Missions Archives

June 25, 2015December 23, 2015 by Ken Kremer

Rosetta Orbiter Approved for Extended Mission and Bold Comet Landing

This single frame Rosetta navigation camera image of Comet 67P/Churyumov-Gerasimenko was taken on 15 June 2015 from a distance of 207 km from the comet centre. The image has a resolution of 17.7 m/pixel and measures 18.1 km across. Credit: ESA/Rosetta/NAVCAM – CC BY-SA IGO 3.0

Rosetta will attempt comet landing
This single frame Rosetta navigation camera image of Comet 67P/Churyumov-Gerasimenko was taken on 15 June 2015 from a distance of 207 km from the comet centre. The image has a resolution of 17.7 m/pixel and measures 18.1 km across. Credit: ESA/Rosetta/NAVCAM – CC BY-SA IGO 3.0 [/caption]

Europe’s history making Rosetta cometary spacecraft has been granted a nine month mission extension to plus up its bountiful science discoveries as well as been given the chance to accomplish one final and daring historic challenge, as engineers attempt to boldly go and land the probe on the undulating surface of the comet its currently orbiting.

Officials with the European Space Agency (ESA) gave the “GO” on June 23 saying “The adventure continues” for Rosetta to march forward with mission operations until the end of September 2016.

If all continues to go well “the spacecraft will most likely be landed on the surface of Comet 67P/Churyumov-Gerasimenko” said ESA to the unabashed glee of the scientists and engineers responsible for leading Rosetta and reaping the rewards of nearly a year of groundbreaking research since the probe arrived at comet 67P in August 2014.

“This is fantastic news for science,” says Matt Taylor, ESA’s Rosetta Project Scientist, in a statement.

It will take about 3 months for Rosetta to spiral down to the surface.

After a decade long chase of over 6.4 billion kilometers (4 Billion miles), ESA’s Rosetta spacecraft arrived at the pockmarked Comet 67P/Churyumov-Gerasimenko on Aug. 6, 2014 for history’s first ever attempt to orbit a comet for long term study.

Since then, Rosetta deployed the piggybacked Philae landing craft to accomplish history’s first ever touchdown on a comets nucleus on November 12, 2014. It has also orbited the comet for over 10 months of up close observation, coming at times to as close as 8 kilometers. It is equipped with a suite 11 instruments to analyze every facet of the comet’s nature and environment.

ESA Philae lander approaches comet 67P/Churyumov–Gerasimenko on 12 November 2014 as imaged from Rosetta orbiter after deployment and during seven hour long approach for 1st ever touchdown on a comets surface. Credit: ESA/Rosetta/MPS for OSIRIS Team MPS/UPD/LAM/IAA/SSO/INTA/UPM/DASP/IDA - Composition by Marco Di Lorenzo/Ken Kremer — ESA Philae lander approaches comet 67P/Churyumov–Gerasimenko on 12 November 2014 as imaged from Rosetta orbiter after deployment and during seven hour long approach for 1st ever touchdown on a comets surface. Credit: ESA/Rosetta/MPS for OSIRIS Team MPS/UPD/LAM/IAA/SSO/INTA/UPM/DASP/IDA – Composition by Marco Di Lorenzo/Ken Kremer

Currently, Comet 67P is still becoming more and more active as it orbits closer and closer to the sun over the next two months. The mission extension will enable researchers to a far greater period of time to compare the comets activity, physical and chemical properties and evolution ‘before and after’ they arrive at perihelion some six weeks from today.

The pair reach perihelion on August 13, 2015 at a distance of 186 million km from the Sun, between the orbits of Earth and Mars.

“We’ll be able to monitor the decline in the comet’s activity as we move away from the Sun again, and we’ll have the opportunity to fly closer to the comet to continue collecting more unique data. By comparing detailed ‘before and after’ data, we’ll have a much better understanding of how comets evolve during their lifetimes.”

Because the comet is nearly at its peak of outgassing and dust spewing activity, Rosetta must observe the comet from a stand off distance, while still remaining at a close proximity, to avoid damage to the probe and its instruments.

Furthermore, the Philae lander “awoke” earlier this month after entering a sven month hibernation period after successfully compleing some 60 hours of science observations from the surface.

Jets of gas and dust are blasting from the active neck of comet 67P/Churyumov-Gerasimenko in this photo mosaic assembled from four images taken on 26 September 2014 by the European Space Agency’s Rosetta spacecraft at a distance of 26.3 kilometers (16 miles) from the center of the comet. Credit: ESA/Rosetta/NAVCAM/Marco Di Lorenzo/Ken Kremer/kenkremer.com

As the comet again edges away from the sun and becomes less active, the team will attempt to land Rosetta on comet 67P before it runs out of fuel and the energy produced from the huge solar panels is insufficient to continue mission operations.

“This time, as we’re riding along next to the comet, the most logical way to end the mission is to set Rosetta down on the surface,” says Patrick Martin, Rosetta Mission Manager.

“But there is still a lot to do to confirm that this end-of-mission scenario is possible. We’ll first have to see what the status of the spacecraft is after perihelion and how well it is performing close to the comet, and later we will have to try and determine where on the surface we can have a touchdown.”

During the extended mission, the team will use the experience gained in operating Rosetta in the challenging cometary environment to carry out some new and potentially slightly riskier investigations, including flights across the night-side of the comet to observe the plasma, dust, and gas interactions in this region, and to collect dust samples ejected close to the nucleus, says ESA.

Rosetta’s lander Philae has returned the first panoramic image from the surface of a comet. The view as it has been captured by the CIVA-P imaging system, shows a 360º view around the point of final touchdown. The three feet of Philae’s landing gear can be seen in some of the frames. Superimposed on top of the image is a sketch of the Philae lander in the configuration the lander team currently believe it is in. The view has been processed to show further details. Credit: ESA/Rosetta/Philae/CIVA. Post processing: Ken Kremer/Marco Di Lorenzo

Stay tuned here for Ken’s continuing Earth and planetary science and human spaceflight news.

Ken Kremer

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Learn more about Rosetta, SpaceX, Europa, Mars rovers, Orion, SLS, Antares, NASA missions and more at Ken’s upcoming outreach events:

Jun 25-28: “SpaceX launch, Orion, Commercial crew, Curiosity explores Mars, Antares and more,” Kennedy Space Center Quality Inn, Titusville, FL, evenings

This single frame Rosetta navigation camera image was taken from a distance of 77.8 km from the centre of Comet 67P/Churyumov-Gerasimenko on 22 March 2015. The image has a resolution of 6.6 m/pixel and measures 6 x 6 km. The image is cropped and processed to bring out the details of the comet’s activity. Credit: ESA/Rosetta/NAVCAM – CC BY-SA IGO 3.0

June 19, 2015December 30, 2015 by Susie Murph

NASA’S New Horizon’s Hangout: Countdown to Pluto!

Check out our own Fraser Cain and the scientists from the New Horizon team as they discuss the imminent arrival of the New Horizons spacecraft at Pluto!

Watch the hangout here and subscribe to the New Horizons YouTube Channel!

June 15, 2015December 23, 2015 by Ken Kremer

First Interplanetary CubeSats to Launch on NASA’s 2016 InSight Mars Lander

NASA’s two small MarCO CubeSats will be flying past Mars in 2016 just as NASA’s next Mars lander, InSight, is descending to land on the surface. MarCO, for Mars Cube One, will provide an experimental communications relay to inform Earth quickly about the landing. Credits: NASA/JPL-Caltech
See fly by and cubesat spacecraft graphics and photos below[/caption]

CubeSats are taking the next great leap for science – departing Earth and heading soon for the fourth rock from the Sun.

