ExoMars 2018 Rover Postponed to 2020 Launch

ESA Exomars rover launch has been rescheduled to launch two years later in 2020. Credit:ESA
ESA Exomars rover launch has been rescheduled to launch two years later in 2020.  Credit:ESA
ESA Exomars rover launch has been rescheduled to launch two years later in 2020. Credit:ESA

Liftoff of the ExoMars 2018 rover mission currently under development jointly by Europe and Russia has just been postponed for two years to 2020, according to an announcement today, May 2, from the European Space Agency (ESA) and the Russian space agency Roscosmos.

The delay was forced by a variety of technical and funding issues that ate up the schedule margin to enable a successful outcome for what will be Europe’s first Mars rover. The goal is to search for signs of life.

“Taking into account the delays in European and Russian industrial activities and deliveries of the scientific payload, a launch in 2020 would be the best solution,” ESA explained in a statement today.

The ambitious ExoMars rover is the second of two joint Euro-Russian missions to explore the Red Planet. It is equipped with an ESA deep driller and a NASA instrument to search for preserved organic molecules.

The first mission known as ExoMars 2016 was successfully launched last month from the Baikonur Cosmodrome in Kazakhstan atop a Russian Proton-M rocket on March 14.

The renamed ExoMars 2020 mission involves a European-led rover and a Russian-led surface platform and is also slated to blastoff on an Russian Proton rocket.

Roscosmos and ESA jointly decided to move the launch to the next available Mars launch window in July 2020. The costs associated with the delay are not known.

ExoMars 2016 lifted off on a Proton-M rocket from Baikonur, Kazakhstan at 09:31 GMT on 14 March 2016.   Copyright ESA–Stephane Corvaja, 2016
ExoMars 2016 lifted off on a Proton-M rocket from Baikonur, Kazakhstan at 09:31 GMT on 14 March 2016. Copyright ESA–Stephane Corvaja, 2016

The delay means that the Euro-Russian rover mission will launch the same year as NASA’s 2020 rover.

The rover is being built by prime contractor Airbus Defense and Space in Stevenage, England.

The descent module and surface science package are provided by Roscosmos with some contributions by ESA.

Recognizing the potential for a delay, ESA and Roscosmos set up a tiger team in late 2015 to assess the best options.

“Russian and European experts made their best efforts to meet the 2018 launch schedule for the mission, and in late 2015, a dedicated ESA-Roscosmos Tiger Team, also including Russian and European industries, initiated an analysis of all possible solutions to recover schedule delays and accommodate schedule contingencies,” said ESA in the statement.

The tiger team reported their results to ESA Director General Johann-Dietrich Woerner and Roscosmos Director General Igor Komarov.

Woerner and Komarov then “jointly decided to move the launch to the next available Mars launch window in July 2020, and tasked their project teams to develop, in cooperation with the industrial contactors, a new baseline schedule aiming towards a 2020 launch. Additional measures will also be taken to maintain close control over the activities on both sides up to launch.”

The ExoMars 2016 interplanetary mission is comprised of the Trace Gas Orbiter (TGO) and the Schiaparelli lander. The spacecraft are due to arrive at Mars in October 2016.

The ExoMars craft releases the Schiaparelli lander in October in this artist's view. Credit: ESA
The ExoMars craft releases the Schiaparelli lander in October in this artist’s view. Credit: ESA

The goal of TGO is to search for possible signatures of life in the form of trace amounts of atmospheric methane on the Red Planet.

The main purpose of Schiaparelli is to demonstrate key entry, descent, and landing technologies for the follow on 2nd ExoMars mission that will land the first European rover on the Red Planet.

The now planned 2020 ExoMars mission will deliver an advanced rover to the Red Planet’s surface. It is equipped with the first ever deep driller that can collect samples to depths of 2 meters (seven feet) where the environment is shielded from the harsh conditions on the surface – namely the constant bombardment of cosmic radiation and the presence of strong oxidants like perchlorates that can destroy organic molecules.

ExoMars was originally a joint NASA/ESA project.

But thanks to hefty cuts to NASA’s budget by Washington DC politicians, NASA was forced to terminate the agencies involvement after several years of extremely detailed work and withdraw from participation as a full partner in the exciting ExoMars missions.

NASA is still providing the critical MOMA science instrument that will search for organic molecules.

Thereafter Russia agreed to take NASA’s place and provide the much needed funding and rockets for the pair of launches in March 2016 and May 2018.

TGO will also help search for safe landing sites for the ExoMars 2020 lander and serve as the all important data communication relay station sending signals and science from the rover and surface science platform back to Earth.

ExoMars 2016 is Europe’s most advanced mission to Mars and joins Europe’s still operating Mars Express Orbiter (MEX), which arrived back in 2004, as well as a fleet of NASA and Indian probes.

The Trace Gas Orbiter (TGO) and Schiaparelli lander arrive at Mars on October 19, 2016.

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

Ken Kremer

Stunning Auroras From the Space Station in Ultra HD – Videos

Still image shows a stunning aurora captured from the International Space Station. This frame is from a compilation of ultra-high definition time-lapses of the aurora shot from the space station. Credit: NASA
Still image shows a stunning aurora captured from the International Space Station. This frame is from a compilation of ultra-high definition time-lapses of the aurora shot from the space station.  Credit: NASA
Still image shows a stunning aurora captured from the International Space Station. This frame is from a compilation of ultra-high definition time-lapses of the aurora shot from the space station. Credit: NASA

Stunning high definition views of Earth’s auroras and dancing lights as seen from space like never before have just been released by NASA in the form of ultra-high definition videos (4K) captured from the International Space Station (ISS).

Whether seen from the Earth or space, auroras are endlessly fascinating and appreciated by everyone young and old and from all walks of life.

The spectacular video compilation, shown below, was created from time-lapses shot from ultra-high definition cameras mounted at several locations on the ISS.

It includes HD view of both the Aurora Borealis and Aurora Australis phenomena seen over the northern and southern hemispheres.

