ESA’s Solar Eclipse-Making Proba-3 Mmssion Head to India
ESA’s Proba-3 mission, designed to create solar eclipses in space to study the Sun’s corona, has officially left European soil and is en route to its launch site in India. This dual-spacecraft mission departed from Redwire Space’s facility in Kruibeke, Belgium, to travel to the Satish Dhawan Space Centre near Chennai, where the final launch preparations are set to begin. The mission’s objective is to enable extended observation of the Sun’s corona—something only briefly visible during natural eclipses on Earth—by creating an artificial eclipse in space.
Breakthrough Formation Flying for Solar Study
Proba-3, a pioneering European Space Agency mission, is comprised of two spacecraft: the Occulter and the Coronagraph. These satellites will achieve formation flying with a precision that allows one satellite to cast a shadow on the other, creating the eclipse effect needed for corona observation. According to ESA Mission Manager Damien Galano, achieving this feat has required years of work to ensure the satellites can operate autonomously in formation with an accuracy of just one millimetre. The mission aims to offer unprecedented insights into solar phenomena by capturing detailed views of the Sun’s outer atmosphere.
Launch Details and Technical Challenges
The Proba-3 mission is scheduled to launch aboard India’s PSLV-XL rocket on 4 December. This launch will place the spacecraft pair into a highly elliptical orbit, ranging from 600 km to 60,000 km above Earth. Such an orbit is essential to allow the spacecraft’s formation flying to occur at altitudes where gravity’s pull is lessened, reducing fuel consumption. After an initial setback with air freight arrangements, where the spacecraft’s batteries had to be shipped separately, the mission is now back on schedule.
Global Collaboration and Advanced Technology
The Proba-3 mission has drawn on expertise from across 14 ESA Member States and Canada. Led by Spain’s Sener and supported by Airbus Defence and Space, the project has involved partners such as GMV and Spacebel, specialising in satellite navigation and software. Key instruments include the ASPIICS corona-imaging device from Belgium’s Royal Observatory and the DARA radiometer from Switzerland’s Physical Meteorological Observatory, designed to study solar energy output.
Pre-launch Simulations Underway
Final mission control operations will be conducted at ESA’s European Space Security and Education Centre in Redu, Belgium. Rigorous simulations and training exercises are currently underway to prepare for Proba-3’s deployment and ongoing operations in space, marking a significant milestone in space-based solar observation.
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A team of U.S.-based astronomers is building a new kind of coronagraph — one powered by quantum mechanics — that could enable direct imaging of Earth-like exoplanets previously considered too faint or too close to their host stars to detect. Traditional telescopes have advanced since Galileo’s time, with instruments like the James Webb Space Telescope (JWST) now capable of analysing distant planetary atmospheres. But even these devices generally are not able to capture images of planets and asteroids that orbit nearby bright stars, as their light is frequently drowned out. Now, a breakthrough could be in sight.
Quantum-Sensitive Coronagraph May Revolutionize Exoplanet Imaging With Sub-Diffraction Precision
As per a recent Space.com report, researchers from the University of Arizona and the University of Maryland have developed a “quantum-sensitive” coronagraph that filters starlight before it reaches the telescope’s detector. By exploiting differences in the spatial modes of photons — how light waves behave in space — the device physically separates planetary light from overwhelming stellar glare. “This method routes photons to different regions before they even hit the sensor,” one co-author explained, emphasising its superiority to digital image processing.
This experimental device uses a “spatial mode sorter”, a series of precision-crafted optical phase masks that redirect light waves from exoplanets, allowing astronomers to view them below the diffraction limit. Normally, achieving this resolution would require telescopes too massive for current spaceflight capabilities. But quantum engineering may bypass that need altogether, provided that light purity — known as mode fidelity — reaches the stringent 1-in-a-billion requirement needed to block star photons while preserving exoplanet signals.
In lab tests, researchers successfully simulated star-planet systems and demonstrated that their system could resolve a dim, Earth-like planet even when positioned one-tenth the distance modern coronagraphs can handle. At higher star-to-planet contrast ratios — up to 1,000:1 — the device maintained accuracy within a few percentage points of theoretical limits, showcasing its potential for space-based observatories.
