007 Color Release of MSL Observations
  • [PDF] “Information for Scientific Users of HiRISE Color Products” By Alfred McEwen and Eric Eliason, October 10, 2007
  • University of Arizona Press Release: “HiRISE Releases Color Images, Movie of Prospective Landing Sites on Mars“
  • HiBlog
• Mars Science Laboratory (MSL)
• Mars Reconnaissance Orbiter (MRO)

• Division for Planetary Sciences 40th Annual Meeting
• Ithaca, NY, USA
• October 11-15, 2008

• Division for Planetary Sciences 39th Annual Meeting
• The University of Central Florida, Orlando, FL, USA
• October 07-12, 2007

[Launch Coverage] | [Commentary]

2:10 AM PST

Too early! But despite the small hours of the morning here I am very excited for the big launch of the Dawn spacecraft planned for this morning. NASA TV playing in Windows Media Player, the oven heating for some waffles, and a groggy yet excited brain…here we go!

2:18 AM PST

Launch is still planned for 7:20 AM PST (4:20 AM EST.)

Image Credit: NASA TV screen capture - Dawn Launch Coverage as of 2:24 AM PST

2:38 AM PST

The launch vehicle is a Delta II Heavy 2925H (modified Delta II) that will lift 1,217.7 kilograms (2,684.6 pounds) of spacecraft plus fuel. Right now technicians are adding liquid oxygen in preparation for launch. Launch will be from Cape Canaveral Air Force Station in Florida, USA.

Dawn will visit the two largest objects in the Asteroid Belt: asteroid Vesta and dwarf planet Ceres. This is not just a flyby mission; Dawn will actually approach and then go into orbit around each body, meaning that after it finishes with its exploration of Vesta, it will need to restart its ion propulsion engine to leave orbit and travel on to Ceres. Dawn should reach Vesta in September 2011 and Ceres in February 2015.

Other coverage:

• Dawn Mission Home Page
• Space.com
• The Planetary Society Weblog

2:54 AM PST

Image Caption: “Hubble Images of Asteroids Help Astronomers Prepare for Spacecraft Visit”
Credits for Vesta: NASA, ESA, and L. McFadden (University of Maryland)
Credits for Ceres: : NASA, ESA, and J. Parker (Southwest Research Institute)

Notice that Ceres is large enough to be roughly spherical in shape. Vesta is just slightly too small to be a sphere. The Hubble images are some of the best images taken of these bodies to date. The journey from discovery of a light in the sky followed by improving telescope images culminating in close up images by spacecraft is the reason why I find planetary science so fascinating. Just take a moment to appreciate what we do not know about Ceres and Vesta, and what we do know, captured in these blurry images. In just a few years, pending a successful launch, we will finally gain a much clearer perspective of these mysterious planetary bodies when their surfaces are revealed in great detail by Dawn.

3:09 AM PST

Image Credit: NASA TV screen capture - Dawn Launch Coverage as of 3:07 AM PST - venting oxygen vapor

3:22 AM PST

The operations teams heard during launch coverage sound like well-oiled machines, checking off items on their checklists with great confidence and professionalism. This indicates both the complexity of the logistics involved with any launch and the experience and abilities of highly skilled humans. A highlight of NASA TV coverage is when, at particular intervals in the activity leading up to launch, various teams report in that their subsystems are “Go!” This same sequence of “Go!” pronouncements just prior to launch was a highlight for those of us on the HiRISE team who attended the launch of Mars Reconnaissance Orbiter. Sometimes we try to do the same thing at work, to liven up the place, to various degrees of success.

3:32 AM PST

A built-in hold of 20 minutes is coming up soon, followed by the restart of countdown, a 10 minute hold, and then, potentially on schedule, launch!

3:35 AM PST

T minus 15 minutes and holding for twenty minutes…

Image Credit: NASA TV screen capture - Dawn Launch Coverage as of 3:35 AM PST - Logos through vapor

3:45 AM PST

The Dawn Mission website has a wealth of images, graphics, and video, including this graphic of the spacecraft:

Image Credit: Orbital Sciences Corporation - “Dawn Spacecraft“

3:55 AM PST

The countdown clock has restarted with 15 minutes and one last built-in hold expected prior to launch. Weather is reported to be good. And dawn is breaking behind Dawn!

Image Credit: NASA TV screen capture - Dawn Launch Coverage as of 3:53 AM PST - Dawn breaks behind Dawn

4:02 AM PST

Image Credit: NASA TV screen capture - Dawn Launch Coverage as of 3:59 AM PST - Engineering

4:05 AM PST

Next built-in hold of ten minutes has begun, at T minus 4 minutes.

