The close encounter between comet Siding Spring and Mars in October 2014 flooded the planet with an invisible tide of charged particles from the comet’s coma, according to data from NASA’s Mars Atmosphere and Volatile Evolution (MAVEN) spacecraft. The comet’s powerful magnetic field temporarily merged with, and overwhelmed, the planet’s weak field.
Astronomers have used computer simulations based on theoretical models to explain massive star formation observed in dwarf galaxies. Researchers in the US and the Netherlands found that during a dark matter satellite’s closest approach to a dwarf galaxy, through gravity it compresses the gas in the dwarf, triggering significant episodes of starbursts.
The Very Large Telescope Interferometer at ESO’s Paranal Observatory in Chile has obtained the sharpest view ever of the dusty disc around an ageing star. For the first time such features can be compared to those around young stars — and they look surprisingly similar. It is even possible that a disc appearing at the end of a star’s life might also create a second generation of planets.
Although thick cloud in parts of Indonesia spoiled the view for some along the path of totality, tens of millions more were greeted to spectacular views of the 9 March total solar eclipse. NASA, in partnership with the Exploratorium Science Center, hosted live coverage of the event from the coral island of Woleai in the Pacific Ocean.
Microscopic particles of stardust, known as “pre-solar grains,” have been found in meteoritic material on Earth. Researchers are investigating whether these particles may have formed in classical novae explosions, ejecting stellar material in the form of gas and dust into the space between stars in the galaxy, eventually to be recycled in the creation of our solar system.
The Moon will pass in front of the Sun on 9 March 2016 UT, casting its shadow over much of Southeast Asia. The path of totality, in which all of the Sun’s bright face is blocked by the Moon, is nearly 100 miles wide as it crosses Indonesia, while the partial phases can be seen from East Asia, Australia and the Pacific Ocean. Here is our detailed guide.
If you left it too late to book your Indonesian flight to view the total solar eclipse on the morning of Wednesday, 9 March (UT), don’t despair — put away your passport, sit back and enjoy the spectacle online, courtesy of Exploratorium and NASA TV. For virtual eclipse viewers in the UK, the event starts at 1am GMT on 9 March.
As the Moon slowly covers the face of the Sun on the morning of 9 March, a team of NASA scientists in Indonesia will be anxiously awaiting the start of totality. They plan to take 59 exposures of the Sun in just over three minutes, capturing data on the corona — the innermost parts of the Sun’s volatile, superhot atmosphere.
Scientists have long been puzzled about what makes Mercury’s surface so dark. The innermost planet reflects much less sunlight than the Moon, a body on which surface darkness is controlled by the abundance of iron-rich minerals. These are known to be rare at Mercury’s surface, so what is the “darkening agent” there?
© 2026 Nebula Press Ltd