The video begins with an incredible time lapse sequence of an astronaut cranking open the covers off the domed cupola – everyone’s favorite locale. Along the way it also shows views taken from inside the cupola.

The cupola also houses the robotics works station for capturing visiting vehicles like the recently arrived unmanned SpaceX Dragon and Orbital ATK Cygnus cargo freighters carrying science experiments and crew supplies.

The video was produced by Harmonic exclusively for NASA TV UHD;

Video caption: Ultra-high definition (4K) time-lapses of both the Aurora Borealis and Aurora Australis phenomena shot from the International Space Station (ISS). Credit: NASA

The video segue ways into multi hued auroral views including Russian Soyuz and Progress capsules, the stations spinning solar panels, truss and robotic arm, flying over Europe, North America, Africa, the Middle East, star fields, the setting sun and moon, and much more.

Auroral phenomena occur when electrically charged electrons and protons in the Earth’s magnetic field collide with neutral atoms in the upper atmosphere.

“The dancing lights of the aurora provide a spectacular show for those on the ground, but also capture the imaginations of scientists who study the aurora and the complex processes that create them,” as described by NASA.

Here’s another musical version to enjoy:

The ISS orbits some 250 miles (400 kilometers) overhead with a multinational crew of six astronauts and cosmonauts living and working aboard.

The current Expedition 47 crew is comprised of Jeff Williams and Tim Kopra of NASA, Tim Peake of ESA (European Space Agency) and cosmonauts Yuri Malenchenko, Alexey Ovchinin and Oleg Skripochka of Roscosmos.

Some of the imagery was shot by recent prior space station crew members.

Here is a recent aurora image taken by flight engineer Tim Peake of ESA as the ISS passed through on Feb. 23, 2016.

“The @Space_Station just passed straight through a thick green fog of #aurora…eerie but very beautiful,” Peake wrote on social media.

The @Space_Station just passed straight through a thick green fog of #aurora…eerie but very beautiful.  Credit: NASA/ESA/Tim Peake
The @Space_Station just passed straight through a thick green fog of #aurora…eerie but very beautiful. Credit: NASA/ESA/Tim Peake

A new room was just added to the ISS last weekend when the BEAM experimental expandable habitat was attached to a port on the Tranquility module using the robotic arm.

BEAM was carried to the ISS inside the unpressurized trunk section of the recently arrived SpaceX Dragon cargo ship.

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

Ken Kremer

See Historic Comet BA14 Up Close In These New Radar Images

These radar images of comet P/2016 BA14 were taken on March 23, 2016, by scientists using an antenna of NASA's Deep Space Network at Goldstone, California. At the time, the comet was about 2.2 million miles (3.5 million kilometers) from Earth. Credit: NASA/JPL-Caltech/GSSR
These radar images of comet P/2016 BA14 were taken on March 23, 2016, by scientists using an antenna of NASA's Deep Space Network at Goldstone, California. At the time, the comet was about 2.2 million miles (3.5 million kilometers) from Earth. Credit: NASA/JPL-Caltech/GSSR
These radar images of comet P/2016 BA14 were taken on March 23, 2016, by scientists using an antenna of NASA’s Deep Space Network at Goldstone, California. At the time, the comet was about 2.2 million miles (3.5 million kilometers) from Earth. Credit: NASA/JPL-Caltech/GSSR

On March 22, Comet P/2016 BA14 (Pan-STARRS) flew just 2.2 million miles (3.5 million kilometers) from Earth, making it the third closest comet ever recorded. The last time a comet appeared on our doorstep was in 1770, when Lexell’s Comet breezed by at about half that distance. Through a telescope, comet BA14 looked (and still looks) like a faint star, though time exposures reveal a short, weak tail. With an excellent map and large amateur telescope you might still find it making a bead across the Big Dipper and constellation Bootes tonight through the weekend.


Flyby Comet Imaged by Radar

While normal telescopes show few details, NASA’s Goldstone Solar System Radar in California’s Mojave Desert pinged P/2016 BA14 with radar over three nights during closest approach and created a series of crisp, detailed images from the returning echoes. They show a bigger comet than expected — about 3,000 feet (one kilometer) across —  and resolve features as small as 26 feet (8 meters) across.

“The radar images show that the comet has an irregular shape: looks like a brick on one side and a pear on the other,” said Shantanu Naidu, a researcher at NASA’s Jet Propulsion Laboratory. “We can see quite a few signatures related to topographic features such as large flat regions, small concavities and ridges on the surface of the nucleus.”

I honestly thought we’d see a more irregular shape assuming that astronomers were correct in thinking that BA14 broke off from its parent 252P/LINEAR though it’s possible it happened so long ago that the “damage” has been repaired by vaporizing ice softening its contours.

Comets are as dark as charcoal but appear light only because the sun illuminates them against the blackness of outer space. I shone a flashlight on a charcoal briquette (left) to simulate comet lighting. The same charcoal when viewed in normal light appears black. Credit: Bob King
Comets are as dark as charcoal but appear light only because the sun illuminates them against the blackness of outer space. I shone a flashlight on a charcoal briquette (left) to simulate comet lighting. The same charcoal when viewed in normal light appears black. Credit: Bob King

Radar also shows that the comet is rotating on its axis once every 35 to 40 hours. While radar eyes focused on BA14, Vishnu Reddy, of the Planetary Science Institute, Tucson, Arizona, used the NASA Infrared Telescope Facility (IRTF) on Mauna Kea, Hawaii to examine the comet in infrared light. He discovered its dark surface reflects less than 3% of the sunlight that falls on it. The infrared data is expected to yield clues of the comet’s composition as well.

