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November GeoRoundUp: the best of the Earth sciences from around the web

November GeoRoundUp: the best of the Earth sciences from around the web

Drawing inspiration from popular stories on our social media channels, major geoscience headlines, as well as unique and quirky research, this monthly column aims to bring you the latest Earth and planetary science news from around the web.

Major stories

Earth’s red and rocky neighbor has been grabbing a significant amount of attention from the geoscience media this month. We’ll give you the rundown on the latest news of Mars.

The NASA-led InSight lander, short for Interior Exploration using Seismic Investigations, Geodesy and Heat Transport, touched down on the Red Planet’s surface last week, causing the space agency’s Jet Propulsion Laboratory (JPL) control room to erupt in applause, fist pumps, and cool victory handshakes.

The lander, equipped with a heat probe, a radio science instrument and a seismometer, will monitors the planet’s deep interior. Currently, no other planet besides our own has been analysed in this way.

While scientists know quite a bit about the atmosphere and soil level of Mars, their understanding of the planet’s innerworkings, figuratively and literally, only scratches the surface. “We don’t know very much about what goes on a mile below the surface, much less 2,000 miles below the surface down to the center,” explains Bruce Banerdt, a scientist at JPL, to the Atlantic.

By probing into Mars’ depths, researchers hope the mission gives insight into the evolution of our solar system’s rocky planets in their early stages and helps explain why Earth and Mars formed such different environments, despite originating from the same cloud of dust.

“Our measurements will help us turn back the clock and understand what produced a verdant Earth but a desolate Mars,” Banerdt said recently in a press release.

The InSight lander launched from Earth in May this year, making its way to Mars over the course of seven months. Once reaching the planet’s upper atmosphere, the spacecraft decelerated from about 5,500 to 2.4 metres per second, in just about six minutes. To safely slow down its descent, the lander had to use a heatshield, a parachute and retro rockets.

“Although we’ve done it before, landing on Mars is hard, and this mission is no different,” said Rob Manning, chief engineer at JPL, during a livestream. “It takes thousands of steps to go from the top of the atmosphere to the surface, and each one of them has to work perfectly to be a successful mission.”

This artist’s concept depicts NASA’s InSight lander after it has deployed its instruments on the Martian surface. Credit: NASA/JPL-Caltech

The InSight lander is currently situated on Elysium Planitia, a plane near the planet’s equator also known by the mission team as the “biggest parking lot on Mars.” Since landing, the robot has taken its first photos, opened its solar panels, and taken preliminary data. It will spend the next few weeks prepping and unpacking the instruments onboard.

The devices will be used to carry out three experiments. The seismometers will listen for ‘marsquakes,’ which can offer clues into the location and composition of Mars’ rocky layers. The thermal probe will reveal how much heat flows out of the planet’s interior and hopefully show how alike (or unalike) Mars is to Earth. And finally, radio transmissions will demonstrate how the planet wobbles on its axis.

In other news, NASA has also chosen a landing site for the next Mars rover, which is expected to launch in 2020. The space agency has announced that the rover will explore and take rock samples from Jezero crater, one of the three locations shortlisted by scientists. The crater is 45 kilometres wide and at one point had been filled with water to a depth of 250 metres. The sediment and carbonate rocks left behind could offers clues on whether Mars had sustained life.

What you might have missed

By analysing radar scans and sediment samples, a team of scientists have discovered a massive crater, hidden underneath more than 900 metres of ice in northwest Greenland. After surveying the site, scientists say it’s likely that a meteorite created the sometime between 3 million and 12,000 years ago.

The depression under Hiawatha Glacier is 31 kilometres wide, big enough to hold the city of Paris. At this size, the crater is one of the top 25 largest craters on Earth; it’s also the first to be found under ice. An impact of this size significant mark on the Earth’s environment. “Such an impact would have been felt hundreds of miles away, would have warmed up that area of Greenland and may have rained rocky debris down on North America and Europe,” said Jason Daley from Smithsonian Magazine.

Links we liked

The EGU Story

This month, we have announced changes to the EGU General Assembly 2019 schedule, which aim to give more time for all presentation types. Check our news announcement for more information. In other news, we have opened applications to the EGU General Assembly 2019 mentoring programme, and are advertising a job opportunity for geoscientists with science communication experience to work at the meeting.