The technology could augment missions like NASA’s upcoming Habitable Worlds Observatory, designed to detect biosignatures on exoplanets. While scientists caution that the method isn’t a standalone solution, they believe it could dramatically expand the toolkit for planetary discovery. The findings were published on April 22 in Optica.
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Homo erectus, an extinct human ancestor is an important part of our evolutionary history. Emerging at least 2 million years ago, it was the first species to develop human-like body proportions and the first human species to migrate out of Africa, eventually finding its way to Southeast Asia. Homo erectus was first discovered in Java and was known as “Java Man” until the species was officially renamed. Long thought to have been isolated on the island of Java, two fossil fragments of a Homo erectus skull—which surfaced with recent ocean dredging in preparation for the construction of an artificial island—revealed that this hominin species migrated and spread throughout the islands when they could still walk over bridges of land.
The drowned Sundaland
According to four studies published in Quaternary Environments and Human, by archaeologist Harold Berghuis and his team, these lost lands, called drowned Sundaland, were once vast open plains interspersed with rivers around 140,000 years ago.
During the glacial period that chilled the Earth 140,000 years ago, sea levels in the Indonesian region of Sundaland were low enough for present-day islands to tower like mountain ranges with a lowland savannah stretching between them. It was an expanse of mostly dry grasslands with strips of forest edging the rivers, and animals like crocodiles, river sharks, elephants, hippos, rhinos, and Komodo dragons flourished in the region.
Hunting and Cultural exchanges
Berghuis and his team argue that these ancient rivers provided not just water, but sustenance through fruit-bearing trees, fish, shellfish, and edible plants. Tool marks on bones Fossils show that Homo erectus hunted river turtles and large terrestrial animals.
The hunting techniques observed, such as targeting animals in their prime, are typically associated with more modern humans, raising questions about whether this H. erectus group developed such strategies independently or learned them through cultural exchange with other human relatives like Denisovans or Neanderthals. H. erectus is believed to have survived on Java until about 117,000 years ago, well after it disappeared elsewhere in Asia.
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Fast Evolving X-ray Transients (FEXTs) are intense bursts of soft X-ray emissions that can last for minutes to hours with a wide range of luminosities. Due to their enigmatic nature, FEXTs have been a importance for scientists. Einstein Probe (EP) is one of the crucial space telescopes for the search and investigation of FEXTs. An international team of astronomers using the Einstein Probe reports the discovery of a new peculiar fast-evolving X-transient. The newfound transient exhibits an unprecedentedly long-lasting X-ray emission.
A Puzzling Long-Lived X-ray Transient
The finding was detailed in a paper published May 12 on the arXiv preprint server. According to the published paper, the newfound peculiar FEXT, dubbed EP241021a, was detected on Oct 21, 2024, with the help of EP’s wide-field X-ray telescope (WXT). EP241021a was identified by WXT as an intense flare, which lasted for approximately 92 seconds and reached a luminosity of about one quindecillion erg/s. The X-ray spectrum of the flare was found to be relatively hard with a photon index of 1.8.
The team of astronomers, led by Xinwen Shu of the Anhui Normal University in China, has concluded that EP241021a is an extremely unusual transient mainly due to its extended emission period. Follow-up observations of the flare up to 79 days after its detection revealed that its X-ray light curve shows a nearly plateau phase for the first 7 days, which is followed by a steep decline during the period of about 30 days. Afterward, the X-ray emission rapidly drops under the detection level.
The researchers also detected significant multiwavelength signals associated with EP241021a. About 1.8 days after the initial X-ray detection, optical emissions were also detected. This emission is likely connected to the flare’s afterglow.
Possible origins
The origin of FEXTs is puzzling. Astronomers try to explain their origin take into account several scenarios; for instance, stellar flares, supernova shock breakouts, or long gamma-ray bursts (GRBs).
Trying to explain the origin of EP241021a, the authors of the paper favor two scenarios. These are: a magnetar engine, involving a highly magnetized neutron star, or a jetted tidal disruption event (TDE), where a star is consumed by a black hole.
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