Illustration of Comet 67P/C-G brought down to Earth in the city of Los Angeles, Calif. Compare to the same image (below) as viewed in space. Credit: ESA and anosmicovni
Illustration of Comet 67P/Churyumov-Gerasimenko brought down to Earth in the city of Los Angeles, Calif. Not only can we appreciate its size but also its truly dark surface.  Credit: ESA and anosmicovni

Comets are exceptionally dark objects often compared to the appearance of a fresh asphalt road or parking lot. They appear bright in photos because seen against the blackness of space, they’re still reflective enough to stand out. Comet 67P/Churyumov-Gerasimenko, still the apple of the orbiter Rosetta’s eye, is similarly dark, reflecting about 4% of sunlight.

What makes comets so dark even though they composed primarily of ice? Astronomers believe a comet grows a dark ‘skin’ both from accumulated dust and irradiation of its pristine ices by cosmic rays. Cosmic rays loosen oxygen atoms from water ice, freeing them to combine with simple carbon molecules present on comets to form larger, more complex and darker compounds resembling tars and crude oil. Dust settles on a comet’s surface after it’s set free from ice that vaporizes in sunlight.

Comet 67P/C-G photographed from a distance of just 7.5 miles (12 kilometers) on March 19, 2016 by Rosetta's Navcam. Credit: ESA/Rosetta/NAVCAM – CC BY-SA IGO 3.0.
What a view! Comet 67P/C-G photographed from a distance of just 7.5 miles (12 kilometers) on March 19, 2016 by Rosetta’s Navcam. The largest boulder to the right is Cheops, which stands about 82 feet (25 meters) high. Credit: ESA/Rosetta/NAVCAM – CC BY-SA IGO 3.0

I live in Minnesota, where our annual State Fair features every kind of deep-fried food you can imagine: deep-fried Twinkies, deep-fried fruit, deep-fried bacon and even deep-fried Smores. Just now, I can’t shake the thought that comets are just another deep-fried confection made of pristine, 4.5-billion-year-old ice toasted by eons of sunlight and cosmic bombardment.

ExoMars Mission Narrowly Avoids Exploding Booster

The ExoMars craft releases the Schiaparelli lander in October in this artist's view. Credit: ESA
At least nine moving objects, all thought to be related to a possible explosion of the Breeze-M upper stage after separation from the ExoMars spacecraft, move across the sky in this animation. ExoMars is further ahead and outside the frame. Credit and copyright: OASI Observatory team; D. Lazzaro, S. Silva / ESA
At least nine moving objects, all thought to be related to a possible explosion of the Breeze-M upper stage after separation from the ExoMars spacecraft, move across the sky in this animation made late on March 14. ExoMars is further ahead and outside the frame. Credit and copyright: OASI Observatory team; D. Lazzaro, S. Silva / ESA

On March 14, the ExoMars mission successfully lifted off on a 7-month journey to the planet Mars but not without a little surprise. The Breeze-M upper booster stage, designed to give the craft its final kick toward Mars, exploded shortly after parting from the probe. Thankfully, it wasn’t close enough to damage the spacecraft.

Michel Denis, ExoMars flight director at the European Space Operations, Center in Darmstadt, Germany, said that the two craft were many kilometers apart at the time of the breakup, so the explosion wouldn’t have posed a risk. Still, the mission team won’t be 100% certain until all the science instruments are completely checked over in the coming weeks.

All went well during the takeoff and final separation of the probe, but then something odd happened. Breeze-M was supposed to separate cleanly into two pieces — the main body and a detachable fuel tank — and maneuver itself to a graveyard or “junk” orbit, where rockets and spacecraft are placed at the end of their useful lives, so they don’t cause trouble with operational satellites.

But instead of two pieces, tracking photos taken at the OASI Observatory in Brazil not long after the stage and probe separated show  a cloud of debris, suggesting an explosion occurred that shattered the booster to pieces. There’s more to consider. Space probes intended to either land or be crashed into planets have to pass through strict sterilization procedures that rocket boosters aren’t subject to. Assuming the Breeze-M shrapnel didn’t make it to its graveyard orbit, there exists the possibility some of it might be heading for Mars. If any earthly bugs inhabit the remains, it could potentially lead to unwanted consequences on Mars.

And this isn’t the first time a Russian Breeze-M has blown up.

According to Russian space observer Anatoly Zak in a recent article in Popular Mechanics, a Breeze-M that delivered a Russian spy satellite into orbit last December exploded on January 16. Propellant in one of its fuel tanks may not have been properly vented into space; heated by the sun, the tank’s contents likely combusted and ripped the stage apart. A similar incident occurred in October 2012.

The ExoMars craft releases the Schiaparelli lander in October in this artist's view. Credit: ESA
Artist view of the ExoMars craft releasing the Schiaparelli lander in October. Credit: ESA

For now, we’ll embrace the good news that the spacecraft, which houses the Trace Gas Orbiter (TGO) and the Schiaparelli lander, are underway to Mars and in good health.

ExoMars is a joint venture between the European Space Agency (ESA) and the Russian Federal Space Agency (Roscosmos). One of the mission’s key goals is to follow up on the methane detection made by ESA’s Mars Express probe in 2004 to understand where the gas comes from. Mars’ atmosphere is 95% carbon dioxide with the remaining 5% divided among nitrogen, argon, oxygen and others including small amounts of methane, a gas that on Earth is produced largely by living creatures.

NASA researchers using telescopes right here on Earth also detected multiple methane plumes coming from the surface on Mars in 2003. Credit: Trent Schindler/NASA
NASA researchers using telescopes right here on Earth also detected multiple methane plumes coming from the surface on Mars in 2003. Credit: Trent Schindler/NASA

Scientists want to know how martian methane got into the atmosphere. Was it produced by biology or geology? Methane, unless it is continuously produced by a source, only survives in the Martian atmosphere for a few hundreds of years because it quickly breaks down to form water and carbon dioxide. Something is refilling the atmosphere with methane but what?

TGO will also look at potential sources of other trace gases such as volcanoes and map the planet’s surface. It can also detect buried water-ice deposits, which, along with locations identified as sources of the trace gases, could influence the choice of landing sites of future missions.

