Category Archives: Space
Not one but two Aussie dishes were used to get the TV signals back from the Apollo 11 moonwalk

NASA
The role Australia played in relaying the first television images of astronaut Neil Armstrong’s historic walk on the Moon 50 years ago this July features in the popular movie The Dish.
But that only tells part of the story (with some fictionalisation as well).
What really happened is just as dramatic as the movie, and needed two Australian dishes. Australia actually played host to more NASA tracking stations than any other country outside the United States.
Read more:
How big is the Moon? Let me compare …
Right place, right time
Our geographical location was ideal as US spacecraft would pass over Australia during their first orbit, soon after launch. Tracking facilities in Australia could confirm and refine their orbits at the earliest possible opportunity for the mission teams.
To maintain continuous coverage of spacecraft in space as the Earth turned, NASA required a network of at least three tracking stations, spaced 120 degrees apart in longitude. Since the first was established in the US at Goldstone, California, Australia was in exactly the right longitude for another tracking station. The third station was near Madrid in Spain.
Australia’s world-leading place in radio astronomy was another factor, having played a key role in founding the science after the second world war. Consequently, Australian engineers and scientists developed great expertise in designing and building sensitive radio receivers and antennas.
While these were great at discovering pulsars and other stars, they also excelled at tracking spacecraft. When the CSIRO Parkes radio telescope opened in 1961 it was the most advanced and sensitive dish in the world. It became the model for NASA’s large tracking antennas.

CSIRO, Author provided
The Commonwealth Rocket Range at Woomera, South Australia, also allowed Australians to gain experience in tracking missiles and other advanced systems.
The dish you need is at Honeysuckle Creek
NASA invested a considerable amount in its Australian tracking facilities, all staffed and operated by Australians under a nation-to-nation treaty signed in February 1960.
For human spaceflight, the main tracking station was at Honeysuckle Creek, near Canberra. Its 26-metre dish was designed as NASA’s prime antenna in Australia for supporting astronauts on the Moon.

Hamish Lindsay, Author provided
NASA’s nearby Deep Space Network station at Tidbinbilla also had a 26-metre antenna but with a more sensitive radio receiver. It was called on to act as a wing station to Honeysuckle Creek, enhancing its capabilities, and ultimately tracked the orbiting command module during Apollo 11.
Over in Western Australia, Carnarvon’s smaller 9-metre antenna was used to track the Apollo spacecraft when initially in Earth orbit, as well as to receive signals from the lunar surface experiments.
To augment the receiving capabilities of these stations, the 64-metre Parkes radio telescope was asked to support Apollo 11 while astronauts were on the lunar surface. The observatory’s director, John Bolton, was prepared to accept a one-line contract:
The Radiophysics Division would agree to support the Apollo 11 mission.
The original plan
The decision to broadcast the first moonwalk was almost an afterthought.
Originally, the tracking stations were to receive only voice communications and spacecraft and biomedical telemetry. What mattered most to mission control was the vital telemetry on the status of the astronauts and the lunar module systems.
Since Parkes was an astronomical telescope, it could only receive the signals, not transmit. It was regarded as a support station to Honeysuckle Creek, which was also tasked with receiving the signals from the lunar module, Eagle.
When the decision was made to broadcast the moonwalk, Parkes came into its own. The large collecting area of its dish provided extra gain in signal strength, making it ideal for receiving a weak TV signal transmitted 384,000km from the Moon, using the same power output as two LED lights today.
One giant leap
On Monday, July 21 1969, at 6.17am (AEST), astronauts Neil Armstrong and Buzz Aldrin landed the Eagle lunar module on the Sea of Tranquillity.
It occurred during the coverage period of the Goldstone station, while the Moon was still almost seven hours from rising in Australia.
The flight plan had the astronauts sleeping for six hours before preparing to exit the lunar module. Parkes was all set to become the prime receiving station for the TV broadcast.
This changed when Armstrong exercised his option for an immediate walk – five hours before the Moon was to rise at Parkes. With this change of plan, it seemed the moonwalk would be over before the Moon even rose in Australia.
But as the hours passed, it became evident that the process of donning the spacesuits took much more time than anticipated. The astronauts were being deliberately careful in their preparations. They also had some difficulty in depressurising the cabin of the lunar module.
Meanwhile, moonrise was creeping closer in Australia. Staff at Honeysuckle Creek and Parkes began to hope they might get to track the moonwalk after all – at least as a backup to Goldstone in the US.
Bad weather hits
The weather at Parkes on the day of the landing was miserable. It was a typical July winter’s day – grey overcast skies with rain and high winds. During the flight to the Moon and the days in lunar orbit, the weather at Parkes had been perfect, but this day, of all days, a violent squall hit the telescope.

