Indian Space Program: News & Discussions

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Europe Meets India Event Promotes GNSS Research, Industry

May 31, 2019 - By Inside GNSS

The European Union-funded GNSS.asia H2020 project hosted a major roundtable discussion around the theme of “Europe Meets India” at the recent 2019 Munich Satellite Navigation Summit. The event was aimed at promoting cooperation between the GNSS research and industrial communities in Europe and Asia-Pacific.

Speaking on behalf of the European Commission, Christoph Kautz, Deputy Head of Unit, Galileo Directorate, DG GROW, reaffirmed the EU’s commitment to partnering with India, as illustrated by the recent visit to India of Elzbieta Bienkowska, European Commissioner for Internal Market, Industry, Entrepreneurship and SMEs. Kautz also described the current operational status of the European satellite navigation programs, Galileo and EGNOS. There are now 26 Galileo satellites in orbit, 22 of which are fully operational. The constellation is set for completion by 2020, according to the European Global Navigation Satellite Systems Agency (GSA).

The keynote was delivered by Manish Saxena, Associate Director, Satellite Navigation Directorate, India Space Research Organization (ISRO). He talked about the Indian Regional Navigation Satellite System (IRNSS), also known as NavIC, which means “the sky” in Hindi. NavIC is an autonomous regional satellite navigation system that provides accurate real-time positioning and timing services. It covers India and a region extending more than 1,000 kilometers around it, with plans for further extension.

“One of our very important ultimate goals is to have NavIC available in mobile phones,” said Saxena, in an article published on the GSA website (http://www.gsa.europa.eu). “This will open up scope for many applications in a compact form factor and a convenient interface. This initiative needs to be pursued by developers to benefit the common citizens.”

Saxena pointed out that the recently unveiled Xiaomi MI8 smartphone is NavIC-enabled.
(Do what you want China, I'm not buying a Xiaomi, no amount of रिश्वत will change that.)

Meanwhile, India’s GAGAN is a satellite-based augmentation system (SBAS) for the Indian airspace. Its purpose is to serve safety-of-life civil aviation applications. The system has been successfully completed and is interoperable with other international SBAS systems, such as WAAS in the U.S., Europe’s EGNOS and the Japanese MSAS. GAGAN’s footprint extends from Africa to Australia and can be expanded for seamless SBAS navigation services across regions.

One of the key challenges for GAGAN, Saxena explained, is that India falls under equatorial regions, where ionospheric scintillation effects are most pronounced and can affect signal quality. Thus, the results of research work on these effects will be of interest to the wider GNSS community.

GSA Efforts

The important topic of “downstream ecosystem dynamics” was introduced by Martin Sunkevic, the GSA’s Market Development Officer. The GSA is responsible for market development and operations of Galileo and EGNOS. It publishes the GNSS Market Report and the GNSS User Technology Report, each of which presents trends and forecasting in their respective subject areas.

Among its other tasks, the GSA also supports research towards the development of new GNSS receivers and applications, and the creation of new business. “What’s really important for us right now is to create synergies with other space data,” said Sunkevic, “and to bring the GNSS industrial and research communities together to identify new downstream applications.”

Next to speak was SV Satish, Executive Director of Air Traffic Management for India’s Airport Authority. He discussed a range of new applications being made possible by the NavIC system, including helping fisherman to identify fishing zone boundaries, and for receiving targeted weather alerts. “There are various downstream applications that we can imagine for the common public,” Satish said. “This is a huge market. It will change agriculture. All application developers should be looking at this; India is a vast country, with oceans and mountains. So we have the marine field. There are definitely opportunities all over the place.”

More background on the European GNSS initiatives was provided by Thierry Racaud, CEO of the EGNOS Satellite Service Provider (ESSP). ”Our main mission is to act as the EGNOS service provider. The EGNOS contract is funded by the EU and managed through the GSA, and it gives us a clear mandate to help foster the use of satellite navigation within Europe and particularly in the domain of aviation,” he said.
In addition to EGNOS Services, ESSP delivers consultancy services for aviation, and global, satellite-based communication, navigation and surveillance (CNS) services for aviation.