The orbiter will also act as a data relay for the second ExoMars mission — a rover and stationary surface science platform scheduled for launch in May 2018 and arriving in early 2019.

Schiaparelli will demonstrate the capability of ESA and European industry to perform a controlled landing on the surface of Mars. Credit: ESA
Schiaparelli will demonstrate the capability of ESA and European industry to perform a controlled landing on the surface of Mars. It will also gather data on Mars’ atmosphere. Credit: ESA

On October 16, when the spacecraft is still 559,000 miles (900,000 kilometers) from the Red Planet, the Schiaparelli lander will separate from the orbiter and three days later parachute down to the Martian surface. The orbiter will take measurements of the planet’s atmosphere (including methane) as well as any atmospheric electrical fields.

Clouds gather over Mars' Hellas Basin in this photo taken March 23. The Red Planet has intrigued humankind for centuries. Credit: Anthony Wesley
Clouds gather over Mars’ Hellas Basin in this photo taken March 23. The Red Planet has intrigued humankind for centuries. Credit: Anthony Wesley

Mars is a popular place. There are currently five active orbiters there: two European (Mars Express and Mars Odyssey), two American (Mars Reconnaissance Orbiter and MAVEN), one Indian (Mars Orbiter Mission) and two rovers (Opportunity and Curiosity) with another lander and orbiter en route!

Bold Euro-Russian Expedition Blasts Free of Earth En Route to Mars in Search of Life’s Indicators

Artists concept of ExoMars spacecraft separation from Breeze M fourth stage. Credit: ESA
Artists concept of ExoMars spacecraft separation from Breeze M fourth stage. Credit: ESA
Artists concept of ExoMars spacecraft separation from Breeze M fourth stage after launch atop Proton rocket on March 14, 2016. Credit: ESA

The cooperative Euro-Russian ExoMars 2016 expedition is now en route to the Red Planet after successfully firing its upper stage booster one final time on Monday evening, March 15, to blast free of the Earth’s gravitational tug and begin a 500 million kilometer interplanetary journey in a bold search of indications of life emanating from potential Martian microbes.

The vehicle is in “good health” with the solar panels unfurled, generating power and on course for the 500 Million kilometer (300 million mile) journey to Mars.

“Acquisition of signal confirmed. We have a mission to Mars!” announced Mission Control from the European Space Agency.

The joint European/Russian ExoMars spacecraft successfully blasted off from the Baikonur Cosmodrome in Kazakhstan atop a Russian Proton-M rocket at 5:31:42 a.m. EDT (0931:42 GMT), Monday, March 14, with the goal of searching for possible signatures of life in the form of trace amounts of atmospheric methane on the Red Planet.

Video caption: Blastoff of Russian Proton rocket from the Baikonur Cosmodrome carrying ExoMars 2016 mission on March 14, 2016. Credit: Roscosmos

The first three stages of the 191-foot-tall (58-meter) Russian-built rocket fired as scheduled over the first ten minutes and lofted the 9,550-pound (4,332-kilogram) ExoMars to orbit.

Three more firings from the Breeze-M fourth stage quickly raised the probe into progressively higher temporary parking orbits around Earth.

But the science and engineering teams from the European Space Agency (ESA) and Roscosmos had to keep their fingers crossed and endure an agonizingly long wait of more than 10 hours before the fourth and final ignition of the Proton’s Breeze-M upper stage required to break the bonds of Earth.

The do or die last Breeze-M upper stage burn with ExoMars still attached was finally fired exactly as planned.

The probe was released at last from the Breeze at 20:13 GMT.

However, it took another long hour to corroborate the missions true success until the first acquisition of signal (AOS) from the spacecraft was received at ESA’s control centre in Darmstadt, Germany via the Malindi ground tracking station in Africa at 5:21:29 p.m. EST (21:29 GMT), confirming a fully successful launch with the spacecraft in good health.

It was propelled outwards to begin a seven-month-long journey to the Red Planet to the great relief of everyone involved from ESA, Roscosmos and other nations participating. An upper stage failure caused the total loss of Russia’s prior mission to Mars; Phobos-Grunt.

“Only the process of collaboration produces the best technical solutions for great research results. Roscosmos and ESA are confident of the mission’s success,” said Igor Komarov, General Director of the Roscosmos State Space Corporation, in a statement.

The ExoMars 2016 mission is comprised of a joined pair of European-built spacecraft consisting of the Trace Gas Orbiter (TGO) plus the Schiaparelli entry, descent and landing demonstrator module, built and funded by ESA.

“It’s been a long journey getting the first ExoMars mission to the launch pad, but thanks to the hard work and dedication of our international teams, a new era of Mars exploration is now within our reach,” says Johann-Dietrich Woerner, ESA’s Director General.

“I am grateful to our Russian partner, who have given this mission the best possible start today. Now we will explore Mars together.”

ExoMars 2016 Mission to the Red Planet.  It consists of two spacecraft -  the Trace Gas Orbiter (TGO) and the Entry, Descent and Landing Demonstrator Module (EDM) which will land.  Credit: ESA
ExoMars 2016 Mission to the Red Planet. It consists of two spacecraft – the Trace Gas Orbiter (TGO) and the Entry, Descent and Landing Demonstrator Module (EDM) which will land. Credit: ESA

The cooperative mission includes significant participation from the Russian space agency Roscosmos who provided the Proton-M launcher, part of the science instrument package, the surface platform and ground station support.

The Trace Gas Orbiter (TGO) and Schiaparelli lander are speeding towards Mars joined together, on a collision course for the Red Planet. They will separate on October 16, 2016 at distance of 900,000 km from the planet, three days before arriving on October 19, 2016.
TGO will fire thrusters to alter course and enter an initial four-day elliptical orbit around the fourth planet from the sun ranging from 300 km at its perigee to 96 000 km at its apogee, or furthest point.