For the first time, two tiny CubeSat probes will launch into deep space in early 2016 on their first interplanetary expedition – aiming for the Red Planet as part of an experimental technology relay demonstration project aiding NASA’s next Mission to Mars; the InSight lander.

NASA announced the pair of briefcase-sized CubeSats, called Mars Cube One or MarCO, as a late and new addition to the InSight mission, that could substantially enhance communications options on future Mars missions. They were designed and built by NASA’s Jet Propulsion Laboratory (JPL), Pasadena, California.

InSight, which stands for Interior Exploration Using Seismic Investigations, Geodesy and Heat Transport, is a stationary lander. It will join NASA’s surface science exploration fleet currently comprising of the Curiosity and Opportunity missions which by contrast are mobile rovers.

InSight is the first mission to understand the interior structure of the Red Planet. Its purpose is to elucidate the nature of the Martian core, measure heat flow and sense for “Marsquakes.”

The full-scale mock-up of NASA's MarCO CubeSat held by Farah Alibay, a systems engineer for the technology demonstration, is dwarfed by the one-half-scale model of NASA's Mars Reconnaissance Orbiter behind her. Credits: NASA/JPL-Caltech — The full-scale mock-up of NASA’s MarCO CubeSat held by Farah Alibay, a systems engineer for the technology demonstration, is dwarfed by the one-half-scale model of NASA’s Mars Reconnaissance Orbiter behind her. Credits: NASA/JPL-Caltech

Because of their small size – roughly 4 inches (10 centimeters) square) – and simplicity using off-the-shelf components, they are a favored platform for university students and others seeking low cost access to space – such as the Planetary Society’s recently successful Light Sail solar sailing cubesat demonstration launched in May. Six units are combined together to create MarCO.

Over the past few years many hundreds of cubesats have already been deployed in Earth orbit – including many dozens from the International Space Station (ISS) – but these will be the first going far beyond our Home Planet.

Data relayed by MarCO at 8 kbps in real time could reveal InSight’s fate on the Martian surface within minutes to mission controllers back on Earth, rather than waiting for a potentially prolonged period of agonizing nail-biting lasting an hour or more.

The two probes, known as MarCO-A and MarCO-B, will operate during InSight’s highly complex entry, descent and landing (EDL) operations as it descends through the thin Martian atmosphere. Their function is merely to quickly relay landing data. But the cubesats will have no impact on the ultimate success of the mission. They will intentionally sail by but not land on Mars.

“MarCO is an experimental capability that has been added to the InSight mission, but is not needed for mission success,” said Jim Green, director of NASA’s planetary science division at the agency’s headquarters in Washington, in a statement.

The MarCO Cubesats will serve as a test bed for a revolutionary communications mode that seeks to quickly relay data back to Earth about the status of InSight – in real time – as it plummets down to the Red Planet for the “Seven Minutes of Terror” that hopefully climaxes with a soft landing.

The MarCO duo will fly by past Mars at a planned distance and altitude of about 3,500 kilometers as InSight descends towards the surface during EDL operations. They will rapidly retransmit signals coming from the lander in real time, directly back to NASA’s huge Deep Space Network (DSN) receiving dish antennas back on Earth.

MarCO cubesats fly by trajectory for rapid communications relay as NASA’s InSight spacecraft lands on Mars in September 2016. Credit: NASA/JPL-Caltech

For this flight, six cubesats will be joined together to provide the additional capability required for the journey to Mars and to accomplish their communications task.

The six-unit MarCO CubeSat has a stowed size of about 14.4 inches (36.6 centimeters) by 9.5 inches (24.3 centimeters) by 4.6 inches (11.8 centimeters) and weighs 14 kilograms.

The solar powered probes will be outfitted with UHF and X-band communications gear as well as propulsion, guidance and more.

The overall cost to design, build, launch and operate MarCO-A and MarCO-B is approximately $13 million, a NASA spokesperson told Universe Today.

InSight and MarCO are slated to blastoff together on March 4, 2016 atop a United Launch Alliance Atlas V rocket from Vandenberg Air Force Base, California.

After launch, both MarCO CubeSats will separate from the Atlas V booster and travel along their own trajectories to the Red Planet.

“MarCO will fly independently to Mars,” says Green.

They will be navigated independently from InSight. They will all reach Mars at approximately the same time for InSight’s landing slated for Sept. 28, 2016.

MarCO’s two solar panels and two radio antennas will unfurl after being released from the Atlas booster. The high-gain, X-band antenna is a flat panel engineered to direct radio waves the way a parabolic dish antenna does,” according to a NASA description.

The softball-size radio “provides both UHF (receive only) and X-band (receive and transmit) functions capable of immediately relaying information received over UHF.”

MarCO cubesat graphic annotated to show dimensions, instruments, physical characteristics and capabilities. Credit: NASA/JPL-Caltech

During EDL, InSight will transmit landing data via UHF radio to the MarCO cubesats sailing past Mars as well as to NASA’s Mars Reconnaissance Orbiter (MRO) soaring overhead.

MarCO will assist InSight by receiving the lander information transmitted in the UHF radio band and then immediately forward EDL information to Earth using the X-band radio. By contrast, MRO cannot simultaneously receive information over one band while transmitting on another, thus delaying confirmation of a successful landing possibly by an hour or more.

Engineers for NASA's MarCO technology demonstration display a full-scale mechanical mock-up of the small craft in development as part of NASA's next mission to Mars. Mechanical engineer Joel Steinkraus and systems engineer Farah Alibay are on the team at NASA's Jet Propulsion Laboratory, Pasadena, California, preparing twin MarCO (Mars Cube One) CubeSats for a March 2016 launch. Credit: NASA/JPL-Caltech — Engineers for NASA’s MarCO technology demonstration display a full-scale mechanical mock-up of the small craft in development as part of NASA’s next mission to Mars. Mechanical engineer Joel Steinkraus and systems engineer Farah Alibay are on the team at NASA’s Jet Propulsion Laboratory, Pasadena, California, preparing twin MarCO (Mars Cube One) CubeSats for a March 2016 launch. Credit: NASA/JPL-Caltech

“Ultimately, if the MarCO demonstration mission succeeds, it could allow for a “bring-your-own” communications relay option for use by future Mars missions in the critical few minutes between Martian atmospheric entry and touchdown,” say NASA officials.

It’s also very beneficial and critical to the success of future missions to have a stream of data following the progress of past missions so that lessons can be learned and applied, whatever the outcome.

“By verifying CubeSats are a viable technology for interplanetary missions, and feasible on a short development timeline, this technology demonstration could lead to many other applications to explore and study our solar system,” says NASA.

InSight will smash into the Martian atmosphere at high speeds of approximately 13,000 mph in September 2016 and then decelerate within a few minutes for landing via a heat shield, retro rocket and parachute assisted touchdown on the plains at flat-lying terrain at “Elysium Planitia,” some four degrees north of Mars’ equator, and a bit north of the Curiosity rover.

As I reported in recently here, InSight has now been assembled into its flight configuration and begun a comprehensive series of rigorous environmental stress tests that will pave the path to launch in 2016 on a mission to unlock the riddles of the Martian core.

The countdown clock is ticking relentlessly towards liftoff in less than nine months time in March 2016.

NASA's InSight Mars lander spacecraft in a Lockheed Martin clean room near Denver. As part of a series of deployment tests, the spacecraft was commanded to deploy its solar arrays in the clean room to test and verify the exact process that it will use on the surface of Mars. Credits: NASA/JPL-Caltech/Lockheed Martin — NASA’s InSight Mars lander spacecraft in a Lockheed Martin clean room near Denver. As part of a series of deployment tests, the spacecraft was commanded to deploy its solar arrays in the clean room to test and verify the exact process that it will use on the surface of Mars. Credits: NASA/JPL-Caltech/Lockheed Martin

Stay tuned here for Ken’s continuing Earth and planetary science and human spaceflight news.

