Astronomy
World Asteroid Day 2025: Watch live views of near-Earth asteroids for free online on June 30
'Apollo 13' at 30: The space movie where scientists have the right stuff too
NASA exoplanet-hunting spacecraft and citizen scientists discover a cool new alien world
Cells Can ‘Hear’ Sounds—And Respond Genetically
Audible sound can affect gene activity in mouse cells, boosting the attachment of muscle precursors to surrounding tissue and decreasing fat accumulation
Why Did the Company behind the Dakota Access Pipeline Sue Greenpeace?
Energy Transfer, the company behind the Dakota Access Pipeline, sued the nonprofit Greenpeace over alleged conspiracy—the host of Drilled explains why
NASA budget cuts threaten Europe's already troubled flagship Mars rover
Plato’s eyes meet brain
On 11 June, engineers at OHB’s facilities in Germany joined together the two main parts of ESA’s Plato mission.
They used a special crane to lift Plato’s payload module, housing its 26 ultra-sensitive cameras, into the air and carefully line it up over the service module. The supporting service module contains everything else that the spacecraft needs to function, including subsystems for power, propulsion and communication with Earth.
With millimetre-level precision, the engineers gently lowered the payload module into place. Once perfectly positioned, the team tested the electrical connections.
Finally, they securely closed a panel that connects the payload module to the service module both physically and electronically (seen ‘hanging’ horizontally above the service module in this image). This panel, which opens and closes with hinges, also contains the electronics to process data from the cameras.
Now in one piece, Plato is one step closer to beginning its hunt for Earth-like planets.
In the coming weeks, the spacecraft will undergo tests to ensure its cameras and data processing systems still work perfectly.
Then it will be driven from OHB’s cleanrooms to ESA’s technical heart (ESTEC) in the Netherlands. At ESTEC, engineers will complete the spacecraft by fitting it with a combined sunshield and solar panel module.
Following a series of essential tests to confirm that Plato is fit for launch and ready to work in space, it will be shipped to Europe’s launch site in French Guiana.
The mission is scheduled to launch on an Ariane 6 in December 2026.
Access the related broadcast quality video footage.
ESA’s Plato (PLAnetary Transits and Oscillations of stars) will use 26 cameras to study terrestrial exoplanets in orbits up to the habitable zone of Sun-like stars.
Plato's scientific instrumentation, consisting of the cameras and electronic units, is provided through a collaboration between ESA and the Plato Mission Consortium. This Consortium is composed of various European research centres, institutes and industries, led by the German Aerospace Center (DLR). The spacecraft is being built and assembled by the industrial Plato Core Team led by OHB together with Thales Alenia Space and Beyond Gravity.
Webb spots a starburst shining in infrared
What Islands Can Teach Us About Planetary Protection
As Charles Darwin explored the Galapagos Islands, he discovered how the different islands allowed for different species to thrive. This is very similar to our current exploration of the Solar System; individual worlds, separated by the vacuum of space. The similarities provide a new insight into predictin planetary contamination risks and improve protection methods. A new paper by Daniel J. Brener and Charlesg S. Cockell uses the spread of life to new islands as a powerful model for rethinking how we prevent Earth's microbes from contaminating other worlds, shifting focus from probability calculations to whether microbes can actually survive in alien environments.
If We Can't Detect the First Stars, Maybe We Can See Their First Galaxies
Population III stars are the first generation that formed in the Universe, made from pristine hydrogen and helium, without any heavier "metals." They're difficult to find, surrounded by the early cosmic fog and lasting for only a few million years, but a new paper proposes that Webb could detect the pollution from these first stars as they're enriching the gas around them. There would be a hybrid phase when the first galaxies could contain second-generation stars and the polluted gas from the first stars.
Webb Could Detect if Supermassive Black Holes Formed Directly
An unfolding mystery is how early supermassive black holes got so big, so early. Their high mass is tough to explain through a ladder of mergers; instead, astronomers suggest they could have formed directly from huge clouds of gas. In a new paper, researchers propose the signals these directly-forming supermassive black holes might emit, and how they could even be detectable by James Webb before they collapse.
Flyby Mission Strategies for Detecting Oceans on Uranus’ Moons
What methods can be used to identify subsurface oceans on the five largest moons of Uranus: Ariel, Umbriel, Titania and Oberon, and Miranda? This is what a recent study presented at the 56th Lunar and Planetary Science Conference hopes to address as a team of scientists from NASA’s Jet Propulsion Laboratory (JPL) investigated potentially using radio science on the Uranus Orbiter and Probe (UOP) concept mission, which was designated as a high priority Flagship-class mission by the 2023–2032 Planetary Science Decadal Survey.
Altered gut microbiome linked to fertility issues in people with PCOS
Altered gut microbiome linked to fertility issues in people with PCOS
Planets Form Earlier Than Thought Around Baby Stars
The Sun and its planets formed out of the solar nebula, around 4.6 billion years ago. But what was the delay between the Sun's formation and the planets? Astronomers have surveyed 78 protoplanetary disks in the Ophiuchus star-forming region and seen examples of every step in the planetary formation process. They found that the planets start forming much earlier than previously believed, when the disk is still filled with gas and dust, growing together with their host stars.
Cryovolcanism and Resurfacing on Pluto’s Largest Moon, Charon
What processes during the formation of Pluto’s largest moon, Charon, potentially led to it having cryovolcanism, and even an internal ocean? This is what a recent study presented at the 56th Lunar and Planetary Science Conference hopes to address as a team of researchers investigated the formation and evolution of Charon to ascertain whether it once possessed an internal ocean during its history and if this could have led to cryovolcanism based on images obtained by NASA’s New Horizons probe.
New Propulsion Systems Could Enable a Mission to Sedna
The dwarf planet Sedna will reach its closest point to the Sun in 2075, the ideal time to send a mission to study this world that takes 11,000 years to orbit the Sun. In a new paper, researchers consider two exotic propulsion systems for a mission like this: a direct fusion drive, and an enhanced solar sail. Both methods could allow a spacecraft to reach Sedna in under a decade of flight time.