Over the next year, engineers will command TGO to fire thrusters and conduct a complex series of ‘aerobraking’ manoeuvres that will gradually lower the spacecraft to circular 400 km (250 mi) orbit above the surface.

The science mission to analyse for rare gases, including methane, in the thin Martian atmosphere at the nominal orbit is expected to begin in December 2017.

ExoMars 2016: Trace Gas Orbiter and Schiaparelli. Credit:  ESA/ATG medialab
ExoMars 2016: Trace Gas Orbiter and Schiaparelli. Credit:
ESA/ATG medialab

As TGO enters orbit, the Schiaparelli lander will smash into the atmosphere and begin a harrowing six minute descent to the surface.

The main purpose of Schiaparelli is to demonstrate key entry, descent, and landing technologies for the follow on 2nd ExoMars mission in 2018 that will land the first European rover on the Red Planet.

The battery powered lander is expected to operate for perhaps four and up to eight days until the battery is depleted.

It will conduct a number of environmental science studies such as “obtaining the first measurements of electric fields on the surface of Mars that, combined with measurements of the concentration of atmospheric dust, will provide new insights into the role of electric forces on dust lifting – the trigger for dust storms,” according to ESA.

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

Ken Kremer

ExoMars Spacecraft Launches to Red Planet Searching for Signs of Life

ExoMars 2016 lifted off on a Proton-M rocket from Baikonur, Kazakhstan at 09:31 GMT on 14 March 2016. Copyright ESA–Stephane Corvaja, 2016
ExoMars 2016 lifted off on a Proton-M rocket from Baikonur, Kazakhstan at 09:31 GMT on 14 March 2016.   Copyright ESA–Stephane Corvaja, 2016
ExoMars 2016 lifted off on a Proton-M rocket from Baikonur, Kazakhstan at 09:31 GMT on 14 March 2016. Copyright ESA–Stephane Corvaja, 2016

The joint European/Russian ExoMars spacecraft successfully launched early this morning from the Baikonur Cosmodrome in Kazakhstan atop a Proton-M rocket at 5:31:42 a.m. EDT (0931:42 GMT), Monday, March 14, with the goal of searching for signs of life on the Red Planet.

After settling into orbit around Mars, it’s instruments will scan for minute signatures of methane gas that could possibly be an indication of life or of nonbiologic geologic processes ongoing today.

The spacecraft is currently circling in a temporary and preliminary parking orbit around Earth following liftoff of the 191-foot-tall (58-meter) Russian-built rocket under overcast skies – awaiting a critical final engine burn placing the probe on an interplanetary trajectory to Mars.

The 9,550-pound (4,332-kilogram) ExoMars 2016 spacecraft continued soaring to orbit after nominal firings of the Proton’s second and third stages and jettisoning of the payload fairing halves protecting the vehicle during ascent through Earth’s atmosphere.

A total of four more burns from the Breeze-M upper stage are required to boost ExoMars higher and propel it outwards on its seven-month-long journey to the Red Planet.

So the excitement and nail biting is not over yet and continues to this moment. The final successful outcome of today’s mission cannot be declared until more than 10 hours after liftoff – after the last firing of the Breeze-M upper stage sets the probe on course for Mars and escaping the tug of Earth’s gravity.

ExoMars 2016 lifted off on a Proton-M rocket from Baikonur, Kazakhstan at 09:31 GMT on 14 March 2016.   Copyright ESA–Stephane Corvaja, 2016
ExoMars 2016 lifted off on a Proton-M rocket from Baikonur, Kazakhstan at 09:31 GMT on 14 March 2016. Copyright ESA–Stephane Corvaja, 2016

The first three Breeze-M fourth stage burns have now been completed as of about 9:40 am EST, according to ESA mission control on Darmstadt, Germany.

The fourth and final ignition of the Breeze-M upper stage and spacecraft separation is slated for after 3 p.m. EDT today, March 14, 2016.

The first acquisition of signal from the spacecraft is expected later at about 5:21:29 p.m. EST (21:29 GMT).

Artists concept of ExoMars spacecraft separation from Breeze fourth stage. Credit: ESA
Artists concept of ExoMars spacecraft separation from Breeze fourth stage. Credit: ESA

The ExoMars 2016 mission is comprised of a joined pair of European-built spacecraft consisting of the Trace Gas Orbiter (TGO) plus the Schiaparelli entry, descent and landing demonstrator module, built and funded by the European Space Agency (ESA).

The cooperative mission includes significant participation from the Russian space agency Roscosmos who provided the Proton-M launcher, part of the science instrument package, the surface platform and ground station support.

The launch was carried live courtesy of a European Space Agency (ESA) webcast:

http://www.esa.int/Our_Activities/Space_Science/ExoMars/Watch_ExoMars_launch

ESA is continuing live streaming of the launch events throughout the day as burns continue and events unfold lead up to the critical final burn of the Breeze-M upper stage

The ExoMars 2016 TGO orbiter is equipped with a payload of four science instruments supplied by European and Russian scientists. It will investigate the source and precisely measure the quantity of the methane and other trace gases, present at levels of one percent or far less.

On Earth methane can be produced by biology, volcanoes, natural gas and hydrothermal activity. TGO will investigate what makes it on Mars and follow up on measurements from NASA’s Curiosity rover and other space based assets and telescopes.

Martian methane has a lifetime of about 400 years, until it is destroyed by solar UV & mixed by atmosphere, says Jorge Vago, ESA ExoMars 2016 principal scientist.

The 2016 lander will carry an international suite of science instruments and test European entry, descent and landing (EDL) technologies for the 2nd ExoMars mission in 2018.

The battery powered lander is expected to operate for perhaps four and up to eight days until the battery is depleted.

The 2018 ExoMars mission will deliver an advanced rover to the Red Planet’s surface.

It is equipped with the first ever deep driller that can collect samples to depths of 2 meters (seven feet) where the environment is shielded from the harsh conditions on the surface – namely the constant bombardment of cosmic radiation and the presence of strong oxidants like perchlorates that can destroy organic molecules.