Industry Stepping Forward

The GNSS.asia initiative brings together European and Asian GNSS and industrial communities with the aim of forming partnerships. European industry took the spotlight, in the persons of Philippe Badia, Business Development officer at Syntony; Alexander Rügamer, Group Leader at Fraunhofer IIS; Luis Serrano, Technical Marketing Manager at STMicroelectronics; and Petr Bares, CEO of Iguassu Software. Each of them delivered a brief pitch, explaining what their companies can do in the field of GNSS, and specifically what kinds of things they can offer in terms of cooperation with India and other Asian partners.

Also joining the “Europe meets India” roundtable event was Sanguk Lee of ETRI, based in Korea. ETRI is a global IT research institute that has been making an immense effort to stimulate growth in Korea in the field of IT. Indeed, Korea is the latest member of the international GNSS club, having just recently launched the new KPS (Korean Positioning System) program. Meanwhile, the EU-Korea Galileo Agreement has been in place since 2006. The Agreement provides for co-operative activities in the areas of scientific research and training, industrial cooperation, trade and market development, standards, certification and regulatory measures, regional and local augmentations, according to the GSA.
Lee presented the EU-funded STRIKE3 project, whose overall objective is to develop and validate new international standards for the monitoring, reporting and testing of GNSS threats. “We have particular problems in South Korea with hostile jamming and other issues,” said Lee. “International standards require international collaboration and international agreement. Moreover, such an ambitious task is only possible by bringing together existing organizations and technologies.”

For more details on the STRIKE3 project, read this GNSS Solutions column.

STRIKE3 will also provide a crucial new tool for police forces, highway authorities, toll operators, port authorities and governmental organizations, essentially creating an international task-force to defend against the criminal use of jamming technologies.

Supporting India

Closing remarks were delivered by Matthias Petschke, European Commission Director of European GNSS Programmes. “We see a huge potential and a very vibrant start-up scene in India,” he said. “The visit of Commissioner Bienkowska to India resulted in, among many other things, a new joint bilateral GNSS working group, which is very significant. So this is just the start of our bilateral relations and we look forward to our future cooperation.”

The EU-India exchange didn’t end there. The Indian delegation of course attended the Munich Satellite Navigation Summit, which opened in the same venue just after the “Europe Meets India” event ended and they also enjoyed industrial visits and Bavarian-style networking across the region on subsequent days.

Europe Meets India Event Promotes GNSS Research, Industry - Inside GNSS
 
AstroSat peers into the heart of Jellyfish galaxy

By Sarita Vig, Last Updated: Tuesday 04 June 2019

According to the authors, this galaxy is unique as it provides direct evidence of internal and external mechanisms at work to halt the formation of stars in the galaxy
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The Ultraviolet Imaging Telescope onboard India’s space observatory, AstroSat, has provided an insight into processes at work in the heart of a jellyfish galaxy.

Researchers who studied anatomy of a jellyfish galaxy, called JO201, have found that it comprises of a central bright region surrounded by a bright broken ring-like emission structure.

Ensconced in between is a cavity or void like region of rather faint ultraviolet emission. The ultraviolet light from the bright ring is due to young stars formed in the last 200 to 300 million years.

By comparing this with images from other telescopes at different wavebands, researchers have shown that the cavity is due to scarcity of young stars. This means no new stars have been formed in this cavity region for at least the last 100 million years.

Galaxies are very large aggregates of billions of stars held by the gravitation. Milky Way, our home galaxy is believed to house nearly ten billion stars with the Sun as one amongst them. On a larger scale, it has been found that even galaxies flock together due to gravity in groups of hundreds to thousands, known as galaxy clusters.

The region between these galaxies is filled with very hot gas whose temperature can be as high as millions of degrees. As a galaxy moves through this hot gas, some of the cold gas in the galaxy's outer regions can be pulled back, leading to formation of stars in structures that resemble tails or tentacles. This gives them the appearance of jellyfish, and hence, they are called jellyfish galaxies. One such jellyfish galaxy is JO201, which has been studied by astronomers from India and abroad as a part of an international collaboration called GASP.