CSIRO/David Cooke, Author provided
Still, the giant dish of the Parkes radio telescope was fully tipped down to its 30-degree elevation limit (the telescope’s horizon is 30 degrees above the true horizon), waiting for the Moon to rise in the north-east.
As the Moon slowly crept up to the telescope’s horizon, dust was seen racing across the country from the south. The dish, being fully tipped over, was at its most vulnerable, acting like a huge sail.
The winds picked up and two sharp gusts exceeding 110km/h struck the large surface, slamming it back against the zenith angle drive pinions that controlled the telescope’s up and down motion. The control tower shuddered and swayed from this battering, creating concern in all present.
The atmosphere in the control room was tense, with the wind alarm ringing and the 1,000-ton telescope ominously rumbling overhead.
Parkes had two radio receivers installed in the focus cabin of the telescope. The main receiver was on the focus position and a second, less sensitive receiver was offset a very short distance away, which gave it a view just below the main receiver.
Fortunately, as the winds abated, the Moon rose into the field-of-view of the telescope’s offset receiver, just as Aldrin activated the TV at 12.54pm (AEST). It was a remarkable piece of timing.

CSIRO/David Cooke, Author provided
The 64m antenna at Goldstone, the 26m antenna at Honeysuckle Creek and the 64m dish at Parkes all received the signal simultaneously.
At first, NASA switched between the signals from Goldstone and Honeysuckle Creek, searching for the best-quality TV picture.
After finding Goldstone’s image initially upside down and then of poor quality, Houston selected Honeysuckle’s incoming signal as the one used to broadcast Armstrong’s “one giant leap” to the world.
Eight minutes into the broadcast, at 1.02pm (AEST), the Moon finally rose high enough to be received by Parkes’ main, on-focus receiver. The TV quality improved, so Houston switched to Parkes and stayed with it for the remainder of the two-and-a-half hours of the moonwalk, never switching away.
Honeysuckle continued to concentrate on their main task of communications with the astronauts and receiving that vital telemetry data.

CSIRO/David Cooke, Author provided
Throughout the moonwalk, the weather remained bad at Parkes. The telescope operated well outside safety limits for the entire duration. It even hailed toward the end, but there was no degradation in the TV signal.
It’s hailing on the dish.
CSIRO, Author provided321 KB (download)
CSIRO, Author provided321 KB (download)
The moonwalk lasted a total of 2 hours, 31 minutes and 40 seconds, from the time the Eagle’s hatch opened to the time the hatch closed.
Australians saw it first
In Australia, the Apollo 11 feed was split. One feed was sent to NASA mission control for broadcast around the world. The other went directly to the ABC’s Gore Hill studios, in Sydney, for distribution to Australian TV networks.
As a result Australians watched the moonwalk, and Armstrong’s first step through Honeysuckle, just 300 milliseconds before the rest of the world.
Read more:
We need to protect the heritage of the Apollo missions
An estimated 600 million people, one-sixth of the world’s population at the time, watched the historic Apollo 11 moonwalk live on TV. At the time it was the greatest television audience in history. As a proportion of the world’s population, it has not been exceeded since.
The success of the Apollo 11 mission was due to the combined effort, dedication and professionalism of hundreds of thousands of people in the United States and around the planet.
Australians from Canberra to Parkes, remote Western Australia to central Sydney played a critical role in helping broadcast that historic moment to an awestruck world.
Parkes gives NASA the best TV pictures yet.
NASA/CSIRO, Author provided267 KB (download)
NASA/CSIRO, Author provided267 KB (download)