Ken Kremer

June 13, 2015December 23, 2015 by Bob King

Have We Found Rosetta’s Lost Philae Lander?

Left image from Rosetta’s OSIRIS narrow-angle camera shows the Philae lander on November 12, 2014 after it left the spacecraft for the comet's nucleus. Right: Close-up of a promising candidate for the lander photographed on December 12. Copyright: ESA/Rosetta/MPS for OSIRIS Team MPS/UPD/LAM/IAA/SSO/INTA/UPM/DASP/IDA

It’s only a bright dot in a landscape of crenulated rocks, but the Rosetta team thinks it might be Philae, the little comet lander lost since November.

The Rosetta and Philae teams have worked tirelessly to search for the lander, piecing together clues of its location after a series of unfortunate events during its planned landing on the surface of Comet 67P/Churyumov-Gerasimenko last November 12.

The journey of Rosetta’s Philae lander as it approached and then rebounded from its first touchdown on Comet 67P/Churyumov–Gerasimenko on November 12, 2014. The mosaic comprises a series of images captured by Rosetta’s OSIRIS camera over a 30 minute period spanning the first touchdown. The time of each of image is marked on the corresponding insets and is in Greenwich Mean Time. Credit: ESA/Rosetta/MPS for OSIRIS Team MPS/UPD/LAM/IAA/SSO/INTA/UPM/DASP/IDA — Mosaic photo capturing Philae’s flight above the comet’s nucleus and one of its three touchdowns on November 12, 2014. The images cover a 30 minute period spanning the first touchdown. The Greenwich Mean Time time of each of image is marked on the corresponding insets. Credit: ESA/Rosetta/MPS for OSIRIS Team MPS/UPD/LAM/IAA/SSO/INTA/UPM/DASP/IDA

Philae first touched down at the Agilkia landing site that day, but the harpoons that were intended to anchor it to the surface failed to work, and the ice screws alone weren’t enough to do the job. The lander bounced after touchdown and sailed above the comet’s nucleus for two hours before finally settling down at a site called Abydos a kilometer from its intended landing site.

No one yet knows exactly where Philae is, but an all-out search has finally turned up a possible candidate.

Approximate locations of five lander candidates initially identified in high-resolution photos taken in December 2014, from a distance of about 12.4 miles (20 km) from the comet's center. The candidates identify Philae-sized features about 3-6 feet (1-2 meters) across. The contrast has been stretched in some of the images to better reveal the candidates. All but one of these candidates (top left) have subsequently been ruled out. The candidate at top left lies near to the current CONSERT ellipse (see below). Credit: ESA/Rosetta/NavCam – CC BY-SA IGO 3.0; insets: ESA/Rosetta/MPS for OSIRIS Team MPS/UPD/LAM/IAA/SSO/INTA/UPM/DASP/IDA — Approximate locations of five lander candidates initially identified in high-resolution photos taken in December 2014, from a distance of about 12.4 miles (20 km) from the comet’s center. The candidates identify Philae-sized features about 3-6 feet (1-2 meters) across. The contrast has been stretched in some of the images to better reveal the candidates. All but one of them (top left) have subsequently been ruled out. The candidate at top left lies near to the current CONSERT ellipse (see below). Credit: ESA/Rosetta/NavCam – CC BY-SA IGO 3.0; insets: ESA/Rosetta/MPS for OSIRIS Team MPS/UPD/LAM/IAA/SSO/INTA/UPM/DASP/IDA

Rosetta’s navigation and high-resolution cameras identified the first landing site and also took several pictures of Philae as it traveled above the comet before coming down for a final landing. Magnetic field measurements taken by an instrument on the lander itself also helped establish its location and orientation during flight and touchdown. The lander is thought to be in rough terrain perched up against a cliff and mostly in shadow.

High resolution images of the possible landing zone were taken by Rosetta back in December when it was about 11 miles (18 km) from the comet’s surface. At this distance, the OSIRIS narrow-angle camera has a resolution of 13.4 inches (34 cm) per pixel. The body of Philae is just 39 inches (1-meter) across, while its three thin legs extend out by up to 4.6 feet (1.4-meters) from its center. In other words, Philae’s just a few pixels across — a tiny target but within reach of the camera’s eye.

The current 50 x 525 feet (16 x 160 m) CONSERT ellipse overlaid on an OSIRIS narrow-angle camera image of the same region. It's believed Philae is located within or near this ellipse. Copyright Ellipse: ESA/Rosetta/Philae/CONSERT; Image: ESA/Rosetta/MPS for OSIRIS Team MPS/UPD/LAM/IAA/SSO/INTA/UPM/DASP/IDA — The current 50 x 525 feet (16 x 160 m) CONSERT ellipse overlaid on an OSIRIS narrow-angle camera image of the same region. It’s believed Philae is located within or near this ellipse. Copyright Ellipse: ESA/Rosetta/Philae/CONSERT; Image: ESA/Rosetta/MPS for OSIRIS Team MPS/UPD/LAM/IAA/SSO/INTA/UPM/DASP/IDA

The candidates in the photo above are “all over the place.” To narrow down the location, the Rosetta team used radio signals sent between Philae and Rosetta as part of the COmet Nucleus Sounding Experiment or CONSERT after the final touchdown. According to Emily Baldwin’s recent posting on the Rosetta site:

“Combining data on the signal travel time between the two spacecraft with the known trajectory of Rosetta and the current best shape model for the comet, the CONSERT team have been able to establish the location of Philae to within an ellipse roughly 50 x 525 feet (16 x 160 meters) in size, just outside the rim of the Hatmehit depression.”

Zooming in towards the current CONSERT ellipse, a number of bright dots are seen in the region. As only one (at most) of these could be the lander, the majority must be associated with surface features on the comet nucleus. Credits: ESA/Rosetta/MPS for OSIRIS Team MPS/UPD/LAM/IAA/SSO/INTA/UPM/DASP/IDA — Zooming in to the CONSERT ellipse, a number of bright dots are seen in the region. Since only one could be the lander, the majority must be associated with surface features on the comet nucleus.
Credits: ESA/Rosetta/MPS for OSIRIS Team MPS/UPD/LAM/IAA/SSO/INTA/UPM/DASP/IDA

So what can we see there? Zooming in closer, a number of glints or bright spots appear, and they change depending on the viewing angle. But among those glints, one might be Philae. What mission scientists examined images of the area under the same lighting conditions before Philae landed and then put them side by side with those taken after November 12. That way any transient glints could be eliminated, leaving what’s left as a potential candidate.

‘Before’ and ‘after’ comparison images of a promising candidate located near the CONSERT ellipse as seen in images from Rosetta. Each box covers roughly 65x65 feet (20 x 20 m) on the comet. The left-hand image shows the region as seen on 22 October (before the landing of Philae) from a distance of about 6 miles from the center of the comet, while the center and right-hand images show the same region on December 12 and 13 from 12 miles (20 km) after landing. The candidate is only seen in the two later pictures. Credits: ESA/Rosetta/MPS for OSIRIS Team MPS/UPD/LAM/IAA/SSO/INTA/UPM/DASP/IDA — ‘Before’ and ‘after’ comparison images of a promising candidate located near the CONSERT ellipse as seen in images from Rosetta. Each box covers roughly 65×65 feet (20 x 20 m) on the comet. The left-hand image shows the region as seen on 22 October (before the landing of Philae) from a distance of about 6 miles from the center of the comet, while the center and right-hand images show the same region on December 12 and 13 from 12 miles (20 km) after landing. The candidate is only seen in the two later pictures.
Credits: ESA/Rosetta/MPS for OSIRIS Team MPS/UPD/LAM/IAA/SSO/INTA/UPM/DASP/IDA

In photos taken on December 12 and 13, a bright spot is seen that didn’t appear in the earlier photos. Might this be Philae? It’s possible and the best candidate yet. But it may also be a new physical feature that developed between November and December. Comet surfaces are forever changing as sunlight sublimates ice both on and beneath the surface

For now, we still can’t be sure if we’ve found Philae. Higher resolution pictures will be required as will patience. The comet’s too close to the Sun right now and too active. Rubble flying off the nucleus could damage Rosetta’s instruments. Mission scientists will have to wait until well after the comet’s August perihelion (closest approach to the Sun) for a closer look.

