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TGS to Participate at United States (U.S.)-Africa Energy Forum (USAEF) 2025 Amid Growing Data-Driven Activity in Africa
TGS to Participate at United States (U.S.)-Africa Energy Forum (USAEF) 2025 Amid Growing Data-Driven Activity in Africa

Zawya

time3 days ago

  • Business
  • Zawya

TGS to Participate at United States (U.S.)-Africa Energy Forum (USAEF) 2025 Amid Growing Data-Driven Activity in Africa

The U.S.-Africa Energy Forum (USAEF), taking place in Houston on August 6-7, 2025, is pleased to announce Kristian Johansen, Chief Executive Officer of TGS, as a featured speaker. TGS is a global leader in energy data and subsurface intelligence, with an expanding footprint across Africa supporting exploration and investment in oil, gas and renewable energy. As African nations prepare for new licensing rounds, farm-outs and energy diversification, access to high-quality seismic data and digital solutions is proving vital in attracting global capital. TGS' work across the continent – from deepwater seismic reprocessing to renewable resource assessments – is enabling governments to present technically de-risked, investment-ready acreage to the market. Recent activity spans some of Africa's most promising and underexplored regions. In Angola, TGS has reprocessed legacy data in a block previously relinquished by Shell, unlocking new geological insight. In the Republic of Congo, the company is supporting digitalization to enhance transparency and efficiency in upstream development. Expanded seismic coverage in Tanzania and Benin is helping to bring new frontier acreage to market, while in Mauritania, TGS is growing its multi-client 3D seismic library across more than 101,000 square-kilometers offshore – cementing its role in advancing exploration in high-potential deepwater zones. Meanwhile in Cabo Verde, the company is assessing renewable energy opportunities, including offshore wind, as part of its support for Africa's broader energy transition. TGS' growing presence in Africa highlights the critical role of data in enhancing the technical credibility and commercial appeal of emerging energy opportunities. By equipping governments and investors with deeper geological insight and actionable intelligence, the company is enabling faster, more confident decision-making – especially as exploration budgets tighten globally. With multiple licensing rounds anticipated across the continent, TGS continues to serve as a strategic data partner, supporting African markets in presenting transparent, competitive and technically validated acreage. For tickets, sponsorship opportunities and more information, please contact sales@ or visit Join us in Houston to connect with the leaders shaping Africa's energy landscape and experience the momentum that drives ECP's events worldwide. Distributed by APO Group on behalf of Energy Capital&Power.

New signals point to vast ocean of water hidden beneath Mars's crust
New signals point to vast ocean of water hidden beneath Mars's crust

The Independent

time12-05-2025

  • Science
  • The Independent

New signals point to vast ocean of water hidden beneath Mars's crust

Evidence is mounting that a secret lies beneath the dusty red plains of Mars, one that could redefine our view of the Red Planet: a vast reservoir of liquid water, locked deep in the crust. Mars is covered in traces of ancient bodies of water. But the puzzle of exactly where it all went when the planet turned cold and dry has long intrigued scientists. Our new study may offer an answer. Using seismic data from Nasa 's InSight mission, we uncovered evidence that the seismic waves slow down in a layer between 5.4 and 8 kilometres below the surface, which could be because of the presence of liquid water at these depths. The mystery of the missing water Mars wasn't always the barren desert we see today. Billions of years ago, during the Noachian and Hesperian periods (4.1 billion to 3 billion years ago), rivers carved valleys and lakes shimmered. As Mars' magnetic field faded and its atmosphere thinned, most surface water vanished. Some escaped to space, some froze in polar caps, and some was trapped in minerals, where it remains today. But evaporation, freezing and rocks can't quite account for all the water that must have covered Mars in the distant past. Calculations suggest the 'missing' water is enough to cover the planet in an ocean at least 700 metres deep, and perhaps up to 900 metres deep. One hypothesis has been that the missing water seeped into the crust. Mars was heavily bombarded by meteorites during the Noachian period, which may have formed fractures that channelled water underground. Deep beneath the surface, warmer temperatures would keep the water in a liquid state – unlike the frozen layers nearer the surface. A seismic snapshot of Mars' crust In 2018, Nasa's InSight lander touched down on Mars to listen to the planet's interior with a super-sensitive seismometer. By studying a particular kind of vibration called 'shear waves', we found a significant underground anomaly: a layer between 5.4 and 8 kilometres down where these vibrations move more slowly. This 'low-velocity layer' is most likely highly porous rock filled with liquid water, like a saturated sponge. Something like Earth's aquifers, where groundwater seeps into rock pores. We calculated the 'aquifer layer' on Mars could hold enough water to cover the planet in a global ocean 520–780m deep — several times as much water as is held in Antarctica 's ice sheet. This volume is compatible with estimates of Mars' 'missing' water (710–920m), after accounting for losses to space, water bound in minerals, and modern ice caps. Meteorites and marsquakes We made our discovery thanks to two meteorite impacts in 2021 (named S1000a and S1094b) and a marsquake in 2022 (dubbed S1222a). These events sent seismic waves rippling through the crust, like dropping a stone into a pond and watching the waves spread. InSight's seismometer captured these vibrations. We used the high-frequency signals from the events — think of tuning into a crisp, high-definition radio station — to map the crust's hidden layers. We calculated 'receiver functions,' which are signatures of these waves as they bounce and reverberate between layers in the crust, like echoes mapping a cave. These signatures let us pinpoint boundaries where rock changes, revealing the water-soaked layer 5.4 to 8 kilometres deep. Why it matters Liquid water is essential for life as we know it. On Earth, microbes thrive in deep, water-filled rock. Could similar life, perhaps relics of ancient Martian ecosystems, persist in these reservoirs? There's only one way to find out. The water may be a lifeline for more complex organisms, too – such as future human explorers. Purified, it could provide drinking water, oxygen, or fuel for rockets. Of course, drilling kilometres deep on a distant planet is a daunting challenge. However, our data, collected near Mars' equator, also hints at the possibility of other water-rich zones – such as the icy mud reservoir of Utopia Planitia. What's next for Mars exploration? Our seismic data covers only a slice of Mars. New missions with seismometers are needed to map potential water layers across the rest of the planet. Future rovers or drills may one day tap these reservoirs, analysing their chemistry for traces of life. These water zones also require protection from Earthly microbes, as they could harbour native Martian biology. For now, the water invites us to keep listening to Mars' seismic heartbeat, decoding the secrets of a world perhaps more like Earth than we thought. Hrvoje Tkalčić is a Professor, Head of Geophysics, and Director of Warramunga Array at Australian National University

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