ExoMars was originally a joint NASA/ESA project.

But thanks to hefty cuts to NASA’s budget by Washington DC politicians, NASA was forced to terminate the agencies involvement after several years of extremely detailed work and withdraw from participation as a full partner in the exciting ExoMars missions.

NASA is still providing the critical MOMA science instrument that will search for organic molecules.

Thereafter Russia agreed to take NASA’s place and provide the much needed funding and rockets for the pair of launches in March 2016 and May 2018.

TGO will also help search for safe landing sites for the ExoMars 2018 lander and serve as the all important data communication relay station sending signals and science from the rover and surface science platform back to Earth.

ExoMars 2016 is Europe’s most advanced mission to Mars and joins Europe’s still operating Mars Express Orbiter (MEX), which arrived back in 2004, as well as a fleet of NASA and Indian probes.

ExoMars 2016: Trace Gas Orbiter and Schiaparelli. Credit:  ESA/ATG medialab
ExoMars 2016: Trace Gas Orbiter and Schiaparelli. Credit:
ESA/ATG medialab

The Trace Gas Orbiter (TGO) and Schiaparelli lander arrive at Mars on October 19, 2016.

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

Ken Kremer

Proton rocket and ExoMars 2016 spacecraft stand vertical at the launch pad at the Baikonur cosmodrome, Kazakhstan Copyright: ESA - B. Bethge
Proton rocket and ExoMars 2016 spacecraft stand vertical at the launch pad at the Baikonur cosmodrome, Kazakhstan
Copyright: ESA – B. Bethge

Countdown Begins for Blastoff of ExoMars 2016 Spacecraft on March 14 – Watch Live

Proton rocket and ExoMars 2016 spacecraft rolled out to launch pad at the Baikonur cosmodrome, Kazakhstan Copyright: ESA - B. Bethge
Proton rocket and ExoMars 2016 spacecraft rolled out to launch pad at the Baikonur cosmodrome, Kazakhstan Copyright: ESA - B. Bethge
Proton rocket and ExoMars 2016 spacecraft rolled out to launch pad at the Baikonur cosmodrome, Kazakhstan
Copyright: ESA – B. Bethge

The countdown has begun for blastoff of the ambitious European/Russian ExoMars 2016 spacecraft from the Baikonur Cosmodrome in Kazakhstan on March 14. Its goal is to search for minute signatures of methane gas that could possibly be an indication of life or of nonbiologic geologic processes ongoing today.

Final launch preparations are now in progress. Liftoff of the powerful Russian Proton booster from Baikonur carrying the ExoMars spacecraft is slated for 5:31:42 a.m. EDT (0931:42 GMT), Monday morning, March 14.

You can watch the launch live courtesy of a European Space Agency (ESA) webcast:

http://www.esa.int/Our_Activities/Space_Science/ExoMars/Watch_ExoMars_launch

The prelaunch play by play begins with live streaming at 4:30 a.m. EDT (08:30 GMT).

The first acquisition of signal from the spacecrft is expected at 21:29 GMT

As launch and post launch events unfold leading to spacecraft separation, ESA plans additional live streaming events at 7:00 a.m. EDT (11:00 GMT) and 5:10 p.m. (21:10 GMT)

Spacecraft separation from the Breeze upper stage is expected at about 10 hours, 41 minutes.

Artists concept of ExoMars spacecraft separation from Breeze fourth stage. Credit: ESA
Artists concept of ExoMars spacecraft separation from Breeze fourth stage. Credit: ESA

The ExoMars 2016 mission is comprised of a pair of European spacecraft named the Trace Gas Orbiter (TGO) and the Schiaparelli entry, descent and landing demonstration lander, built and funded by the European Space Agency (ESA).

Russian is providing the Proton booster and part of the science instrument package.

“The main objectives of this mission are to search for evidence of methane and other trace atmospheric gases that could be signatures of active biological or geological processes and to test key technologies in preparation for ESA’s contribution to subsequent missions to Mars,” says ESA.

Proton rocket and ExoMars 2016 spacecraft stand vertical at the launch pad at the Baikonur cosmodrome, Kazakhstan Copyright: ESA - B. Bethge
Proton rocket and ExoMars 2016 spacecraft stand vertical at the launch pad at the Baikonur cosmodrome, Kazakhstan
Copyright: ESA – B. Bethge

ExoMars is Earth’s lone mission to the Red Planet following the two year postponement of NASA’s InSight lander from 2016 to 2018 to allow time to fix a defective French-built seismometer.

ESA reported late today , March 13, that at T-minus 12 hours the Trace Gas Orbiter has been successfully switch on, a telemetry link was established and the spacecrft battery charging has been completed.

The Proton rocket with the encapsulated spacecraft bolted atop were rolled out to the Baikonur launch pad on Friday, March 11 and the launcher was raised into the vertical position.

ESA mission controller then completed a full launch dress rehearsal on Saturday, March 12.

The ExoMars 2016 TGO orbiter is equipped with a payload of four science instruments supplied by European and Russian scientists. It will investigate the source and precisely measure the quantity of the methane and other trace gases.