Image Credit: NASA TV screen capture - Dawn Launch Coverage as of 4:05 AM PST - Dawn nears launch

4:14 AM PST

The hold has been extended, possibly because of a small aircraft or boat nearby.

4:16 AM PST

According to NASA TV, a ship has been spotted in the area. The Coast Guard has contacted the ship, to make sure it moves out of the way of falling solid rocket boosters. The ship should be out of the area in a few minutes.

4:20 AM PST

New launch time: 7:34 AM EST (4:34 AM PST.)

4:27 AM PST

Image Credit: NASA TV screen capture - Dawn Launch Coverage as of 4:24 AM PST

4:30 AM PST

T minus 4 minutes to launch!

4:31 AM PST

“Go!” for launch…everything seems to be ready…

4:34:00.372 AM PST

Launch!

Image Credit: NASA TV screen capture - Dawn Launch Coverage as of 4:34 AM PST - Launch!

Image Credit: NASA TV screen capture - Dawn Launch Coverage as of 4:34 AM PST - Launch

Image Credit: NASA TV screen capture - Dawn Launch Coverage as of 4:34 AM PST - Column rising

Image Credit: NASA TV screen capture - Dawn Launch Coverage as of 4:34 AM PST

Image Credit: NASA TV screen capture - Dawn Launch Coverage as of 4:34 AM PST

Image Credit: NASA TV screen capture - Dawn Launch Coverage as of 4:35 AM PST

Image Credit: NASA TV screen capture - Dawn Launch Coverage as of 4:35 AM PST - Solid motors jettison

4:38 AM PST

All seems to be well, with events happening as expected. Dawn is racing away up through the atmosphere and away from the Earth.

4:44 AM PST

Dawn has reached Earth orbit. It will coast there for 40 minutes before the second and third stage engines sends Dawn on its way to its first stop: Vesta.

5:10 AM PST

The second stage should reignite around 5:14 AM, followed by the third stage. Separation should occur 62 minutes after launch and then the solar arrays will begin deployment. Confirmation that everything is fine and Dawn is successfully on its way may not come until one hour and 34 minutes after launch, or later. Necessary Dawn autonomous actions mean that the spacecraft will be out of contact with the Earth for much of that time.

5:25 AM PST

Telemetry has been reacquired and all is well. Second stage restart has just occurred. Operations is following along with an animation of events created from telemetry.

5:33 AM PST

The second stage fired, shut down, and separated from the upper stages successfully.

Image Credit: NASA TV screen capture - Dawn Launch Coverage as of 5:26 AM PST - Second stage firing animation

Image Credit: NASA TV screen capture - Dawn Launch Coverage as of 5:29 AM PST - Second stage separation animation

5:37 AM PST

The third stage fired and separated successfully, and Dawn is on its way!

A spacecraft health check should occur in a few hours, followed by a press conference at 1:00 PM EST (10:00 AM PST.)

Despite a 24-hour delay, preparations continue for the launch later this week of the Dawn spacecraft to explore two members of the Asteroid Belt. Dawn is now scheduled to be launched between 7:25 and 7:54 AM EDT on Thursday, September 27, 2007 after weather today interrupted the planned completion of launch vehicle fueling. The spacecraft will be launched from Space Launch Complex 17B at Cape Canaveral Air Force Station, Florida, USA using the Delta 2925H launch vehicle.

The launch period between September 26 and October 15, 2007 will allow Dawn to reach both Asteroid Vesta and recently reclassified dwarf planet Ceres as planned. Dawn has been repeatedly postponed due to a slew of other mission launches this summer and fall. These delays follow the cancellation and surprise reinstatement of the mission after earlier cost concerns were capped and technical issues were addressed.

The Dawn mission is unique because a single spacecraft will enter orbit around two separate bodies. Dawn will use an advanced ion propulsion system to enter orbit around Vesta in 2011 and then Ceres in 2014. Vesta and Ceres are the two largest objects in the Asteroid Belt and are expected to give planetary scientists a glimpse at the early history of the solar system. Scientists believe Vesta and Ceres have had very different histories despite similar beginnings.

NASA TV will broadcast the launch live.

More Information

• Dawn Mission Home Page

In 2005 Saturn’s moon Enceladus was discovered to be an active world with water ice particle geysers at its south pole. The driver of this activity on a moon so small remains a mystery. One possible explanation has been suggested by Dr. Francis Nimmo, a planetary scientist from the University of California Santa Cruz. Nimmo visited the University of Arizona Lunar and Planetary Laboratory to present his model on Thursday, September 18, 2007 for the department’s weekly Planetary Sciences Colloquium. The talk was based on his recent publication [reprint PDF] “Shear heating as the origin of the plumes and heat flux on Enceladus” in Nature.