“Galaxies come in two varieties — those that appear blue have young stars and are the star-forming variety, while red ones are those which have old stars and there has been no recent formation of stars in them,” explained K. George, who carried out the study at the Indian Institute of Astrophysics, Bangalore.

A blue galaxy can become red if it stops forming stars. Galaxies may stop forming stars due to various processes within the galaxy itself such as the effect of supermassive black hole at the centre; the presence of a rectangular bar-like structure which is made up of stars and located near the centre; or massive explosions accompanying stellar death called supernovae. The stripping of gas from the galaxy due to its motion in the hot gas between galaxies in a cluster could also impede the formation of stars.

Regarding the curbing of star-formation in this galaxy, researchers favour the hypothesis of the active galactic nucleus (AGN). Most large galaxies are believed to possess supermassive black-holes at their centres. The mass of these supermassive black holes could be hundreds of thousands to billions of times the mass of Sun. The gas and dust from the neighbourhood swirling at very high velocities into the supermassive blackhole increase the brightness of the central region multi-fold, and the galaxy is said to pass through an AGN phase.

In JO201, it is reported that the central region is bright in ultraviolet because of the AGN, and not due to young stars. The energy released from the AGN heats up cold gas clouds present close by. As stars are formed from cold gas clouds, this heating of gas leads to an arrest of star formation. This, in turn, results in a scarcity of young stars giving the galaxy a cavity-like appearance around the AGN.

The incomplete ring structure seen with lack of ultraviolet towards the left of the bright ring is explained due to the lack of young stars in this region. However, in this case, this cessation of star-formation is explained due to external effects, a result of gas being stripped out from this galaxy. Notice that this is the same side which has the tail like structure, far out in the galaxy.

According to the authors, this galaxy is unique as it provides direct evidence of internal and external mechanisms at work to halt the formation of stars in the galaxy.

The research results have been accepted for publication in the journal Monthly Notices of Royal Astronomical Society. The team included scientists from the GASP collaboration and the Indian Institute of Astrophysics. The picture of JO201 is the subject of the AstroSat Picture of the Month (APOM) series. AstroSat is India’s first multi wavelength observatory launched by the Indian Space Research Organisation in September 2015. (India Science Wire)

https://www.downtoearth.org.in/news...eers-into-the-heart-of-jellyfish-galaxy-64919
 
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Venus is Earth’s evil twin — and space agencies can no longer resist its pull

Once a water-rich Eden, the hellish planet could reveal how to find habitable worlds around distant stars.
By Shannon Hall, NEWS FEATURE, 05 June 2019
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Illustration by Jasiek Krzysztofiak/Nature; Source image: NASA/JPL-Caltech
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The helicopter fell like a stone. It dropped by more than 1,500 metres over Maryland, twisting slightly as the ground grew rapidly closer. Although this was all according to plan, that didn’t settle James Garvin’s nerves. Nor did the realization that his seat belt wasn’t fully fastened — a moment that sent his heart rate skyrocketing.

Then, a mere 6 metres above the ground, the ride got even wilder when the pilots pulled the aircraft out of the fall and climbed skywards, only to fall again. The helicopter dropped ten times that day. And each time, Garvin pointed a camera towards the ground through the open door in an attempt to measure the topography of a rock quarry below — from massive boulders to smooth sheets of sand. Although his interests were hardly terrestrial.

Garvin, the chief scientist at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, is the principal investigator on a proposed mission to Venus that would drop a probe through its atmosphere. That’s why he hired two pilots in August 2016 to plunge a helicopter towards the ground while he tested what a Venus probe might be able to photograph. The harrowing ride was worth it: researchers would love to get their hands on pictures of Venus with so much detail that the scenery would become familiar. “These images would be like you landing in your backyard,” he says.