Comet 67P/Churyumov-Gerasimenko photographed from about 125 miles away on June 5 looks simply magnificent. Only two months from perihelion, the comet shows plenty of jets. One wonders what the chances are of one erupting underneath Philae and sending it back into orbit again. Credit: ESA/Rosetta/NAVCAM – CC BY-SA IGO 3.0 — Magnificent! Comet 67P/Churyumov-Gerasimenko photographed by Rosetta from about 125 miles away on June 5, 2015. Now only two months from perihelion, the comet’s crazy with jets of dust and gas. One wonders what the chances are of a gassy geyser erupting beneath or near Philae and sending it back into orbit again. Credit: ESA/Rosetta/NAVCAM – CC BY-SA IGO 3.0

Meanwhile, mission teams remain hopeful that with increasing sunlight at the comet this summer, Philae’s solar panels will recharge its batteries and the three-legged lander will wake up and resume science studies. Three attempts have been made to contact Philae this spring and more will be made but so far, we’ve not heard a peep.

For the time being, Philae’s like that lost child in a shopping mall. The search party’s been dispatched, clues have been found and it’s only a matter of time before we see her smiling face again.

June 11, 2015December 23, 2015 by Ken Kremer

Record Setting Italian Female Astronaut and ISS Crewmates Land in Sunny Kazakhstan

The Soyuz TMA-15M spacecraft is seen as it lands with Expedition 43 commander Terry Virts of NASA, cosmonaut Anton Shkaplerov of the Russian Federal Space Agency (Roscosmos), and Italian astronaut Samantha Cristoforetti from European Space Agency (ESA) near the town of Zhezkazgan, Kazakhstan on Thursday, June 11, 2015. Virtz, Shkaplerov, and Cristoforetti are returning after more than six months onboard the International Space Station where they served as members of the Expedition 42 and 43 crews. Photo Credit: (NASA/Bill Ingalls)

An international crew comprising a Russian cosmonaut, a US astronaut and an Italian astronaut who accomplished a record setting flight for time in space by a female, departed the International Space Station (ISS) earlier today, June 11, and safely landed in sunny and warm Kazakhstan tucked inside their Russia Soyuz ferry ship after a successful and extended 199-day mission devoted to science and station upgrades.

The multinational trio comprising Expedition 43 Commander Terry Virts of NASA, Flight Engineers Anton Shkaplerov of the Russian Federal Space Agency (Roscosmos) and Samantha Cristoforetti of ESA (European Space Agency) undocked from the orbiting outposts Russian Rassvet module as scheduled in the Soyuz TMA-15M spaceship at 6:20 a.m. EDT while soaring some 250 miles (400 kilometers) above Mongolia.

A four-minute 40-second deorbit burn at 8:51 a.m EDT slowed the craft for the fiery reentry into the Earth’s atmosphere.

The crew touched down just a few hours after undocking at 9:44 a.m. EDT (7:44 p.m., Kazakh time), southeast of the remote town of Dzhezkazgan on the steppes of Kazakhstan, about an hour and a half before sundown in delightfully summer weather. Temperatures today were in the 80s, but they are ‘bone chilling’ in the winter months.

Expedition 43 Commander Terry Virts of NASA, Flight Engineers Anton Shkaplerov of the Russian Federal Space Agency (Roscosmos) and Samantha Cristoforetti of ESA (European Space Agency) touched down at 9:44 a.m. EDT (7:44 p.m., Kazakh time), southeast of the remote town of Dzhezkazgan in Kazakhstan. Credits: NASA TV

The Expedition 43 flight was extended at the last minute due to the surprise launch failure of a Russian rocket carrying a station bound Progress resupply ship in late April.

The Progress 59 cargo vessel, also known as Progress M-27M, spun wildly out of control as it separated from the Soyuz-2.1A carrier rocket. The freighter and all its 2.5 tons of contents fpr the crew were destroyed during an uncontrolled plummet as its crashed back to Earth on May 8.

The Soyuz/Progress 59 failure had far reaching consequences and resulted in a postponement of virtually all Russian crew and cargo flights to the ISS for the remainder of 2015, as announced this week by Roscosmos, the Russian Federal Space Agency.

One result is that Cristoforetti now holds the single mission record for a female astronaut, of nearly 200 days.

Expedition 43 was extended by about a month in the wake of the launch failure of the Progress 59 cargo vessel, which quickly cascaded into an extended mission from its originally planned length of about 170 days to 199+ days.

The Soyuz is only certified to stay on orbit for 200 days. So the return home delayed as much as possible to minimize the time when the ISS reverts to only a three person crew – and consequently reduced time for research.

This past weekend on June 6, Cristoforetti surpassed the female astronaut record of 194 days, 18 hours and 2 minutes established by NASA astronaut Sunita Williams on a prior station flight back in 2007.

Cristoforetti, of the European Space Agency (ESA), is on her first ever space flight also counts as she also counts as Italy’s first female astronaut.

The station departure and parachute assisted soft landing was shown during a live webcast on NASA TV.

“The landing was on time and on target after over 199 days in space,” said NASA commentator Rob Navius.

“Everything went by the book for an on target touchdown. The crew is safely back on Earth!”

Flight Engineer Samantha Cristoforetti of the European Space Agency in Star Trek uniform as SpaceX Dragon arrives at the International Space Station on April 17, 2015. Credit: NASA

In the final stages of the return to Earth, the Soyuz descent module glided down safely using a single mammoth orange and white parachute, aided by braking rockets in the final moments just a few feet above ground.

The Soyuz landed upright, which eased the extraction of the crew. Russian recovery team members hoisted all three up and out from the cramped capsule.

Soyuz commander Anton Shkaplerov was hauled up first, followed by Samantha Cristoforetti and finally Terry Virts.

All three crewmembers were healthy and happy, each signaling their elation with a joyous ‘thumbs up.’

After preliminary medical checks, the crew were flown by helicopter to a staging base at Karaganda. From there they split up. Shkaplerov heads back to Moscow and Star City. Cristoforetti and Virts fly to Mission Control in Houston.

During their time aloft, the crew completed several critical spacewalks, technology demonstrations, and hundreds of scientific experiments spanning multiple disciplines, including human and plant biology,” according to NASA.

Among the research experiments conducted were “participation in the demonstration of new, cutting-edge technologies such as the Synthetic Muscle experiment, a test of a new polymer that contracts and expands similar to real muscle. This technology has the potential for future use on robots, enabling them to perform tasks that require considerable dexterity but are too dangerous to be performed by humans in space.”

“The crew engaged in a number of biological studies, including one investigation to better understand the risks of in-flight infections and another studying the effects microgravity has on bone health during long-duration spaceflight. The Micro-5 study used a small roundworm and a microbe that causes food poisoning in humans to study the risk of infectious diseases in space, which is critical for ensuring crew health, safety and performance during long-duration missions. The Osteo-4 study investigated bone loss in space, which has applications not only for astronauts on long-duration missions, but also for people on Earth affected by osteoporosis and other bone disorders.”