While the old view of the outer solar system as a cold and dead region devoid of most geological activity has eroded with surprising discoveries since the 1980’s, one bias persisted until 2005: only large moons in the outer solar system could potentially be active. Below a particular diameter, moons were not believed to be able to produce sufficient internal heating to drive surface activity. With a diameter of only 252 kilometers (157 miles), Enceladus was expected to have frozen solid long ago. The discover of geysers and a thin oxygen atmosphere at Enceladus proved that this was not the case.

Enceladus’ geysers do not appear to be a global phenomena, however. They are localized to the moon’s south pole, apparently along fractures referred to as “Tiger Stripes.” Taking into consideration the moon’s size, possible internal structures, orbital eccentricity, and other characteristics Nimmo has been working to develop a model that can explain the localized nature of this activity.

An important feature of his model is reorientation theory, where a mass such as a diapir rising to the surface from the mantle can reorient a body, driving the mass’ surface expression toward the poles or equator over time. The presence of such a mass would indicate some driving force such as convection. Applied to Enceladus, this could explain why the tiger stripes have reorientated to their present location at the south pole.

While this may explain the tectonic activity at the south pole, the presence of active water ice plumes requires further explanation. If the tiger stripes are strike-slip faults like the San Andreas Fault on the Earth, then rapid enough motion back and forth along the faults could lead to uplift and shear heating. This friction leads to sublimation of water ice, the primary component of the crust of Enceladus, with some of that vapor being released with heat along the tiger stripes in the form of the spectacular plumes photographed by the Cassini spacecraft.

After developing this model, which Nimmo believes is a better explanation than other theories that have been put forward, such as a near-surface ocean or clathrate decomposition, Nimmo and his colleagues explored possible predictions. While a near-surface ocean does not provide the water vapor to geysers in his model, the model still suggests the presence of an ocean underneath a solid ice crust of at least 5 kilometers (3 miles). The model suggests that this ocean may be transitory, with significant freezing out or remelting depending on the tidal dynamics that change as Enceladus’ orbit around Saturn changes over time.

Furthermore, the orientation of the tiger stripes should change over time, and their fault motions should result in hotter or colder relative temperatures depending on how fast they are moving. In the paper, the team of researchers specify two portions of stripes they predict will have the highest relative tempatures. Some researchers believe fossil tiger stripes may be present elsewhere on Enceladus. Further observations of Enceladus may allow them to test this prediction and confirm or deny the presence of fossil tiger stripes.

Nimmo acknowledged that at present this model of Enceladus is simplistic with several questions still outstanding. Why, for example, does heating appear only at the south pole and not also at the north pole, as predicted by some models of subsurface tidal heating? What prevents the ocean, if it exists, from freezing out completely? Enceladus remains a mystery and will continue to be an important study target for planetary scientists still marveling at a frigid but incredibly active outer solar system.

More Information

• Dr. Francis Nimmo at the University of California Santa Cruz
• Cassini-Huygens Website
  • Saturn’s Moons section
  • Enceladus Information

Image caption: X PRIZE Moon exhibit and logo at WIRED NextFest

A robotic scavenger hunt to the moon is the next big space competition. The X PRIZE Foundation announced at Wired NextFest, along with representatives from Google, NASA, and one of the Apollo 11 astronauts, the Google Lunar X PRIZE. The largest incentive competition in history, US$30 million will go to the first and second privately funded teams to land a rover on the Moon.

US$20 million will be awarded to the first team who makes a soft landing on the surface of the Moon, drives a least 500 meters, and takes two sets of high definition video and images. The second team to accomplish the same tasks will be awarded US$5 million. In addition, $5 million will be awarded for bonus tasks, including finding artifacts from past mission, finding water ice at the lunar south pole, surviving one full lunar night of frigid temperatures, and driving a total of 5 kilometers instead of 500 meters.

On hand for the announcement were Dr. Peter Diamandis, X Prize chairman Robert K. Weiss, Google co-founder Larry Page, Apollo 11 astronaut Buzz Aldrin, Space Exploration Technologies (SpaceX) founder Elon Musk, and NASA Deputy Administrator Shana Dale. Video messages from Google co-founder Sergey Brin and director James Cameron were shown. All expressed their support for the latest prize.