Garvin is not the only scientist preparing such a daring mission. Nearly every space agency around the globe is currently sketching a proposal to explore our long-neglected neighbour (see 'The decade of Venus'). The Indian Space Research Organisation (ISRO) will be first to lift off when it launches an orbiter to Venus in 2023. The United States could follow close behind. Garvin and his colleagues are one of a handful of groups that will soon propose missions to NASA that, if selected, would take off in 2025. The European Space Agency (ESA) is currently considering a proposal to send an orbiter to Venus in 2032. And the Russian space agency Roscosmos is working in collaboration with the United States to send a daring mission to the planet any time from 2026 to 2033, which would include an orbiter, a lander that would send back short-term readings and a research station that would survive for much longer.

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Venus surface: NASA/JPL; Illustration by Jasiek Krzysztofiak/Nature

The new-found interest stands in stark contrast to the fact that nations have long overlooked Venus in favour of chasing Mars, asteroids and other planets. Over the past 65 years, for example, NASA has sent 11 orbiters and 8 landers to Mars, but just 2 orbiters to Venus — and none since 1994. This has not been for lack of scientific interest. Since the mid-1990s, US scientists alone have submitted nearly 30 Venus proposals to NASA. None has been approved.

But momentum is building to explore Venus, in part because scientists say it could hold the secret to understanding what makes a planet habitable. Once Earth’s twin, today Venus is a hellish abode where surface temperatures reach more than 400 °C, atmospheric pressures slam down with enough force to crush heavy machinery and clouds of sulfuric acid blow through the sky. If researchers could decipher why conditions on Venus turned so deadly, that would help them to assess whether life might exist on some of the thousand-plus rocky worlds that astronomers are discovering throughout the Galaxy.

As the scientific justification has grown for exploring Venus, planetary scientists are dreaming up new ways to study the planet and are building technology in the laboratory that can survive the horrendous conditions on its surface. And with India leading the way, there might soon be a parade of probes heading towards the second rock from the Sun.

“It might be the start of a new decade of Venus,” says Thomas Widemann, a planetary scientist at the Paris Observatory.

Double trouble

When humanity initially reached towards the stars, it ventured to Venus. Our neighbour was the target of the first successful interplanetary probe (United States, 1962); the first planet on which a mission crashed (Soviet Union, 1965); and the first alien world to host a successful landing (Soviet Union, 1970). It was during this space race to Venus that scientists discovered a torrid and toxic world (see 'Historical missions'). That could explain why interest in Venus dwindled. Scientists quickly realized that this planet would not be a home for future human exploration, nor an outlet on which to search for life. It would be downright difficult to study at all, even for short amounts of time.

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Source: NASA

And yet in so many ways — size, density, chemical make-up — Venus is Earth’s double. Recent research has even suggested that it might have looked like Earth for three billion years, with vast oceans that could have been friendly to life. “That’s what sets my imagination on fire,” says Darby Dyar, a planetary scientist at Mount Holyoke College in South Hadley, Massachusetts. “If that’s the case, there was plenty of time for evolution to kick into action.”

That could mean that Venus was (somewhat surprisingly) the first habitable planet in the Solar System — a place where life was just as likely to arise as it was on Earth. That alone is a reason to return to the former ocean world. “Why are we investing so much time looking for life on Mars when it only had liquid water for 400 million years?” Dyar asks. “And then there’s Venus with three billion years of water and no one loves her.”

Yet there’s no question that something went terribly wrong. Although Earth and Venus began in a similar fashion, the two have wandered down drastically different evolutionary paths — diverging perhaps as recently as 715 million years ago. That might seem like a reason not to visit, but scientists now argue that it makes the planet even more intriguing. If researchers could only understand what caused Venus to undergo such a deadly metamorphosis, they might gain a better understanding of what caused Earth to become such a haven for life.

“Venus plays a key role in understanding ourselves here — how life evolved on our own planet,” says Adriana Ocampo, science programme manager at NASA headquarters in Washington DC.

It is a crucial question now that astronomers have uncovered thousands of planets outside our Solar System — many of which are rocky worlds that orbit their stars at distances similar to those of Venus and Earth from the Sun. That means that many of these worlds could be Venus-like. “There is growing realization within the exoplanet community that Venus is the best analogue in the Solar System for many of the rocky exoplanets we have found,” says Laura Schaefer, an astronomer at Stanford University in California who studies exoplanets.