Also this month, we opened the call for applications for EGU Public Engagement Grants, and have announced the creation of the EGU Working Group on Diversity and Equality. Finally, we’ve published a press release on a new study that looked into whether data on seabird behavior could be used to track the ocean’s currents.

And don’t forget! To stay abreast of all the EGU’s events and activities, from highlighting papers published in our open access journals to providing news relating to EGU’s scientific divisions and meetings, including the General Assembly, subscribe to receive our monthly newsletter.

NASA’s InSight mission: detecting ‘earthquakes*’ on the surface of Mars

NASA’s InSight mission: detecting ‘earthquakes*’ on the surface of Mars

In three days’ time, NASA’s InSight Lander is expected to plunge through Mars’ atmosphere before parachuting down to a controlled landing on the flat plains of the Elysium Planitia.

Once the dust has settled, a solar powered robotic arm will painstakingly unload the precious instruments stored onboard onto the planet’s surface, carefully guided by scientists back on Earth.

This is an illustration showing a simulated view of NASA’s InSight about to land on the surface of Mars. (Credit: NASA/JPL-Caltech)

These instruments are designed to penetrate further into Mars’ subterranean secrets than any mission before. While previous Martian landers have monitored the planet’s surface and atmosphere, the goal of InSight, short for Interior Exploration using Seismic Investigations, Geodesy and Heat Transport, is to explore Mars’ interior using three specialised tools.

These include a heat probe which will measure the heat flow near to the surface, a radio science instrument which will measure how Mars wobbles on its axis, and a seismometer which will tell us about Mars’ deep interior. Scientists hope this will lead to new information on the formation of the planets in our solar system, perhaps even illuminating more detail on how our own planet came about.

Seismometers detect seismic waves, vibrations that travel through the ground after an event such as fault movement or meteorite impact. The type of wave and the speed at which it travels can provide important details about the material through which it moves. On Earth, a global network of seismometers has provided vital information about the structure of the planet’s core and mantle.

Robert Myhill, a seismologist at the University of Bristol, is part of a large international team of scientists who have been preparing for data returned by InSight’s seismometers (known as SEIS). Until recently, Myhill has been investigating how SEIS will be affected by Mars’ regolith (its shallow soil surface)[1].

Now that SEIS is en route to its Martian home however, Myhill and colleagues are getting ready for the next phase: receiving the data. “We hope to be able to use the waveforms from marsquakes and/or impacts to image the interior structure of the planet for the first time, including the thickness and structure of the crust, and the composition of the mantle and core,” Myhill explains.

“We’ve also been investigating how we can combine the geophysical data returned by InSight with existing geochemical data to tell us about the history of Mars and the continuing evolution of the planet’s deep interior.”

The data they will receive comes from two different types of sensors, a ‘very-broad-band’ (known as ‘VBB’) seismometer and three tiny short-period seismic sensors which are about the size of a Euro coin. The different sensors can detect various types of seismic wave, depending on the size and location of the seismicity.

Animation of InSight deploying it’s seismometer. (Credit: NASA/JPL-Caltech)

Gathering the information needed to achieve the mission’s goals presents numerous challenges. For starters, unlike Earth, which has a network of seismometers that can be used together, InSight will be the only active geophysical station on the Red Planet. Two previous seismometers, mounted on NASA’s Viking Landers in the 1970s, experienced technical faults and design limitations and are no longer in action. As a result, researchers have had to come up with novel ways to gather information from the lone InSight lander [2] [3].

The mission’s designers have also developed new technology to reduce noise and ensure the equipment can operate in Mars’ harsh environment. The seismometer will be mounted on a levelling system close to the Martian surface to minimise tilt and reduce the effect of wind. Once levelled, the lander’s robotic arm will place a wind and thermal shield over the top of the instruments, sheltering the sensitive instruments from extreme temperatures and buffeting by the Martian winds.

Despite the increased protection afforded by the wind and thermal shield, there remain challenges for InSight. “We hope that during the lifetime of the mission, we don’t have a prolonged dust-storm. Although InSight would not be damaged by such an event, it does need solar energy for all its instruments and for data transmission,” said Myhill.