Three cargo flights also arrived at the ISS carrying many tons of essential supplies, research equipment, science experiments, gear, spare parts, food, water, clothing.

The resupply freighters included the Russian Progress in February 2015 as well as two SpaceX Dragon cargo ships on the CRS-5 and CRS-6 flights in January and April.

Expedition 43 commander Terry Virts of NASA, left, cosmonaut Anton Shkaplerov of the Russian Federal Space Agency (Roscosmos), center, and Italian astronaut Samantha Cristoforetti from European Space Agency (ESA) sit in chairs outside the Soyuz TMA-15M spacecraft just minutes after they landed in a remote area near the town of Zhezkazgan, Kazakhstan on Thursday, June 11, 2015. Virtz, Shkaplerov, and Cristoforetti are returning after more than six months onboard the International Space Station where they served as members of the Expedition 42 and 43 crews. Photo Credit: (NASA/Bill Ingalls) — Expedition 43 commander Terry Virts of NASA, left, cosmonaut Anton Shkaplerov of the Russian Federal Space Agency (Roscosmos), center, and Italian astronaut Samantha Cristoforetti from European Space Agency (ESA) sit in chairs outside the Soyuz TMA-15M spacecraft just minutes after they landed in a remote area near the town of Zhezkazgan, Kazakhstan on Thursday, June 11, 2015. Virts, Shkaplerov, and Cristoforetti are returning after more than six months onboard the International Space Station where they served as members of the Expedition 42 and 43 crews. Photo Credit: (NASA/Bill Ingalls)

With the return of Virts crew, the new Expedition 44 begins and comprises NASA astronaut Scott Kelly and Russian cosmonauts Mikhail Kornienko, the two members of the first “ISS 1 Year Mission” as well as cosmonaut Gennady Padalka.

Padalka now assumes command of the station for a record setting fourth time. And he’ll soon be setting another record. In late June, he will break the all time record for cumulative time in space currently held by cosmonaut Sergei Krikalev of 803 days on six space flights.

When Padalka returns to Earth around September 10 in the Soyuz TMA-16M ship, that brought the 1 Year crew to the ISS, he will have been in space for a grand total of over 877 days over five flights.

The next cargo ferry flight involves NASA’s next contracted unmanned Dragon cargo mission by commercial provider SpaceX on the CRS-7 flight.

Dragon CRS-7 is now slated for liftoff on June 26. Watch for my onsite reports from KSC.

The Dragon will be carrying critical US equipment, known as the International Docking Adapter (IDA), enabling docking by the SpaceX Crew Dragon and Boeing CST-100 astronaut transporters – due for first crewed launches in 2017.

The most recent unmanned Dragon cargo CRS-6 mission concluded with a Pacific Ocean splashdown on May 21.

The International Space Station, photographed by the crew of STS-132 as they disembarked. Credit: NASA

Stay tuned here for Ken’s continuing Earth and planetary science and human spaceflight news.

Ken Kremer

Expedition 43 crews rests post landing on Thursday, June 11, 2015, Terry Virts of NASA, comprising cosmonaut Anton Shkaplerov of the Russian Federal Space Agency (Roscosmos), and record setting Italian astronaut Samantha Cristoforetti from European Space Agency (ESA). Credit: NASA

June 9, 2015December 23, 2015 by Ken Kremer

Longest Woman Spaceflyer to Return as Russia Reshuffles Station Launches After Rocket Failure

The longest space mission in history by a female astronaut is now set to conclude on Thursday, following Russia’s confirmation of a significant reshuffling of the crew and cargo flight manifest to the International Space Station (ISS) for the remainder of 2015 – all in the wake of the unexpected Russian launch failure of a station bound Progress resupply ship in late April with far reaching consequences.

The record setting flight of approximately 200 days by Italian spaceflyer Samantha Cristoforetti, along with her two Expedition 43 crewmates, will come to an end on Thursday, June 11, when the trio are set to undock and depart the station aboard their Russian Soyuz crew capsule and return back to Earth a few hours later.

NASA TV coverage begins at 6 a.m. EDT on June 11.

Roscosmos, the Russian Federal Space Agency, officially announced today, June 9, a revamped schedule changing the launch dates of several upcoming crewed launches this year to the Earth orbiting outpost.

Launch dates for the next three Progress cargo flights have also been adjusted.

The next three person ISS crew will now launch between July 23 to 25 on the Soyuz TMA-17M capsule from the Baikonur cosmodrome in Kazakhstan. The exact timing of the Expedition 44 launch using a Russian Soyuz-FG booster is yet to be determined.

Soon after the Progress mishap, the Expedition 43 mission was extended by about a month so as to minimize the period when the ISS is staffed by only a reduced crew of three people aboard – since the blastoff of the next crew was simultaneously delayed by Roscosmos by about two months from May to late July.

Indeed Cristoforetti’s endurance record only came about as a result of the very late mission extension ordered by Roscosmos, so the agency could investigate the root cause of the recent launch failure of the Russian Progress 59 freighter that spun wildly out of control soon after blastoff on April 28 on a Soyuz-2.1A carrier rocket.

Roscosmos determined that the Progress failure was caused by an “abnormal separation of the 3rd stage and the cargo vehicle” along with “associated frequency dynamic characteristics.”

The Expedition 43 crew comprising of Cristoforetti, NASA astronaut and current station commander Terry Virts, and Russian cosmonaut Anton Shkaplerov had been scheduled to head back home around May 13. The trio have been working and living aboard the complex since November 2014.

The 38-year old Cristoforetti actually broke the current space flight endurance record for a female astronaut during this past weekend on Saturday, June 6, when she eclipsed the record of 194 days, 18 hours and 2 minutes established by NASA astronaut Sunita Williams on a prior station flight back in 2007.

Cristoforetti, of the European Space Agency (ESA), also counts as Italy’s first female astronaut.

The Progress 59 cargo vessel, also known as Progress M-27M, along with all its 2.5 tons of contents were destroyed during an uncontrolled plummet back to Earth on May 8.

NASA astronaut Terry Virts (left) Commander of Expedition 43 on the International Space Station along with crewmates Russian cosmonaut Anton Shkaplerov (center) and ESA (European Space Agency) astronaut Samantha Cristoforetti on May 6, 2015 perform a checkout of their Russian Soyuz spacesuits in preparation for the journey back to Earth - now set for June 11, 2015. Credits: NASA — NASA astronaut Terry Virts (left) Commander of Expedition 43 on the International Space Station along with crewmates Russian cosmonaut Anton Shkaplerov (center) and ESA (European Space Agency) astronaut Samantha Cristoforetti on May 6, 2015 perform a checkout of their Russian Soyuz spacesuits in preparation for the journey back to Earth – now set for June 11, 2015. Credits: NASA

Roscosmos announced that they are accelerating the planned launch of the next planned Progress 60 (or M-28M) from August 6 up to July 3 on a Soyuz-U carrier rocket, which is different from the problematic Soyuz-2.1A rocket.

Following the Soyuz crew launch in late July, the next Soyuz will blastoff on Sept. 1 for a 10 day taxi mission on the TMA-18M capsule with cosmonaut Sergei Volkov and ESA astronaut Andreas Mogensen. After British opera singer Sarah Brightman withdrew from participating as a space tourist, a new third crew member will be named soon by Roscosmos.

The final crewed Soyuz of 2015 with the TMA-19M capsule has been postponed from Nov. 20 to Dec. 15.

Also in the mix is the launch of NASA’s next contracted unmanned Dragon cargo mission by commercial provider SpaceX on the CRS-7 flight. Dragon CRS-7 is now slated for liftoff on June 26. Watch for my onsite reports from KSC.