According to Page, science has a serious marketing problem. Competitions like the Google Lunar X PRIZE can help promote science and engineering, while continuing to push progress and economic growth. Page announced during his comments a new version of Google Moon with improved resolution and panoramas captured by Apollo.

Through video and speech, the X PRIZE Foundation recapped incentive competitions to date, including the 2004 culmination of the first X Prize for a private manned suborbital launch. Since then, several new prizes have been announced, including the Archon Genomics X PRIZE, Automotive X PRIZE, and upcoming educational, life science, and energy prizes. The latest prize is being marketed as “Moon 2.0″, with previous lunar activity through the final Apollo mission in 1972 referred to as Moon 1.0. While Moon 1.0 was a competition between the superpowers, Moon 2.0 is expected to open up the moon as a resource.

X PRIZE’s Weiss listed surface silicon and water ice as important lunar resources to enable manned missions of the Moon and potentially help with resource issues on the Earth, including energy concerns. Diamandis said the Google Lunar X PRIZE will be the first commercial steps to exploiting the resources of the Moon.

SpaceX’s Musk announced they will donate profits they would normally make on space launches to lower the cost of launch of X PRIZE competitors’ entries. Other organizations like SETI will provide services to competitors for reduced or no cost.

The setting for the announcement - Wired NextFest - allowed for a somewhat elaborate stage, including a remote controlled rover that joined Diamandis at one point, a life-sized model of an astronaut and lunar rover, and a huge model of the moon unveiled for the photo-op at the end of the presentations, with Diamandis exclaiming “Let the race begin!”. In additions to participating representatives and media, there were many students, parents, and teachers in attendance for the announcement.

A video dramatization of a private team winning the Google Lunar X PRIZE in the future included depictions of access to data returned by the mission via the Internet on laptops, iPhones, and video billboards. Currently, a new website - http://www.googlelunarxprize.org/ - has been created to host educational videos, tools, and hands-on activities for students.

Image caption: X PRIZE Moon and rover exhibit at the fourth annual WIRED NextFest

Image caption: X PRIZE exhibit of Apollo astronaut and moon rover at the fourth annual WIRED NextFest

The HiRISE team has released more of the high resolution “test” images of Mars taken on March 23 and 25, 2006. Incredible detail, color, and a perspective view. Eight images were taken and the rest should be available tomorrow.

read more | digg story

Mars Reconnaissance Orbiter (MRO) performed a flawless engine burn today in a successful bid to enter orbit around Mars. The event, known as Mars Orbital Insertion (MOI), is a risky one for robotic visitors to the Red Planet. Now that MRO is safely in orbit, the spacecraft will soon begin several months of aerobraking to reshape the orbit into a circle approximately 300 km above the martian surface. The primary science phase of the mission will begin in the fall after aerobraking has been completed.

At the University of Arizona, an audience of students, the public, reporters, and other guests watched live NASA TV coverage of the event. The High Resolution Imaging Science Experiment (HiRISE) camera is one of the instruments on board MRO and is operated by a team at the University of Arizona. HiRISE Principal Investigator Alfred McEwen and operations team members were on hand for presentations, narration of the television coverage, and answers to audience questions. [Disclosure: Richard Leis is a HiRISE operations team member.]

The risks of any orbital insertion include missing the target altogether or coming in too closely. During MRO MOI, all predicted events occurred on schedule, including the loss of signal from the spacecraft while it passed behind Mars. Reacquisition of the signal from MRO occurred at around 3:15 pm Mountain Standard time, and a few minutes later flight operations at the Jet Propulsion Laboratory in Pasadena, California, USA confirmed that the spacecraft was in the correct initial orbit around Mars. The audience and HiRISE team applauded and cheered the successful conclusion of each major event.

MRO launched from Cape Canaveral in Florida, USA on August 12, 2005. During its 7 month cruise to Mars, instruments on board were turned on and tested in preparation for future science gathering. HiRISE, for example, snapped high resolution images of the moon and stellar clusters. These images are now being used by the operations team to calibration the instrument and develop imaging processing software and procedures.

MRO will remain in its current orbit for about two weeks prior to the start of aerobraking. During that two weeks, some of the operations teams for the various instruments will again turn on their instruments. HiRISE will take nine images of Mars and once again the operations team will use these images for further calibration and testing.

Aerobraking occurs when MRO dips down into the martian atmosphere to create friction that helps slow down the spacecraft and lower its orbit. The process will take from five to seven months depending on the condition of the martian atmosphere on any given day.

After aerobraking, MRO will into a transition orbit during which time the instrument teams will complete their preparations for the primary science phase of the mission. Know as PSP, this phase of the mission will last for two years while scientific data is gathered.