NASA’s InSight mission tests an engineering version of the spacecraft’s robotic arm in a Mars-like environment at NASA’s Jet Propulsion Laboratory. (Credit: NASA/JPL-Caltech)

From 26 November, he and the others involved must wait with bated breath to see their hard work come to fruition. “We should receive the first data from the instrument deck not long after landing, but full deployment of SEIS (including the wind and thermal shield) is not scheduled until early January 2019,” he explains.

“The timing of first results really depends on the level of seismicity, which is currently very poorly known. In fact, determining the rate of seismic energy generation is one of the primary goals of the InSight Mission. But of course, we’re all hoping to see something soon after deployment.”

For the most up to date information on the mission, as well as more details in the lander’s other exciting capabilities see NASA’s InSight website.

*Astute readers of this blog may have noticed the error in the title. There is no such thing as an earthquake on Mars… instead InSight will be monitoring ‘marsquakes’.

By Keri McNamara, freelance science writer

Keri McNamara is a freelance writer with a PhD in Volcanology from the University of Bristol. She is on twitter @KeriAMcNamara and www.kerimcnamara.com.

References

[1]                      https://link.springer.com/article/10.1007/s11214-018-0514-5

[2]                      https://www.sciencedirect.com/science/article/abs/pii/S001910351400582X

[3]                      https://www.sciencedirect.com/science/article/pii/S0031920116300875?via%3Dihub

October GeoRoundUp: the best of the Earth sciences from around the web

October GeoRoundUp: the best of the Earth sciences from around the web

Drawing inspiration from popular stories on our social media channels, major geoscience headlines, as well as unique and quirky research, this monthly column aims to bring you the latest Earth and planetary science news from around the web.

Major story

In October, the UN Intergovernmental Panel on Climate Change (IPCC) released a landmark report and summary statement that detailed the severe consequences for our environment and society if global warming continues unabated. The special report, also known as the SR15, was compiled by 91 authors from 40 countries, and cites more than 6,000 peer-reviewed studies.

“There’s no doubt that this dense, science-heavy, 33-page summary is the most significant warning about the impact of climate change in 20 years,” said Matt McGrath an environment correspondent for BBC News.

The  EGU announced its support of the IPCC report in a statement published last month. In this address, EGU President Jonathan Bamber said: “EGU concurs with, and supports, the findings of the SR15 that action to curb the most dangerous consequences of human-induced climate change is urgent, of the utmost importance and the window of opportunity extremely limited.”

The IPCC was first commissioned to produce this report by the UN Convention on Climate Change following the Paris agreement, where world leaders pledged to limit global warming to well below 2ºC above pre-industrial levels and “pursue efforts” towards 1.5ºC. The goal of the report was to better understand what it would take for the world to successfully meet this 1.5ºC target and what the consequences would be if we are unable to reach this goal.

The report illustrates the two different outcomes that would arise from limiting global warming to 1.5ºC or allowing temperatures to rise to 2ºC.

While a half-degree doesn’t come across like a pronounced difference, the report explains that additional warming by this degree could endanger tens of millions more people across the world with life-threatening heat waves, water shortages, and coastal flooding from sea level rise. This kind of warming would also increase the chances that coral reefs and Arctic sea ice in the summer would disappear. These are just a few of the impacts detailed in the report. Recently, Carbon Brief has also produced an interactive graphic that does a deep dive into how climate change at 1.5ºC, 2ºC and beyond will impact different regions and communities around the world.

It should be noted that while limiting warming to 1.5ºC is the better of the two pathways, it still isn’t optimal. For example, under this warming threshold, the authors of the report project that global  sea levels would still rise, coral reefs would decline by 70-90%, and more than 350 million additional people would be exposed to severe drought.

Furthermore, the report goes on to explain what action (and just how much of it) would be necessary to limit warming to 1.5ºC. An article from the Guardian perhaps put it best: “there’s one simple critical takeaway point: we need to cut carbon pollution as much as possible, as fast as possible.