The most recent unmanned Dragon cargo CRS-6 mission concluded with a Pacific Ocean splashdown on May 21.

The Dragon will be carrying critical US equipment, known as the IDA, enabling docking by the SpaceX Crew Dragon and Boeing CST-100 astronaut transporters – due for first crewed launches in 2017.

ESA (European Space Agency) astronaut Samantha Cristoforetti enjoys a drink from the new ISSpresso machine. The espresso device allows crews to make tea, coffee, broth, or other hot beverages they might enjoy. Credit: NASA

NASA astronaut Scott Kelly and Russian cosmonauts Mikhail Kornienko and Gennady Padalka will remain aboard the station after the Virts crew returns to begin Expedition 44.

Stay tuned here for Ken’s continuing Earth and planetary science and human spaceflight news.

Ken Kremer

June 8, 2015December 23, 2015 by Ken Kremer

Dawn Does Dramatic Fly Over of Ceres, Enters Lower Mapping Orbit: Video

This image of Ceres was taken by NASA's Dawn spacecraft on May 7, 2015, from a distance of 8,400 miles (13,600 kilometers). Credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDA

Video caption: This new video animation of Ceres was created from images taken by NASA’s Dawn spacecraft at altitudes of 8,400 miles (13,600 kilometers) and 3,200 miles (5,100 kilometers) away. Vertical dimension has been exaggerated by a factor of two and a star field added. Credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDA

Scientists leading NASA’s Dawn mission to dwarf planet Ceres have just released a brand new animated video showing a dramatic fly over of the heavily cratered world featuring its mysterious bright spots whose exact origin and nature remain elusive.

Meanwhile, the venerable probe has just successfully entered its new and lower mapping orbit on June 3 from which researchers hope to glean hordes of new data to unravel the secrets of the bright spots and unlock the nature of Ceres origin and evolution.

Pockmarked Ceres is an alien world unlike any other in our solar system.

“Dawn completed the maneuvering to reach its second mapping orbit and stopped ion-thrusting on schedule. Since May 9, the spacecraft has reduced its orbital altitude from 8,400 miles (13,600 kilometers) to 2,700 miles (4,400 kilometers),” reported Marc Rayman, Dawn Chief Engineer/ Mission Director of NASA’s Jet Propulsion Laboratory, Pasadena, California.

“As Dawn flew 2,700 miles (4,400 kilometers) over Ceres’ north pole on June 5 that marked the beginning of the new mapping phase, and Dawn began taking photos and making other measurements on schedule.”

Each orbit of Dawn around Ceres at this second science mapping orbit lasts 3.1 days.

The new video was created by the research team based on observations of Ceres that were taken from Dawn’s initial mapping orbit, at an altitude of 8,400 miles (13,600 kilometers), as well as the most recent navigational images taken from 3,200 miles (5,100 kilometers), according to NASA.

It is based on data from over 80 images captured by Dawn’s framing cameras which were provided The German Aerospace Center (DLR) and Max Planck Institute for Solar System Research in Göttingen, Germany.

The images were used to provide a three-dimensional video view. The vertical dimension is exaggerated by a factor of two in the video.

“We used a three-dimensional terrain model that we had produced based on the images acquired so far,” said Dawn team member Ralf Jaumann of the German Aerospace Center (DLR), in Berlin.

“They will become increasingly detailed as the mission progresses — with each additional orbit bringing us closer to the surface.”

Imagery of the mysterious bright spots show them to seemingly be sheets of many spots of water ice, and not just single huge patches. The famous duo of ice spots are located inside the middle of a 57 miles (92 kilometers) wide crater situated in Ceres northern hemisphere.

Dawn is an international science mission managed by NASA’s Jet Propulsion Laboratory, Pasadena, California. The trio of science instruments are from the US, Germany and Italy.

The framing camera was provided by the Max Planck Institute for Solar System Research, Göttingen, Germany and the German Aerospace Center (DLR).

This view of Ceres was taken by Dawn spacecraft on May 23 and shows finer detail becoming visible on the dwarf planet. The spacecraft snapped the image at a distance of 3,200 miles (5,100 kilometers) with a resolution of 1,600 feet (480 meters) per pixel. Credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDA

Dawn will spend most if June at this second mapping orbit before firing up the ion engines and spiraling yet lower for a mission expected to last until at least June 2016.

Stay tuned here for Ken’s continuing Earth and planetary science and human spaceflight news.

Ken Kremer

Dawn’s spiral descent from its first mapping orbit (RC3) to its second (survey). The two mapping orbits are shown in green. The color of Dawn’s trajectory progresses through the spectrum from blue, when it began ion-thrusting on May 9, to red, when ion-thrusting concludes on June 3. The red dashed sections show where Dawn is coasting, mostly for telecommunications. The first two coast periods include OpNav 8 and 9. Image credit: NASA/JPL-Caltech

June 4, 2015December 23, 2015 by Bob King

Chaos Reigns At Pluto’s Moons

This set of computer modeling illustrations of Pluto’s moon Nix shows how the orientation of the moon changes unpredictably as it orbits the “double planet” Pluto-Charon. Credit: NASA/ESA/M. Showalter (SETI)/G. Bacon (STScI)

Simulation of Pluto’s moon Nix sped up so that one orbit takes 2 seconds instead of 25 days.

Wobbling and tumbling end-over-end like a badly thrown football, Pluto’s moons are in a state of orbital chaos, say scientists. Analysis of data from NASA’s Hubble Space Telescope shows that two of Pluto’s moons, Nix and Hydra, wobble unpredictably. If you lived on either, you’d never know when and in what direction the Sun would rise. One day it would pop up over your north horizon, the next over the western. Every sunset would be like a proverbial snowflake — not a single one the same.

Watch the video, and you’ll see what I mean. Not only does the moon totter, but the poles flip. If there was ever a solar system body to meet the criteria of end-of-the-world, doomsday crowd, Nix is it. The moons wobble because they’re embedded in the bizarro gravity field of the Pluto-Charon duo. Charon is officially the dwarf planet’s largest moon, but the two bodies act more like a double planet because Charon’s so huge.

OK, it’s only 750 miles (1,212 km) in diameter, but that’s half as big as Pluto. Imagine if our moon was twice as big as it is now, and you get the picture.

Charon is large compared to Pluto, so the orbit about their common center of gravity located in the space between the two bodies. Credit: Wikipedia — Charon is large compared to Pluto, so they orbit about their common center of gravity located in the space between the two bodies. Credit: Wikipedia

As the duo dances an orbital duet about their common center of gravity, their variable gravitational field sends the smaller moons tumbling erratically. The effect is enhanced even more by their irregular and elongated shapes. It’s likely Pluto’s other two moons, Kerberos and Styx, are in a similar situation.

Because their moment to moment motions are essentially unpredictable, scientists describe their behavior is chaotic. Saturn’s moon, Hyperion, also tumbles chaotically.

Pluto (upper right) and its largest moon Charon form a "double planet" as seen in this photo taken by NASA's New Horizons probe which is set to make a close flyby of the Pluto system on July 14. Credit: NASA / NASA / Johns Hopkins University Applied Physics Laboratory / Southwest Research Institute — Pluto (upper right) and its largest moon Charon form a “double planet” as seen in this photo taken by NASA’s New Horizons probe which is set to make a close flyby of the Pluto system on July 14. Credit: NASA / NASA / Johns Hopkins University Applied Physics Laboratory / Southwest Research Institute

The discovery was made by Mark Showalter of the SETI Institute and Doug Hamilton of the University of Maryland using the Hubble Space Telescope and published in today’s issue of the journal Nature. Showalter also found three of Pluto’s moons are presently locked together in resonance, meaning there’s a precise ratio for their orbital periods.