NASA
You can hear more about the Moon landing in our special podcast series, To the Moon and beyond.
John Sarkissian, Operations Scientist, CSIRO
This article is republished from The Conversation under a Creative Commons license. Read the original article.
We need to protect the heritage of the Apollo missions

NASA
Alice Gorman, Flinders University
It’s 50 years since the two Apollo 11 astronauts – Neil Armstrong and Buzz Aldrin – spent 22 hours collecting samples, deploying experiments and sometimes just playing in the Sea of Tranquillity on the Moon.
In doing so, they created an archaeological site unique in human history.
Now, with what’s been called the New Space Race and plans to return to the Moon, the Apollo 11 and other lunar sites are under threat. We need to protect this heritage for future generations.
Read more:
How big is the Moon? Let me compare …
Apollo 11’s archaeological site
The archaeological site of Tranquillity Base consists of the hardware left behind, as well as the marks made in the lunar surface by the astronauts and instruments.

NASA
The hardware component includes the landing module, the famous flag (no longer standing), experiment packages, cameras, antennas, commemorative objects, space boots and many other discarded objects – more than 106 in total.
Around these objects are the first human footprints on the Moon as well as the tracks the astronauts made walking around, and the places where they dug out samples of rock and dust to take back to Earth for scientific analysis.
The artefacts, traces and the landscape constitute an archaeological site. The relationships between them can be used by archaeologists to study human behaviour in this environment so different to Earth, with one-sixth terrestrial gravity and no atmosphere.
Assessing the heritage value
Not only this, but the site has heritage value for people on Earth. To assess this, we can look at a number of categories of cultural significance. Those in the Burra Charter are widely used across the world for heritage assessment.
Historic: There is no doubt that, as the first place where humans set foot on another celestial body, this is a very important place in global history. It also represents the ideologies of the Cold War (1947-1992) between the US and the USSR.

NASA
Scientific: What can we learn from the site? More particularly, what questions would we no longer be able to answer if Tranquillity Base was damaged or destroyed?
This is not just about archaeological research into human behaviour on the Moon. Apollo 11 has been exposed to the harsh lunar environment for 50 years. The surfaces of the hardware are accidental experiments in themseves: they carry the record of 50 years of micrometeorite and cosmic ray bombardment. Finding out how well the materials have survived can also provide information about how to design future missions.
Aesthetic: This type of cultural significance is about how we experience a place. While we can’t assess it in person, there are films and photographs that give us a feeling for the place. This includes the light, shadows and colours of the lunar surface from the perspective of the human senses. The aesthetic qualities have inspired many artists and musicians, including astronaut Alan Bean who devoted his post-Apollo 12 life to painting the Moon.

NASA
Social: This is about the value that contemporary communities place on the site. For the 600 million-plus people who watched the television broadcast of the landing, it was a life-changing moment representing the ingenuity of human technology and visions of a space-age future.
But the mission did not mean the same for everyone. Some African-Americans protested against Apollo 11, seeing it as a waste of resources when there was such great economic and social disparity between white and black communities in the US. For them, it was a sign of human failure rather than a triumph.
The larger the community that has an interest in a heritage place, the higher its level of social significance. It could be argued that Apollo 11 has outstanding universal significance, like places on the World Heritage List (unfortunately the World Heritage Convention cannot be applied to space).
What are the threats?
In the past few years we have seen an increase in proposed missions to return to the Moon. Some have stated their intention to revisit the Apollo sites, by human crew or robot – and this could lead to the removal of material, for souvenirs or science.
But the sites are both fragile and unprotected. The two primary risks to their survival are uncontrolled looting, and damage from abrasive and sticky lunar dust.