The HiRISE camera is the largest such device ever sent outside the Earth’s orbit. The camera will capture high resolution images of the martian surface, up to 20,000 by 60,000 pixels in size. These images are so huge that they will not fit full size on a regular computer monitor. Only a display array of 20 by 60 monitors would have enough pixels available to show one full-sized HiRISE image. Because of this, recent compression and delivery technology known as JPEG2000 is being used to allow the scientific community and the public to browse through these images over the internet.

At its best setting, HiRISE will be able to see objects roughly one meter (approximately one yard) in size. Meanwhile, two other cameras will take lower resolution images but provide more coverage of the planet. Together, these cameras should reveal a different Mars than shown by previous orbiters, simply because so much more detail and wider coverage will become available than ever before. In fact, so much data will be obtained during the course of the mission that it will dwarf what many previous missions have obtained, combined.

MRO is also equipped with a sounding radar called SHARAD (Shallow Radar) which will return the highest resolution data of the martian subsurface. In recent years, previous spacecraft have detected the presence of water deposits beneath the surface of Mars. SHARAD will attempt to better quantify the amount of water present and in what form – ice or liquid – it exists.

Scientists hope to learn where the water believed to have existed on early Mars went, in what form it exists today, and if water might still flow on the surface (as appears to be the case with gullies discovered by previous spacecraft.) They also hope to learn more about the martian atmosphere and surface history. The information obtained could help determine whether or not Mars has ever been hospitable to life and which locations are best to search for fossil or current lifeforms.

More Information

• Mars Reconnaissance Orbiter (MRO)
• The view from MRO.
• HiRISE
  • HiRISE Presentation (Powerpoint file)
  • Mars Mania II - Saturday, April 08, 2006 at the University of Arizona campus

The modern robotic investigation of comets began with a spacecraft from the European Space Agency (ESA) named Giotto. Giotto captured in 1986 the first close-up images of a cometary nucleus and a wealth of other data. ESA is marking the 20th anniversary of Giotto’s successful flyby of Comet Halley on the eve of a NASA press conference regarding science results from the Stardust mission. Twenty years after Giotto, our knowledge about comets, those cold remnants of our solar system’s formation, is undergoing a revolution.

By 1986, six spacecraft were ready for an unprecedented scientific investigation of Comet Halley as it returned to the inner solar system. Due to budget cuts, NASA’s ambitious plans to study Comet Halley were reduced to long distance observations using the International Sun-Earth Explorer 3 (ISEE-3) spacecraft (renamed Interplanetary Comet Explorer (ICE)) already in operations. Meanwhile, after flying by Venus, the Russian Space Research Institute (IKI) spacecrafts VEGA-1 and VEGA-2 were directed toward Comet Halley. Japan’s Institute of Space and Aeronautical Science, which in 2003 became part of Japan Aerospace Exploration Agency (JAXA), used their existing SAKIGAKE (MS-T5) spacecraft for long distance observations and launched SUISEI (PLANET-A), a spacecraft specifically built to study Comet Halley. ESA’s Giotto spacecraft rounded out “Halley Armada.”

Named after the painter of “Adoration of the Magi” which includes a representation of a comet widely believed to be based on Comet Halley, Giotti flew closer to the comet than any of the other spacecraft. The dramatic images and other data returned revealed that Halley was not a round and icy “snow ball” as expected but instead an irregular and dark “dirt ball.” Jets of ice and gas volatiles erupted from the sun-heated surface of the nucleus, creating the bright and extensive coma and tail visible from the Earth.

This first close-up look at a comet revolutionized our understanding of the objects. Since then, several other robotic missions have provided even more highly detailed images and data. Tomorrow, scientists will hold a press conference to report the first science results from their analysis of the first pristine cometary material returned to Earth for extensive analysis. What we learn from the Stardust mission will no doubt radically advance our knowledge.

In twenty years, from the first close-up images of a comet to the first cometary material returned for study, we have learned more about the formation of our solar system and perhaps even the history of life on Earth than in all the thousands of years of comet observation that preceded the Space Age. From Giotto to Stardust in the blink of an eye.

More Information

• ESA Press Release - “Giotto’s brief encounter“
• Halley Armada:
  • Interplanetary Comet Explorer (ICE)
  • SUISEI (PLANET-A)
  • SAKIGAKE (MS-T5)
  • VEGA-1 and VEGA-2
  • Giotto
• Stardust
  • Press Conference, Monday, March 13, 2006 - “NASA ANNOUNCES FIRST STARDUST COMET SAMPLE RESULTS” | Announcement | NASA TV