Off the radar

With such a tantalizing question left unanswered, it’s easy to see why ISRO’s return to Venus has created so much excitement. “I’m thrilled that ISRO is doing this,” Dyar says. “I’m thrilled that the international community is taking note of Venus and proposing missions. That’s fantastic.”

Although the ISRO mission is enveloped in a cloud of secrecy (Nature e-mailed and called project scientists dozens of times, to no avail), it’s clear that the agency plans to send an orbiter smothered in instruments. When ISRO announced the mission late last year, it published a list of a dozen instruments proposed by Indian scientists that have already been chosen — providing a sneak peek of the mission. Of those sensors, two will map the planet using radar, which is arguably the best method to peer through Venus’s dense clouds and trace its surface from orbit.

That said, ISRO is a relatively young space agency with a limited number of successful landings on the Moon and Mars. And, similar to programmes from other fledgling agencies, India’s first Venus mission might be a proof of concept that is less focused on science than on engineering. But given that even basic information on Venus is lacking, any small step will contribute to science.

One such contribution might be new maps of Venus’s surface features — a major step up, scientifically. The last mission to map the planet’s topography was NASA’s Magellan orbiter, which launched 30 years ago. Although those radar maps remain the foundation of Venusian geoscience today, they show topographic details at a horizontal resolution of just 10–20 kilometres per pixel, on average (the image resolution can be two orders of magnitude higher). With such limited topographic data, researchers have a blurry view of Venus’s geology — but the available maps do hint that plate tectonics might be kicking into action today (see 'Planetary facelift').

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Sources: Planetary facelift: NCEI/NOAA (Aleutian trench); NASA/JPL (Artemis corona); NASA/JPL (San Andreas fault).

That is particularly tantalizing, because many scientists think that tectonic activity is a crucial ingredient for life. Tectonic plates — those interlocking slabs of Earth’s crust that fit together like puzzle pieces — constantly move about, with some slipping below others and diving into the planet’s interior in a process called subduction. Over millions of years, that process has kept Earth from growing too hot or cold by cycling heat-trapping carbon dioxide between the atmosphere and the deep Earth. It acts as a natural thermostat, which might mean that fidgety planets are more likely to host life.

As such, scientists are eager to decipher the conditions that allow plate tectonics to arise. That is why Suzanne Smrekar, a planetary scientist at NASA’s Jet Propulsion Laboratory in Pasadena, California, has her eye on Venus — especially some spots that look eerily similar to locations on Earth where subduction is happening now. Scientists agree that subduction is the first step in the path towards plate tectonics, and yet there are no clear signs of large moving plates on Venus — at least not in the decades-old maps produced by Magellan. The San Andreas fault, which forms the tectonic boundary between Earth’s Pacific Plate and North American Plate, for example, varies in width from metres to a kilometre — too narrow to show up in Magellan topographic data.

But future maps might uncloak such tectonic features. Smrekar is the principal investigator on a potential mission, known as VERITAS, that she and her team will soon propose to NASA. The geophysical mission would use radar to map Venus’s topography in higher resolution than before — increasing the accuracy from roughly 15 kilometres to 250 metres — and allowing scientists to uncover features as small as the San Andreas fault for the first time.

Although scientists don’t know what they will find, it is possible that they will uncover evidence for past plate tectonics. Such a discovery would explain why Venus preserved an Earth-like environment for billions of years, Smrekar says — that natural thermostat would have kept CO2 in check. And it would explain how Venus turned hellish. When plate tectonics ceased, CO2 levels would have increased in the atmosphere and trapped so much heat that the oceans vaporized.

But that is only one possible finding. Some scientists are keen to study the planet’s atmosphere, which holds another, equally tantalizing set of secrets.