NASA
Removing material from the sites damages the integrity of the artefacts and the relationships between them. A casual visit could erase the original footprints and astronaut traverses. The corrosive dust disturbed by surface activities could wear away the materials.
Dust was a problem for all the crewed lunar missions. Apollo 16 commander John Young said: “Dust is the number one concern in returning to the Moon.”
The dust can be stirred up by plumes from landing or ascending vehicles, driving vehicles, walking on the surface, or, in the next phase of lunar settlement, by construction and industrial activities, such as mining.
Attempts at protection
The Outer Space Treaty of 1967 forbids making territorial claims in space. Applying any national heritage legislation to a place on the Moon could be interpreted as a territorial claim.
The US states of California and New Mexico have placed the Apollo 11 artefacts left on the Moon on a heritage list. They can do this because, under the treaty, the US legally owns the artefacts. But this does not protect the site itself.

NASA
NASA has established a set of heritage guidelines for its sites on the Moon. The guidelines propose buffer zones around these areas, inside which no-one should enter. They make recommendations for approaching the sites to minimise dust disturbance.
In May 2019, a bill called the One Small Step to Protect Human Heritage in Space Act was introduced to the US Congress. Its purpose is:
To require any Federal agency that issues licences to conduct activities in outer space to include in the requirements for such licences an agreement relating to the preservation and protection of the Apollo 11 landing site, and for other purposes.
But the bill applies only to Apollo 11 and does not have similar requirements for the five other Apollo landing sites. It also applies only to US missions. It’s a step in the right direction, but there is still much more to be done.

NASA
Only in the last decade has the idea of space archaeology gained legitimacy. Until recently, there was no urgency to establish an international framework to manage the cultural values of lunar heritage.
Read more:
Why the Moon is such a cratered place
Now we’re in a new situation. On Earth, it’s common for industrial or urban activities that disturb the environment to be subject to an environmental impact assessment, which includes heritage.
Even when there are no laws to force companies to pay attention to heritage, many consider it important to seek a Social Licence to Operate – support from stakeholder communities to continue their activities.
Everyone on Earth is a stakeholder in the heritage of the Moon. Fifty years from now, what will remain of the Apollo 11 and other sites? What new meanings will people draw from it?
Alice Gorman, Senior Lecturer in Archaeology and Space Studies, Flinders University
This article is republished from The Conversation under a Creative Commons license. Read the original article.
Aboriginal traditions describe the complex motions of planets, the ‘wandering stars’ of the sky

Flickr/Indigo Skies Photography, CC BY-NC-ND
Duane W. Hamacher, Monash University
Aboriginal and Torres Strait Islander readers are advised that this story may contain images and voices of people who have died.
The five planets we can see by naked eye were known to the ancient Greeks as “asteres planetai”, meaning “wandering stars”, due to their wandering journey across the sky relative to the fixed stars. This is where we get the word “planet”.
But knowledge of the planets and their movements goes back much further, being prominent in the traditions of the oldest continuing cultures in the world.
Recent research reveals a wealth of information about the planets and their complex motions in the Knowledge Systems of Indigenous Australians.
The wandering stars
These systems show that Aboriginal and Torres Strait Islander people carefully observe the complex motions of the planets.
Read more:
The stories behind Aboriginal star names now recognised by the world’s astronomical body
In Wardaman traditions, the planets are ancestor spirits who walk across a celestial road. Wardaman Elder Bill Yidumduma Harney calls it the Dreaming Track in the Sky.
Astronomers call this celestial road the zodiac – the region of sky nine degrees on either side of the ecliptic (the path of the Sun). As the planets orbit the Sun in roughly the same plane, they all are visible along this band of the sky.