The report authors emphasise that limiting warming would require a massive international movement to reduce emissions and remove carbon dioxide from the atmosphere; and additionally this effort would need to happen within the next few years to avoid the most severe outcomes. They warn that if greenhouse emissions are still released at their current rate, the Earth’s temperature may reach 1.5ºC some time between 2030 and 2052, and reach more than 3ºC by 2100. Even more so, they concluded that the greenhouse gas reduction actions currently pledged by various countries around the world are still not enough to limit warming to 1.5ºC.

Measures to reach this temperature target include reducing global carbon dioxide emissions by 45% from 2010 levels by 2030, and reach a ‘net-zero’ by 2050. and making dramatic investments in renewable energy. They conclude that 70-35% of the world’s electricity should be generated by renewables like wind and solar power by 2050. By that same time, the coal industry would need to be phased out almost entirely.

Moreover, the authors say that we would need to expand forests and develop technology to suck carbon dioxide from the atmosphere. The report notes that climate action needs to be taken on an individual level as well, such as reducing the amount of meat we eat and time we spend on flying airplanes.

The authors report that we have the technology and means to limit warming by 1.5ºC, but they warn that the current political climate could make reaching this goal less likely.

“Limiting warming to 1.5ºC is possible within the laws of chemistry and physics but doing so would require unprecedented changes,” said Jim Skea, Co-Chair of IPCC Working Group III, in an IPCC press release.

Still have questions about the recent report? The IPCC has released a comprehensive FAQ and Carbon Brief has published an in-depth Q&A that addresses questions such as why the panel released the report, why adaptation is important, what the reaction has been, and what’s next.

What you might have missed

BepiColombo approaching Mercury. Credit: ESA/ATG medialab; Mercury: NASA/JPL

Last month the science media was also abuzz with a series of space agency news. On 20 October, the European-Japanese mission BepiColombo successfully launched from French Guiana, starting its seven-year long journey to Mercury, the smallest and least explored terrestrial planet in the Solar System. The probe is poised to be the third mission to travel to Mercury.

Once it arrives in 2025, the spacecraft will actually separate into two satellites, which will orbit the planet for at least one year. One satellite will investigate Mercury’s magnetic field while the other will take a series of measurements, including collecting data on the planet’s terrain, topography, and surface structure and composition. The researchers involved with the mission hope to learn more about Mercury’s origins and better understand the evolution of our solar system.

While one mission has started its journey, another’s has come to an end. Last month NASA’s planet-hunting Kepler space telescope has officially been retired after running out of fuel. Over its 9-year life span, the telescope has spotted more than 2,600 planets outside our solar system, many of which are possibly capable of sustaining life.

“As NASA’s first planet-hunting mission, Kepler has wildly exceeded all our expectations and paved the way for our exploration and search for life in the solar system and beyond,” said Thomas Zurbuchen, associate administrator of NASA’s Science Mission Directorate in Washington. “Not only did it show us how many planets could be out there, it sparked an entirely new and robust field of research that has taken the science community by storm. Its discoveries have shed a new light on our place in the universe, and illuminated the tantalizing mysteries and possibilities among the stars.”

However, even though Kepler’s planet-scoping days are over, NASA’s new space observatory, the Transiting Exoplanet Survey Satellite (TESS) mission, which launched in April 2018, will continue the search for habitable worlds.

NASA’s Kepler space telescope, shown in this artist’s concept, revealed that there are more planets than stars in the Milky Way galaxy. Image credit: NASA

Links we liked

The EGU story

Earlier in October, we announced the winners of the 2019 EGU awards and medals: 45 individuals who have made significant contributions to the Earth, planetary and space sciences and who will be honoured at the 2019 EGU General Assembly next April. We have also announced the winners of the Outstanding Student Poster and PICO (OSPP) Awards corresponding to the 2018 General Assembly, which you can find on our website. Congratulations to all!

This month, we also opened the call for abstracts for the EGU 2019 General Assembly. If you are interested in presenting your work in Vienna in April, make sure you submit your abstract by 10 January 2019, 13:00 CET. If you would like to apply for a Roland Schlich travel grant to attend the meeting, please submit your abstract no later than 1 December 2018. You can find more information on the EGU website.