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A computer-generated view of the volcano Maat Mons on Venus (with an exaggerated vertical scale) shows dark lava flows in the foreground.NASA/JPL

The probe that Garvin is proposing, called DAVINCI, would drop through the atmosphere to measure the brew of toxic compounds. The isotopes of noble gases, particularly xenon, could give scientists a window into the planet’s volcanic history and reveal whether Venus started with as much water as Earth did. “Venus’s atmosphere is this lurking laboratory for telling us about its history,” Garvin says. “And really, most of the measurements in the atmosphere are woefully incomplete.” In addition, the probe would take images of the surface — thanks to Garvin’s terrifying helicopter flights — until the last few seconds before it hits.

Both VERITAS and DAVINCI will enter NASA’s competition on 1 July for future Discovery missions — a line of low-cost planetary probes that each cost just US$500 million. And rumour has it they’re not alone. There could be as many as five Venus missions (including a balloon) among the dozens of proposals to study various objects in space. NASA’s last Discovery competition, in 2015, for example, considered 27 proposals — from probes that would explore asteroids, moons and planets across the Solar System to telescopes that would image its outer reaches — before choosing two missions that would fly.

At the end of this year, the administration will select a few missions for further study, and it will pick the final project in two years’ time. Both Smrekar and Garvin are hopeful that each of their missions will be selected, in part because they proposed similar missions in the last Discovery competition, and both were chosen for further study, along with three others. If one of the Venus missions is successful, it will launch in the mid-2020s.

Even after that time frame, Venus might remain a hub for interplanetary activity. ESA recently picked a Venus probe called EnVision, along with two other finalists, as a mission that could fly as soon as 2032. Like VERITAS, EnVision is an orbiter. But unlike VERITAS, which would map the entire planet to a resolution of 15–30 metres, EnVision will analyse small portions of the planet with a resolution as high as 1 metre. At that level of accuracy, scientists might be able to see the landers that the Soviet Union left behind.

They could even pick out the type of rock that the landers are resting on. This is possible because astronomers in the early 1990s found that certain wavelengths of light can pass through the CO2 haze that hides the Venusian surface. An orbiter carrying a spectrometer tuned to these transparent ‘windows’ in the light spectrum could analyse the composition of the planet’s surface from above the clouds. That’s an exciting prospect, especially if scientists could spot granite.

Like basalt, granite forms when molten magma cools and hardens. But unlike basalt, the recipe for granite typically requires copious amounts of water — which happens on Earth when water-rich oceanic crust subducts below another plate. So if Venus is found to be rich in granite, it probably once overflowed with liquid water.

And that might be the best hint yet that the planet was formerly a pale blue dot vastly similar to Earth today — another clue in their diverging stories (see 'Water mystery').

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Source: Darby Dyar

The problem is that there are only five narrow spectral windows in Venus’s atmosphere that are actually transparent. With such little information, scientists weren’t sure whether they would be able to differentiate between granite and basalt. So Jörn Helbert, a planetary scientist at the Institute of Planetary Research in Berlin, subjected both types of rock to Venus-like conditions and imaged them through those narrow frequency bands. His experiment suggested that the two rock spectra look radically different from one another, and that future missions could make use of the windows. He and his colleagues built an instrument to use this trick to map any granite on the Venusian surface. It would fly on both VERITAS and EnVision.

Within reach

To truly understand the surface, a number of scientists want to actually land a craft on our toxic twin — a feat that has not been achieved for 35 years. Although the Soviet Union sent several landers to Venus, the ones that survived quickly succumbed to the planet’s harsh environment: the longest-lasting one persevered for a mere 127 minutes.

But scientists hope to break that record, and have already designed technology that can last not just minutes, but months. A team at NASA’s Glenn Research Center in Cleveland, Ohio, is building a station that should survive for at least 60 days. Instead of using its bulk to absorb heat or countering the conditions with refrigeration, the lander would use simple electronics made of silicon carbide (a hybrid of silicon and carbon commonly used in sandpaper and fake diamonds) that can withstand the Venusian environment. “That’s the real game changer for Venus exploration,” says Philip Neudeck, an electronics engineer at the Glenn Research Center.