ESA
Uncle Yidumduma describes the planet-ancestors moving across the sky much like we walk down a busy footpath. We sometimes hurriedly pass each other, or slow down for a chat. Occasionally, we even stop and turn backwards to chat with someone before moving forward again.
Astronomers call this phenomenon retrograde motion. It is an optical effect that occurs as the planets orbit the Sun at different distances and velocities. It means the planets can appear to slow down and move backwards for a time before returning to their normal motion.

ESA
There are five planets visible to the naked eye and right now, and you can see at least four – Venus, Mars, Jupiter and Saturn – in the sky at sunset from most locations across Australia. All of these planets are currently in retrograde motion.

Stellarium.
The (non) twinkling stars
Aboriginal and Torres Strait Islander people recognise that these wandering stars generally do not twinkle – a phenomenon the Meriam people of the eastern Torres Strait call epreki and observe to predict weather and seasonal change.
But sometimes they do twinkle, particularly if they are very low on the horizon. Kamilaroi people of northern New South Wales say Venus occasionally twinkles when it’s low in the sky. They say it’s an old man who told a rude joke and has been laughing ever since.
In the traditions of the Euahlayi people – neighbours of the Kamilaroi – Venus and Mars relate to songlines and trade with Arrernte people of the Central Desert.
During special ceremonies, the Arrernte travel from the MacDonnell Ranges to Quilpie in southwest Queensland, bringing with them a red stone that signifies Mars. The Euahlayi people bring a green and blue stone to the ceremony, representing Venus. They are seen as the different-coloured eyes of the creator spirit Baayami.
Venus – the Morning and Evening Star
Venus is commonly known in many Aboriginal and Torres Strait Islander cultures as both the Morning and Evening Star.
In the Dreaming stories of the Western Arrernte, a celestial baby fell from the Milky Way, striking the ground and creating the giant meteorite crater called Tnorala (Gosses Bluff). The child’s parents – the Morning and Evening Stars – take turns searching for their lost child to this day.
Arrernte mothers warn their children not to look at the Morning or Evening Star, as the celestial parents might mistake them for their lost child and carry them away to the sky.
In Yolngu traditions of Arnhem Land, a special ceremony is held to signify the rising of the Creation ancestor, Banumbirr (Venus), between the mainland and a Burralku – the sacred island of the dead.
The ceremony starts at dusk and continues through the night, reaching a climax when Banumbirr rises a few hours before dawn as Venus transitions from the Evening Star to the Morning Star. Banumbirr communicates with the people through a faint rope that holds her close to the Sun.
Astronomers call this zodiacal light – the glow of dust in the plane of the Solar System.

ESO
The first rising of Venus as the Morning Star, after it transitions from the Evening Star, occurs every 584 days. Astronomers refer to this as Venus’ synodic period.
Read more:
Stars that vary in brightness shine in the oral traditions of Aboriginal Australians
When astronomer Ray Norris asked a Yolngu elder how the people know when to hold the Banumbirr ceremony, the elder responded: “We count the days!”
That’s an achievement not often recognised, and just another example of the detailed understanding of these “wandering stars” in the Knowledge Systems of Indigenous Australians.
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Kirsten Banks, a Wiradjuri woman and astrophysics graduate from the University of New South Wales, contributed to this research and this article. She can be contacted at astronomerkirsten@gmail.com
Duane W. Hamacher, Senior Research Fellow, Monash University
This article was originally published on The Conversation. Read the original article.
How ancient cultures explained comets and meteors

Eve MacDonald, Cardiff University
Comets and meteors have fascinated the human race since they were first spotted in the night sky. But without science and space exploration to aid understanding of what these chunks of rock and ice are, ancient cultures often turned to myth and legend to explain them.
The Greeks and Romans believed that the appearance of comets, meteors and meteor showers were portentous. They were signs that something good or bad had happened or was about to happen. The arrival of a comet could herald the birth of a great figure, and some people have even argued that the star in the sky which the Persian Magi followed to Bethlehem to see the newborn Jesus was actually a comet.
In the spring of 44BC, a comet that appeared was interpreted as a sign of the deification of Julius Caesar, following his murder. Caesar’s adopted son Octavian (soon to be the Emperor Augustus) made much of the comet, which burned in the sky during the funerary games held for Caesar. This portentous event was frequently celebrated in the ancient sources. In his epic poem, the Aeneid, Virgil describes how “a star appeared in the daytime, and Augustus persuaded people to believe it was Caesar”.