“If you were sitting on Nix, you would see that Styx orbits Pluto twice for every three orbits made by Hydra,” said Hamilton.

That’s not all. If you’ve ever grilled with charcoal, you’d have a good idea what Kerberos looks like. Dark as one those briquettes. The other moons are as bright as sand because they’re mostly made of ice. Astronomers had thought that material blasted off the moons by meteorite impacts should make them all the same basic tone, so what’s up with Kerberos? No one knows.

This illustration shows the scale and comparative brightness of Pluto’s small satellites. The surface craters are for illustration only and are not real. Credits: NASA/ESA/A. Feild (STScI) — This illustration shows the scale and comparative brightness of Pluto’s small satellites. The surface craters are for illustration only and are not real.
Credits: NASA/ESA/A. Feild (STScI)

Pluto’s moons are thought to have formed during a collision long ago between the dwarf planet and a similar-sized object. The smash-up created lots of smaller bodies that eventually took up orbits about the present-day Pluto. Outside of Charon, the biggest leftover, the other moons measure in the tens of miles across. The four little ones — Nix, Styx, Kerberos and Hydra — were discovered with the Hubble scope during surveys to better map the Pluto system before New Horizons arrives next month. No one would be surprised if even more itty-bitty moons are found as we draw ever closer to the dwarf planet.

June 4, 2015December 23, 2015 by Nancy Graziano

Returning the “Silent Sentinel” to Active Duty

Situated on the south shore of New Jersey’s Shark River lies 37 acres of land known as Camp Evans. On April 1, 2015, I was privileged to attend the dedication ceremony celebrating Camp Evans’ becoming one of only 2532 locations in the United States designated as a National Historic Landmark.

Plaque Commemorating the Designation of Camp Evans as a National Historic Landmark. April 2, 2015. [photo: Robert Raia Photography] — Plaque Commemorating the Designation of Camp Evans as a National Historic Landmark. April 1, 2015. [photo: Robert Raia Photography]

Camp Evans, originally known as the Belmar Receiving Station, is rich in history:

In 1912, Gugliemlo Marconi and his company, the American Marconi Company, constructed the Belmar Receiving Station which became part of the wireless girdle of the earth.
In 1917, the site was acquired as part of the Navy’s World War I “Trans-Atlantic Communication System.”
In 1941, the Army Signal Corps purchased the property to construct a top-secret research facility, and it was renamed Evans Signal Laboratory which later became Camp Evans Signal Laboratory.
Following a visit in late October, 1953, Senator Joseph McCarthy described Camp Evans as a “house of spies.” Following an investigation that spanned 1953-1954, not one single employee was prosecuted.

But perhaps Camp Evans’ most interesting – and surprising – place in history begins with a small, informal research project taking place on a parcel of land in the Camp’s northeast corner. The ramifications of this project would ultimately give birth the to Space Age, lead to the development of the US Space Program, and start the Cold War.

Following the end of WWII, American scientists at Camp Evans continued their investigation into whether the earth’s ionosphere could be penetrated using radio waves – a feat that had been studied prior to the end of the War but had long been believed impossible. Project Diana, led by Lt. Col. John H. DeWitt, Jr., aimed to prove that it could indeed be penetrated. A group of radar scientists awaiting their discharge from the Army modified a radar antenna – including significantly boosting its output power – and placed it in the northeast corner of Camp Evans.

RADAR Dish at Camp Evans Circa 1946 — Location of the Radar Antenna on the Northeast Corner of Camp Evans Circa 1946. [photo: InfoAge website]

On the morning of January 10, 1946, with the dish pointed at the rising moon, a series of radar signals was broadcast. Exactly 2.5 seconds after each signal’s broadcast, its corresponding echo was detected. This was significant because 2.5 seconds is precisely the time required for light to travel the round trip distance between the earth and the moon. Project Diana – and her scientists – had successfully demonstrated that the ionosphere was, in fact, penetrable, and communication beyond our planet was possible. And thus was born the Space Age – as well as the field of Radar Astronomy.

SCR-271 Bedspring RADAR Antenna Pointing at the Moon [photo: David Mofenson; InfoAge website]

By mid-1958 the United States had launched the Television InfraRed Observation Satellite (TIROS) program designed to study the viability of using satellite imagery and observations as a means of studying the Earth and improving weather forecasting. As part of this effort, the original “Moonbounce” antenna was replaced with a 60-foot parabolic radio antenna dish which would serve as the project’s downlink Ground Communication Station.

60-Meter Parabolic Dish Being Constructed on Project Diana Site [photo: Frank Vosk; InfoAge website]

On April 1, 1960, NASA successfully launched its TIROS I satellite and the “Silent Sentinel Radio Dish” at Camp Evans began receiving its data being sent down to earth.

The resulting images were so astonishing and groundbreaking that the first photos received from TIROS I were immediately printed and flown to Washington where they were presented to President Eisenhower by NASA Administrator T. Keith Glennan.

President Eisenhower and NASA Administrator Glennan Viewing the First Satellite Images from TIROS I. [photo: wikimedia commons]

The TIROS program would go on to be instrumental in meteorological applications not only because it provided the first accurate weather forecasts and hurricane tracking based on satellite information, but also because it began providing continuous coverage of the earth’s weather in 1962, and ultimately lead to the development of more sophisticated observational satellites. ^[1]

In addition to serving as the downlink Ground Communications Center for the TIROS I and TIROS II satellites, this same dish has also tracked:

Explorer 1, America’s first satellite, in January, 1958 (pre-dates the launch of TIROS I), and
Pioneer V Space Probe.

Sadly, by the mid-1970s, the technology within the TIROS dish (officially named the TLM-18 Space Telemetry Antenna) had become obsolete, and it was retired. Camp Evans was decommissioned and closed in 1993 and its land was transferred to the National Park Service. But in 2012, Camp Evans was designated a National Historic Landmark, and thus began a new, revitalized era for this immensely significant site. In addition to the TIROS Dish and the InfoAge Science History Learning Center and Museum, Camp Evans is also home to:

The Military History Museum;
The Radio Technology Museum;
The National Broadcasters’ Hall of Fame.

The Apollo Guidance Computer, Just One of the Many Historical Exhibits on Display at the InfoAge Science History Learning Center and Museum at Historic Camp Evans [photo: Robert Raia Photography]

DISH RESTORATION

In 2001, InfoAge stepped in and began preserving and restoring the mechanical systems of the TIROS dish. In 2006, a donation from Harris Corporation allowed the dish to be completely repainted and preserved.

Norman Jarosik, Senior Research Physicist at Princeton University and Daniel Marlow, PhD. and Evans Crawford 1911 Professor of Physics at Princeton, as well as countless volunteers from the University, InfoAge, Wall Township (NJ), and the Ocean-Monmouth Amateur Radio Club, Inc. (OMARC) have provided the engineering/scientific knowledge and sweat-equity required to refurbish and update the inoperative radio dish. The original vacuum-tube technology has been replaced with smaller electronic counterparts. Rusty equipment has been replaced. Seized/inoperative motors have been reconditioned and rebuilt. And system-level software controls have been added. The TIROS dish has been transformed into a truly modern, state-of-the-art Radio Astronomy Satellite Dish and Control Center.

The TIROS Dish as it Appears Today [photo: Nancy J. Graziano]

On January 19, 2015, scientists from Princeton University pointed the dish skyward toward the center of our galaxy and detected a clear peak at 1420.4 MHz, the well-known 21 cm emission line originating from the deepest recesses of the Milky Way – the dish was working!