The ExoMars 2016 spacecraft composite, comprised of the Trace Gas Orbiter and Schiaparelli, seen during the encapsulation within the launcher fairing  at the Baikonur cosmodrome in Kazakhstan. Launch to Mars is slated for March 14, 2016.  Copyright: ESA - B. Bethge
The ExoMars 2016 spacecraft composite, comprised of the Trace Gas Orbiter and Schiaparelli, seen during the encapsulation within the launcher fairing at the Baikonur cosmodrome in Kazakhstan. Launch to Mars is slated for March 14, 2016. Copyright: ESA – B. Bethge

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

Ken Kremer

ExoMars 2016 Spacecraft Encapsulated for Red Planet Launch in One Week

The ExoMars 2016 spacecraft composite, comprised of the Trace Gas Orbiter and Schiaparelli, seen during the encapsulation within the launcher fairing at the Baikonur cosmodrome in Kazakhstan. Launch to Mars is slated for March 14, 2016. Copyright: ESA - B. Bethge
The ExoMars 2016 spacecraft composite, comprised of the Trace Gas Orbiter and Schiaparelli, seen during the encapsulation within the launcher fairing  at the Baikonur cosmodrome in Kazakhstan. Launch to Mars is slated for March 14, 2016.  Copyright: ESA - B. Bethge
The ExoMars 2016 spacecraft composite, comprised of the Trace Gas Orbiter and Schiaparelli, seen during the encapsulation within the launcher fairing at the Baikonur cosmodrome in Kazakhstan. Launch to Mars is slated for March 14, 2016. Copyright: ESA – B. Bethge

Final launch preparations are now in full swing for the ambitious European/Russian ExoMars 2016 spacecraft which has been encapsulated inside its payload launcher fairing and is slated to blast off for the Red Planet one week from now on March 14, 2016 from Kazakhstan.

On March 2, technicians working at the Baikonur Cosmodrome in Kazakhstan completed the complex multiday mating and enclosure operations of the composite ExoMars 2016 spacecraft to the launch vehicle adapter and the Breeze upper stage inside the nose cone.

The ExoMars 2016 mission is comprised of a pair of European spacecraft named the Trace Gas Orbiter (TGO) and the Schiaparelli lander, built and funded by the European Space Agency (ESA).

“The main objectives of this mission are to search for evidence of methane and other trace atmospheric gases that could be signatures of active biological or geological processes and to test key technologies in preparation for ESA’s contribution to subsequent missions to Mars,” says ESA.

2016’s lone mission to the Red Planet will launch atop a Russian Proton rocket.

The individual orbiter and lander spacecraft were recently mated at Baikonur on February 12.

To prepare for the encapsulation, engineers first tilted the spacecraft horizontally. Then they rolled the first fairing half underneath the spacecraft and Breeze on a track inside the Baikonur cleanroom.

Then they used an overhead crane to carefully lower the second fairing half and maneuver it into place from above to fully encapsulate the precious payload.

Tilting the ExoMars 2016 spacecraft and Breeze upper stage into the horizontal position in preparation of encapsulation within the launcher fairing at the Baikonur cosmodrome in Kazakhstan. Launch to Mars is slated for March 14, 2016.  Copyright: ESA - B. Bethge
Tilting the ExoMars 2016 spacecraft and Breeze upper stage into the horizontal position in preparation of encapsulation within the launcher fairing at the Baikonur cosmodrome in Kazakhstan. Launch to Mars is slated for March 14, 2016. Copyright: ESA – B. Bethge

The 13.5 foot (4.1-meter) diameter payload fairing holding the ExoMars 2016 spacecraft and Breeze upper stage will next be mated to the Proton rocket and rolled out to the Baikonur launch pad.

The launch window extends until March 25.

The ExoMars 2016 TGO orbiter is equipped with a payload of four science instruments supplied by European and Russian scientists. It will investigate the source and precisely measure the quantity of the methane and other trace gases.

ExoMars 2016 Mission to the Red Planet.  It consists of two spacecraft -  the Trace Gas Orbiter (TGO) and the Entry, Descent and Landing Demonstrator Module (EDM) which will land.  Credit: ESA
ExoMars 2016 Mission to the Red Planet. It consists of two spacecraft – the Trace Gas Orbiter (TGO) and the Entry, Descent and Landing Demonstrator Module (EDM) which will land. Credit: ESA

The 2016 lander will carry an international suite of science instruments and test European entry, descent and landing (EDL) technologies for the 2nd ExoMars mission in 2018.

The battery powered lander is expected to operate for up to eight days.

The 2018 ExoMars mission will deliver an advanced rover to the Red Planet’s surface.

It is equipped with the first ever deep driller that can collect samples to depths of 2 meters where the environment is shielded from the harsh conditions on the surface – namely the constant bombardment of cosmic radiation and the presence of strong oxidants like perchlorates that can destroy organic molecules.

ExoMars was originally a joint NASA/ESA project.

But thanks to hefty cuts to NASA’s budget by Washington DC politicians, NASA was forced to terminate the agencies involvement after several years of extremely detailed work and withdraw from participation as a full partner in the exciting ExoMars missions.

Thereafter Russia agreed to take NASA’s place and provide the much needed funding and rockets for the pair of launches in March 2016 and May 2018.

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

Ken Kremer

ESA Planning To Build An International Village… On The Moon!

Chris Hadfield recently explained how humanity should create a Moon base before attempting to colonize Mars. Credit: Foster + Partners is part of a consortium set up by the European Space Agency to explore the possibilities of 3D printing to construct lunar habitations. Credit: ESA/Foster + Partners

With all the talk about manned missions to Mars by the 2030s, its easy to overlook another major proposal for the next great leap. In recent years, the European Space Agency has been quite vocal about its plan to go back to the Moon by the 2020s. More importantly, they have spoken often about their plans to construct a moon base, one which would serve as a staging platform for future missions to Mars and beyond.

These plans were detailed at a recent international symposium that took place on Dec. 15th at the the European Space Research and Technology Center in Noordwijk, Netherlands. During the symposium, which was titled “Moon 2020-2030 – A New Era of Coordinated Human and Robotic Exploration”, the new Director General of the ESA – Jan Woerner – articulated his agency’s vision.

The purpose of the symposium – which saw 200 scientists and experts coming together to discuss plans and missions for the next decade – was to outline common goals for lunar exploration, and draft methods on how these can be achieved cooperatively. Intrinsic to this was the International Space Exploration Coordinated Group‘s (ISECG) Global Exploration Roadmap, an agenda for space exploration that was drafted by the group’s 14 members – which includes NASA, the ESA, Roscosmos, and other federal agencies.