Wikimedia/Classical Numismatic Group, Inc., CC BY-SA
Augustus celebrated the comet and the deification of his father on coins (it did help to be the son of a god when trying to rule the Roman Empire), and many examples survive today.
Meteor showers
The Roman historian Cassius Dio referred to “comet stars” occurring in August 30BC. These are mentioned as among the portents witnessed after the death of the Egyptian queen Cleopatra. Experts are not entirely sure what it means when Dio uses the plural term “comet stars”, but some have connected this recorded event to the annual Perseid meteor shower.
Though it retains an ancient Greek name, we now know that the arrival of the Perseid meteor shower every August is actually the Earth’s orbit passing through debris from the Swift-Tuttle comet.

British Museum, CC BY-NC-SA
The meteor shower is named for the Perseidai (Περσείδαι), who were the sons of the ancient Greek hero Perseus. Perseus was a legendary figure with a fine family pedigree – he was the mythical son of Zeus and Argive princess Danaë (she of the golden rain). Perseus earned himself a constellation after a number of epic adventures across the Mediterranean and Near East that included the frequently illustrated murder of the Gorgon sister, Medusa.
Another of Perseus’s celebrated acts was the rescue of the princess Andromeda. Abandoned by her parents to placate a sea monster, the princess was found by Perseus on a rock by the ocean. He married her and they went on to have seven sons and two daughters. Sky watchers believed that the constellation Perseus, located just beside Andromeda in the night sky, was the origin of the shooting stars they could see every summer, and so the name Perseid stuck.

Wikimedia, CC BY-SA
Tears and other traditions
In Christian tradition the Perseid meteor shower has long been connected to the martyrdom of St Lawrence. Laurentius was a deacon in the early church at Rome, martyred in the year 258AD, during the persecutions of the Emperor Valerian. The martyrdom supposedly took place on August 10, when the meteor shower was at its height, and so the shooting stars are equated to the saint’s tears.
Detailed records of astronomical events and sky watching can be found in historical texts from the Far East too. Ancient and medieval records from China, Korea and Japan have all been found to contain detailed accounts of meteor showers. Sometimes these different sources can be correlated, which has allowed astronomers to track, for example, the impact of Halley’s comet on ancient societies both east and west. These sources have also been used to find the first recorded observation of the Perseid meteor shower as a specific event, in Han Chinese records of 36AD.
Though the myths and legends may make one think that ancient civilisations had little scientific understanding of what meteors, comets and asteroids could be, this couldn’t be farther from the truth. The early astronomers of the Near East, those who created the Babylonian and Egyptian calendars, and astronomical data were – by far – the most advanced in antiquity. And a recent study of ancient cuneiform texts has proven that the Babylonian ability to track comets, planetary movements and sky events as far back as the first millennium BC involved a much more complex geometry than had been previously believed.
Eve MacDonald, Lecturer in Ancient History, Cardiff University
This article was originally published on The Conversation. Read the original article.
A brief history of Martian exploration – as the InSight Lander prepares to launch