Interested in science and art? After successfully hosting a cartoonist and a poet in residence at last year’s annual meeting, we are now opening a call for artists to apply for a residency at the EGU 2019 General Assembly. The deadline for applications is 1 December. You can find more information about the opportunity online here.

And don’t forget! To stay abreast of all the EGU’s events and activities, from highlighting papers published in our open access journals to providing news relating to EGU’s scientific divisions and meetings, including the General Assembly, subscribe to receive our monthly newsletter.

NASA’s Juno mission reveals Jupiter’s magnetic field greatly differs from Earth’s

NASA’s Juno mission reveals Jupiter’s magnetic field greatly differs from Earth’s

NASA scientists have revealed surprising new information about Jupiter’s magnetic field from data gathered by their space probe, Juno.

Unlike earth’s magnetic field, which is symmetrical in the North and South Poles, Jupiter’s magnetic field has startlingly different magnetic signatures at the two poles.

The information has been collected as part of the Juno program, NASA’s latest mission to unravel the mysteries of the biggest planet in our solar system. The solar-powered spacecraft is made of three 8.5 metre-long solar panels angled around a central body. The probe (pictured above) cartwheels through space, travelling at speeds up to 250,000 kilometres per hour.

Measurements taken by a magnetometer mounted on the spacecraft have allowed a stunning new insight into the planet’s gigantic magnetic field. They reveal the field lines’ pathways vary greatly from the traditional ‘bar magnet’ magnetic field produced by earth.

Jupiter’s magnetic field is enormous. if magnetic radiation were visible to the naked eye, from earth, Jupiter’s magnetic field would appear bigger than the moon. Credit: NASA/JPL/SwRI

The Earth’s magnetic field is generated by the movement of fluid in its inner core called a dynamo. The dynamo produces a positive radiomagnetic field that comes out of one hemisphere and a symmetrical negative field that goes into the other.

The interior of Jupiter on the other hand, is quite different from Earth’s. The planet is made up almost entirely of hydrogen gas, meaning the whole planet is essentially a ball of moving fluid. The result is a totally unique magnetic picture. While the south pole has a negative magnetic field similar to Earth’s, the northern hemisphere is bizarrely irregular, comprised of a series of positive magnetic anomalies that look nothing like any magnetic field seen before.

“The northern hemisphere has a lot of positive flux in the northern mid latitude. It’s also the site of a lot of anomalies,” explains Juno Deputy Principal Investigator, Jack Connerney, who spoke at a press conference at the EGU General Assembly in April. “There is an extraordinary hemisphere asymmetry to the magnetic field [which] was totally unexpected.”

NASA have produced a video that illustrates the unusual magnetism, with the red spots indicating a positive magnetic field and the blue a negative field:

Before its launch in 2016, Juno was programmed to conduct 34 elliptical ‘science’ orbits, passing 4,200 kilometres above Jupiter’s atmosphere at its closest point. When all the orbits are complete, the spacecraft will undertake a final deorbit phase before impacting into Jupiter in February 2020.

So far Juno has achieved eleven science orbits, and the team analysing the data hope to learn more as it completes more passes. “In the remaining orbits we will get a finer resolution of the magnetic field, which will help us understand the dynamo and how deep the magnetic field forms” explains Scott Bolton, Principal Investigator of the mission.

The researchers’ next steps are to examine the probe’s data after its 16th and 34th passes meaning it will be a few more months before they are able to learn more of Jupiter’s mysterious magnetosphere.

By Keri McNamara, EGU 2018 General Assembly Press Assistant

Further reading

Connerney, J. E. P., Kotsiaros, S., Oliversen, R. J., Espley, J. R., Joergensen, J. L., Joergensen, P. S., et al. A new model of Jupiter’s magnetic field from Juno’s first nine orbits. Geophysical Research Letters, 45, 2590–2596. 2018

Bolton, S. J. et al. Jupiter’s interior and deep atmosphere: The initial pole-to-pole passes with the Juno spacecraft, Science, 356(6340), p. 821 LP-825. 2017

Guillot, T. et al. A suppression of differential rotation in Jupiter’s deep interior, Nature. Macmillan Publishers Limited, part of Springer Nature. All rights reserved., 555, p. 227. 2018