The ISECG is an international group of space agencies dedicated to common exploration goals. Credit: globalspaceexploration.org
The ISECG is an international group of space agencies dedicated to common exploration goals. Credit: globalspaceexploration.org

This roadmap not only lays out the strategic significance of the Moon as a global space exploration endeavor, but also calls for a shared international vision on how to go about exploring the Moon and using it as a stepping stone for future goals. When it came time to discuss how the ESA might contribute to this shared vision, Woerner outlined his agency’s plan to establish an international lunar base.

In the past, Woerner has expressed his interest in a base on the Moon that would act as a sort of successor to the International Space Station. Looking ahead, he envisions how an international community would live and perform research in this environment, which would be constructed using robotic workers, 3D printing techniques, and in-situ resources utilization.

The construction of such a base would also offer opportunities to leverage new technologies and forge lucrative partnerships between federal space agencies and private companies. Already, the ESA has collaborated with the architectural design firm Foster + Partners to come up with the plan for their lunar village, and other private companies have also been recruited to help investigate other aspects of building it.

Going forward, the plan calls for a series of manned missions to the Moon beginning in the 2020s, which would involve robot workers paving the way for human explorers to land later. These robots would likely be controlled through telepresence, and would combine lunar regolith with magnesium oxide and a binding salt to print out the shield walls of the habitat.

The ESAs plan for establishing a base on the Moon. Credit: spaceflight.esa.int
The ESAs plan for establishing a base on the Moon, which would rely on robotic workers and human astronauts. Credit: spaceflight.esa.int

At present, the plan is for the base to be built in southern polar region, which exists in a near-state of perpetual twilight. Whether or not this will serve as a suitable location will be the subject of the upcoming Lunar Polar Sample Return mission – a joint effort between the ESA and Roscosmos that will involve sending a robotic probe to the Moon’s South Pole-Aitken Basin by 2020 to retrieve samples of ice.

This mission follows in the footsteps of NASA’s Lunar Reconnaissance Orbiter (LRO), which showed that the Shakleton crater – located in the Moon’s southern polar region – has an abundant supply of water ice. This could not only be used to provide the Moon base with a source of drinking water, but could also be converted into hydrogen to refuel spacecraft on their way to and from Earth.

As Woerner was quoted as saying by the Daily Mail during the course of the symposium, this lunar base would provide the opportunity for scientists from many different nations to live and work together:

The future of space travel needs a new vision. Right now we have the Space Station as a common international project, but it won’t last forever. If I say Moon Village, it does not mean single houses, a church, a town hall and so on… My idea only deals with the core of the concept of a village: people working and living together in the same place. And this place would be on the Moon. In the Moon Village we would like to combine the capabilities of different spacefaring nations, with the help of robots and astronauts. The participants can work in different fields, perhaps they will conduct pure science and perhaps there will even be business ventures like mining or tourism.

Naturally, the benefits would go beyond scientific research and international cooperation. As NexGen Space LLC (a consultant company for NASA) recently stated, such a base would be a major stepping stone on the way to Mars. In fact, the company estimated that if such a base included refueling stations, it could cut the cost of any future Mars missions by about $10 billion a year.

And of course, a lunar base would also yield valuable scientific data that would come in handy for future missions. Located far from Earth’s protective magnetic field, astronauts on the Moon (and in circumpolar obit) would be subjected to levels of cosmic radiation that astronauts in orbit around Earth (i.e. aboard the ISS) are not. This data will prove immeasurably useful when plotting upcoming missions to Mars or into deep space.

An additional benefit is the possibility of creating an international presence on the Moon that would ensure that the spirit of the Outer Space Treaty endures. Signed back in 1966 at the height of the “Moon Race”, this treaty stated that “the exploration and use of outer space shall be carried out for the benefit and in the interests of all countries and shall be the province of all mankind.”

In other words, the treaty was meant to ensure that no nation or space agency could claim anything in space, and that issues of territorial sovereignty would not extend to the celestial sphere. But with multiple agencies discussing plans to build bases on the Moon – including NASA, Roscosmos, and JAXA – it is possible that issues of “Moon sovereignty” might emerge at some point in the future.

And having a base that could facilitate regular trips to the Moon would also be a boon for the burgeoning space tourism industry. Beyond offering trips into Low Earth Orbit (LEO) aboard Virgin Galactic, Richard Branson has also talked about the possibility of offering trips to the Moon by 2043. Golden Spike, another space tourism company, also hopes to offer round-trip lunar adventures someday (at a reported $750 million a pop).

Other private space ventures that are looking to make the Moon a tourist destination include Space Adventures and Excalibur Almaz – both of which are hoping to offer lunar fly-bys (no Moon walks, sorry) for $150 million apiece someday. Many analysts predict that in the coming decade, this industry will begin to (no pun intended) take flight. As such, establishing infrastructure there ahead of time would certainly be beneficial.

“We’re going back to the Moon”. That appeared to be central the message behind the recent symposium and the ESA’s plans for future space exploration. And this time, it seems, we will be staying there! And from there, who knows? The Universe is a big place…

Further Reading: European Space Agency

ExoMars 2016 Orbiter and Lander Mated for March Launch

ExoMars Schiaparelli lander being mated with the Trace Gas Orbiter on 12 February 2016. Credit: ESA - B. Bethge
ExoMars Schiaparelli lander being mated with the Trace Gas Orbiter on 12 February 2016. Credit: ESA - B. Bethge
ExoMars Schiaparelli lander being mated with the Trace Gas Orbiter on 12 February 2016. Credit: ESA – B. Bethge

Earth’s lone mission to the Red Planet this year has now been assembled into launch configuration and all preparations are currently on target to support blastoff from Baikonur at the opening of the launch window on March 14, 2016.

The ambitious ExoMars 2016 mission is comprised of a pair of European spacecraft named the Trace Gas Orbiter (TGO) and the Schiaparelli lander, built and funded by the European Space Agency (ESA). Continue reading “ExoMars 2016 Orbiter and Lander Mated for March Launch”