NASA
Helen Maynard-Casely, Australian Nuclear Science and Technology Organisation
Roughly every two years Mars and Earth wander a bit closer to each other, making the leap between these two planets a little easier. In July this year, Mars will only be about 58 million kilometres away – and NASA is set to take advantage by launching their next mission to the red planet in May 2018. The InSight Lander, will be the first Mars mission to investigate the planet’s “inner space”, and will listen for marsquakes to investigate the crust, mantle, and core.
InSight will join two rovers currently exploring the surface of Mars, and 14 spacecraft that are in orbit about it – albeit only six of which are currently sending us data.
Read more:
Ice mined on Mars could provide water for humans exploring space
Why does Mars, the red planet, have such a hold over us?
There are, after all, seven (or eight) other planets to explore – and yet we seem to have such a hang up on this one.
I guess it’s the tantalising nature of Mars. Here is a planet that we could conceivably walk on (unlike the gas giants), without being crushed by atmospheric pressure (like on Venus), having to deal with the radiation of being closer to the sun (Mercury) or just being far too far away (like Pluto). It calls to us through science fiction and fact, a planet that is so like our own Earth, but so unlike it at the same time.
The six current operational missions show that the fascination with Mars isn’t limited to one country, as European, Russian, American and Indian space agencies all have stakes in these crafts.
For comparison: our other nearest neighbour, Venus, only has one spacecraft currently in orbit about it, Akatsuki the spacecraft that wouldn’t quit. In fact, after the dramatic ending of the Cassini spacecraft, the only other planet currently being orbited by an Earth-built satellite is Jupiter, with the Juno mission.
Read more:
Juno mission unveils Jupiter’s complex interior, weather and magnetism
Water on Mars
But, while our progress to walking on Mars has been very slow, our progress in understanding our neighbour has been really quite impressive. When I started my planetary science degree in 2001, the course did not include sedimentology, the branch of geology that investigates how water has shaped rocks. It was deemed there was no point as no water has been seen on any other planet.
By the time I was in third year, the first years students behind me were getting well versed in how water could push around sand, silt and clay on other planets.
Finding water on Mars had been an obsession to many, and thanks to data from Mars rovers Spirit, Opportunity and latterly Curiosity we know that it’s there – just trapped in the rocks. A couple of years ago it was thought that we had even found water flowing on the surface of Mars, but that evidence is (ahem) drying up now.
Read more:
Dear diary: another day in the life on Mars
However, whether the water flows or is trapped in the rocks, the next question is where is the rest of it? If many of the rocks we see on Mars had been laid down by water – where is that water now?
The answer would be tangled up with the fate of Mars’s atmosphere. Though pitifully thin now, it must have been thick enough in the past to support flowing water on the surface. The mission of the spacecraft Maven (along with others) has been investigating this question – and all evidence is pointing to the Sun as the culprit for Mars’ missing atmosphere, with the solar wind gradually stripping it away.
Mars’ surface
It’s often touted that we know more about the surface of Mars than we do the bottom of our own oceans – and in terms of mapping resolution that’s true. Through the efforts of four orbiting missions we know how old most of the surface is, as well as how active it has been.
You can spend a joyful afternoon of procrastination flitting through HiRISE images that show sweeping dunes and pock-marked plains on Mars. With these images we can really apply our understanding of processes on Earth to what makes up the surface of Mars – from the formations of geological features, the movement of dust and sand and how the ice caps change through the seasons.
What’s inside Mars?
So we know there is water on Mars, we know where its atmosphere went and also the shifts of its sands – but there’s a missing piece of the puzzle. What’s on the inside?
To be fair, in this respect the interior of our own Earth is just as much of a mystery – but we have had centuries of seismic studies. From monitoring the passage of earthquakes through our planet we have built a picture of the layers that make up its interior. From that we’ve been able to undertake experiments that recreate the conditions and add more to that picture. At the moment we can only guess at the conditions within the interior of Mars – something that the InSight mission will answer.
Read more:
Before we colonise Mars, let’s look to our problems on Earth
After this, the next hurdle will be getting something back from Mars. We have a handful of meteorites that we know came from Mars, but having a sample that’s been collected and returned from a known location will priceless. NASA’s next rover, Mars 2020, will plan to do just this – but the return to Earth bit is still to be worked out.
From sample return to human exploration is still a massive step, and will require a number of innovations to get there. But with the knowledge we’ve built from the missions over the last decade, it’s becoming more of a reality.
Helen Maynard-Casely, Instrument Scientist, Australian Nuclear Science and Technology Organisation
This article was originally published on The Conversation. Read the original article.
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