The Control Console Today. [photo: Nancy J. Graziano]

FUTURE PLANS

After almost 15 years of restoration and nearly 40 years since it last listened to the sky, the TIROS dish is once again operational, is detecting radio signals from the universe, and is well on its way to be used for science education.

Work continues on renovating Building 9162, the original TIROS Control Building, to convert it into the InfoAge Visitor Center. Plans include a NASA-style control room with theater seating for 20-30 students, a full-scale model of the original TIROS I satellite, and other exhibits dedicated to the history of Project Diana, the TIROS program, and the scientific impact these projects have had on our daily lives.

Artist’s Conception: Visitor Center Floorplan [credit: InfoAge]

Future activities being planned using the dish include a Moonbounce experiment, communicating with NOAA weather satellites, performing real-time satellite imaging, viewing the Milky Way in the radio spectrum, and tracking deep space pulsars.

If you are interested in visiting the InfoAge Science History Learning Center and Museum at Historic Camp Evans, they are open to the public on Wednesdays, Saturdays, and Sundays, from 1-5pm.

To learn more about Camp Evans, Project Diana, the TIROS Satellite project, and InfoAge, tune into this week’s Weekly Space Hangout. This week’s special guest is Stephen Fowler, the Creative Director at InfoAge. He will be chatting with Fraser about the history and plans for Camp Evans and the TIROS dish.

Still want to learn more? Click on any of the links provided in this article, or visit the following sites:

May 29, 2015December 23, 2015 by Ken Kremer

NASA’s Journey to Mars Ramps Up with InSight, Key Tests Pave Path to 2016 Lander Launch

NASA’s ‘Journey to Mars’ is ramping up significantly with ‘InSight’ – as the agency’s next Red Planet lander has now been assembled into its flight configuration and begun a comprehensive series of rigorous and critical environmental stress tests that will pave the path to launch in 2016 on a mission to unlock the riddles of the Martian core.

The countdown clock is ticking relentlessly and in less than nine months time, NASA’s InSight Mars lander is slated to blastoff in March 2016.

But before it will even be allowed to get to the launch pad, the Red Planet explorer must first prove its mettle and show that it can operate in and survive the harsh and unforgiving rigors of the space environment via a battery of prelaunch tests. That’s an absolute requirement in order for it to successfully carry out its unprecedented mission to investigate Mars deep interior structure.

InSight’s purpose is to elucidate the nature of the Martian core, measure heat flow and sense for “Marsquakes.” These completely new research findings will radically advance our understanding of the early history of all rocky planets, including Earth and could reveal how they formed and evolved.

“Today, our robotic scientific explorers are paving the way, making great progress on the journey to Mars,” said Jim Green, director of NASA’s Planetary Science Division at the agency’s headquarters in Washington, in a statement.

“Together, humans and robotics will pioneer Mars and the solar system.”

The science deck of NASA's InSight lander is being turned over in this April 29, 2015, photo from InSight assembly and testing operations inside a clean room at Lockheed Martin Space Systems, Denver. The large circular component on the deck is the protective covering to be placed over InSight's seismometer after the seismometer is placed directly onto the Martian ground. Credits: NASA/JPL-Caltech/Lockheed Martin — The science deck of NASA’s InSight lander is being turned over in this April 29, 2015, photo from InSight assembly and testing operations inside a clean room at Lockheed Martin Space Systems, Denver. The large circular component on the deck is the protective covering to be placed over InSight’s seismometer after the seismometer is placed directly onto the Martian ground. Credits: NASA/JPL-Caltech/Lockheed Martin

The launch window for InSight opens on March 4 and runs through March 30, 2016.

InSight will launch atop a United Launch Alliance (ULA) Atlas V rocket from Vandenberg Air Force Base, California.

InSight counts as NASA’s first ever interplanetary mission to launch from California.

The car sized probe will touch down near the Martian equator about six months later in the fall of 2016.

The prime contractor for InSight is Lockheed Martin Space Systems in Denver, Co and the engineering and technical team recently finished assembling the lander into its final configuration.

So now the time has begun to start the shakedown that literally involve “shaking and baking and zapping” the spacecraft to prove its ready and able to meet the March 2016 launch deadline.

During the next seven months of environmental testing at Lockheed’s Denver facility, “the lander will be exposed to extreme temperatures, vacuum conditions of nearly zero air pressure simulating interplanetary space, and a battery of other tests.”

“The assembly of InSight went very well and now it’s time to see how it performs,” said Stu Spath, InSight program manager at Lockheed Martin Space Systems, Denver, in a statement.

“The environmental testing regimen is designed to wring out any issues with the spacecraft so we can resolve them while it’s here on Earth. This phase takes nearly as long as assembly, but we want to make sure we deliver a vehicle to NASA that will perform as expected in extreme environments.”

The first test involves “a thermal vacuum test in the spacecraft’s “cruise” configuration, which will be used during its seven-month journey to Mars. In the cruise configuration, the lander is stowed inside an aeroshell capsule and the spacecraft’s cruise stage – for power, communications, course corrections and other functions on the way to Mars — is fastened to the capsule.”

After the vacuum test, InSight will be subjected to a series of tests simulating the vibrations of launch, separation and deployment shock, as well as checking for electronic interference between different parts of the spacecraft and compatibility testing.

Finally, a second thermal vacuum test will expose the probe “to the temperatures and atmospheric pressures it will experience as it operates on the Martian surface.”

The $425 million InSight mission is expected to operate for about two years on the Martian surface.

Artist rendition of NASA’s Mars InSight (Interior exploration using Seismic Investigations, Geodesy and Heat Transport) Lander. InSight is based on the proven Phoenix Mars spacecraft and lander design with state-of-the-art avionics from the Mars Reconnaissance Orbiter (MRO) and Gravity Recovery and Interior Laboratory (GRAIL) missions. Credit: JPL/NASA

InSight is an international science mission and a near duplicate of NASA’s successful Phoenix Mars landing spacecraft, Bruce Banerdt, InSight Principal Investigator of NASA’s Jet Propulsion Laboratory (JPL), Pasadena, California, told Universe Today.

“InSight is essentially built from scratch, but nearly build-to-print from the Phoenix design,” Banerdt, of NASA’s Jet Propulsion Laboratory (JPL) in Pasadena , Calif, told me. The team can keep costs down by re-using the blueprints pioneered by Phoenix instead of creating an entirely new spacecraft.

3 Footpads of Phoenix Mars Lander atop Martian Ice. NASA’s Mars InSight spacecraft design is based on the successful 2008 Phoenix lander. This mosaic shows Phoenix touchdown atop Martian ice. Phoenix thrusters blasted away Martian soil and exposed water ice. InSight carries instruments to peer deep into the Red Planet and investigate the nature and size of the mysterious Martian core. Credit: Ken Kremer/kenkremer.com/Marco Di Lorenzo/NASA/JPL/UA/Max Planck Institute

It is funded by NASA’s Discovery Program as well as several European national space agency’s and countries. Germany and France are providing InSight’s two main science instruments; HP3 and SEIS through the Deutsches Zentrum für Luft- und Raumfahrt. or German Aerospace Center (DLR) and the Centre National d’Etudes Spatiales (CNES).

“The seismometer (SEIS, stands for Seismic Experiment for Interior Structure) is from France (built by CNES and IPGP) and the heat flow probe (HP3, stands for Heat Flow and Physical Properties Probe) is from Germany (built by DLR),” Banerdt explained.

SEIS and HP3 are stationed on the lander deck. They will each be picked up and deployed by a robotic arm similar to that flown on Phoenix with some modifications.

Stay tuned here for Ken’s continuing Earth and planetary science and human spaceflight news.

Ken Kremer