The team has already tested the circuits in a Venus simulation chamber — a 14-tonne stainless-steel tank that can imitate the temperature, pressure and specific chemistry of the Venusian surface. The researchers have used those results to design a stationary surface probe called LLISSE (Long-Lived In-Situ Solar System Explorer), which should be ready for flight by the mid-2020s and will be offered to other countries. “Any mission to Venus is welcome to use LLISSE,” says electronics engineer Gary Hunter, also at the Glenn Research Center. He and the team were careful to design a lander that would be only as large as a toaster — making it both small and light enough that it can hitch a ride on a number of future missions.

Despite its small size, LLISSE would be able to record temperature, pressure, wind speed, wind direction, the amount of solar energy at the surface and a few specific chemicals in the low atmosphere. And it would do so for months, providing crucial input for models of the Venusian atmosphere. “Imagine if one tried to say one knew the weather on Earth by going outside for 127 minutes,” Hunter says. That is the current record for any weather data on Venus.

Already, scientists at Roscosmos are eager to use this new technology. In a joint proposal with NASA, they are working on a mission known as Venera-Dolgozhivuschaya (where the latter means long-lasting), or Venera-D for short. Such a mission would comprise a menagerie of components — an orbiter, a lander and a long-lived station. The lander would include a number of advanced instruments but would last for only a few hours; the long-lived station would be simpler in design but continue taking measurements for months. The station is likely to be NASA’s LLISSE.

At least, that’s the baseline architecture — but the mission could include even more. This year, the Venera-D team released a report that covered a number of potential additions, including a balloon that could explore the cloudy atmosphere. And that opens up the possibility of searching for life on Venus. All the other missions proposed so far aim to assess whether Venus was habitable in the past. But a balloon might be able to look for life in the only environment where it might survive today: the skies.

“You can imagine that there’s somewhere in between the hot hostile surface and the cold vacuum of outer space where there are conditions — like Goldilocks’ — that are just right for life,” Dyar says. Not only would that layer have a pleasant temperature, but it could also have nutrients, liquid water and energy from the Sun. If life ever existed on the planet, it might have been carried up to the clouds and survived there after the surface turned toxic.

But even without a balloon, the three main components of the Venera-D mission would provide excellent science, argues Ocampo. “It would be a breakthrough mission in the understanding of Venusian science,” she says. “We haven’t had a mission similar to this before.”

Unfortunately, Venera-D has not yet been selected, and many scientists have expressed some concern over the fact that it has long been discussed and yet still does not have the appropriate funding. But Ludmila Zasova, the lead scientist on the Venera-D mission at the Space Research Institute in Moscow, hopes that might change this year.

It’s not the only big ambitious mission in the works. Some US teams plan to submit Venus projects to NASA’s New Frontiers programme, which is capped at $1 billion, and to the Flagship mission programme, which costs even more. Because Venus proposals have done well in past competitions (often falling just behind the selected proposals), scientists think there is a good chance that they will now rise to the top.

With every space agency eyeing our neighbour, Venus is likely to receive a fleet of visitors over the next few decades. And although they all plan to address the question of habitability in one way or another, Garvin is convinced that whatever they find, it will be “beyond our wildest dreams”. Perhaps they will prove that Venus was formerly an ocean world. Or maybe they’ll discover that it’s tectonically active today. “We need to find out,” he says. “Because she’s waiting to tell us something and I would hate to miss the boat.”

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Venus is Earth’s evil twin — and space agencies can no longer resist its pull
 
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Indian experiments selected to fly on Chinese Space Station

No. 2: Spectroscopic Investigations of Nebular Gas (SING)
This is an experiment in astronomy in space. It was applied and will be implemented by two institutions from two countries, which are: The Indian Institute of Astrophysics, and the Institute of Astronomy of the Russian Academy of Sciences.

No.3: Behaviour of Partially Miscible Fluid in Microgravity
This is an experiment in microgravity fluid physics and combustion. It was applied and will be implemented by two organizations from two countries, namely the Indian Institute of Technology (BHU) and the University Libre de Bruxelles (ULB) in Belgium.

Experiments Selected for China’s Space Station (Updated with experiment list)
 
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