ESA's fourth Automated Transfer Vehicle, ATV Albert Einstein, is set to conduct an autonomous docking with the International Space Station on 15 June. The vessel will deliver scientific experiments, vital supplies and fuel to the astronauts.
ESA's Proba-V has become the first satellite to pick up aircraft tracking signals, allowing aircraft across the globe to be followed in flight from space.
Policy-makers and science and industry representatives are discussing how to make large amounts of Earth observation data accessible to a wider user community.
A new study into the behaviour of bubbles has been published based on a student experiment conducted as part of ESA Education's Drop Your Thesis! Programme. The results will be useful for understanding any system that uses fluids in space – including life support.
As cinema owners worldwide begin to embrace new digital technologies via satellite, audiences are being given more ways to enjoy an evening at the movies.
During ten seconds of weightlessness Brynle Barrett from the Laboratory of Photonics, Numerical Sciences and Nanosciences at the University of Bordeaux monitors an experiment to test the 'weak equivalence principle' – or why a feather in a vacuum falls as fast as a hammer.
To confirm that objects in free-fall behave universally, even at a microscopic level, a team of scientists used lasers to cool atoms to around –273°C. On Earth, atoms fall away from laser beams because of gravity. "In microgravity, atoms stay in the beams for much longer, so we get better data," explains Brynle.
Parabolic flights are the only way to run such experiments on humans without leaving Earth's atmosphere. Over the course of multiple roller-coaster flights at up to 45°, researchers find out more about the effects of gravity on experiments and improve equipment destined for space.
The module carrying the telescope and scientific instruments of ESA's Euclid 'dark Universe' mission is now being developed by Astrium in Toulouse, France.
Secondary-school students can play the ultimate robot game: the annual Zero Robotics tournament turns the International Space Station into a playing field for European students to control minisatellites with self-developed software.
ESA astronaut Luca Parmitano has been settling into life onboard the ISS, but still finding the time to tweet some of the amazing sights he is seeing from the orbital outpost.
Most recently, Luca spotted the island of Sicily in the Mediterranean sea. In this image, North is to the right, with the tip of Italy's 'boot', Calabria, visible in the bottom right.
For much more from Luca during his stay on the ISS, be sure to follow @astro_luca on Twitter, and check out the dedicated Flickr photostream for his mission Volare.
The face-on spiral galaxy M101, or the Pinwheel Galaxy, is seen at ultraviolet and optical wavelengths in this image taken by ESA's XMM-Newton space telescope.
The picture is composed of images taken by XMM-Newton's optical telescope using different filters: red (200–400 nm), green (200–300 nm) and blue (175–275 nm).
The contorted object captured by Hubble in this picture is IRAS 22491-1808, also known as the South America Galaxy. It is an ultraluminous infrared galaxy (ULIRG) that emits a huge amount of light at infrared wavelengths.
The reason for this intense infrared emission lies in an episode of strong star formation activity, which was set off by a collision between two interacting galaxies. In this image the twisted shape hides a number of features.
In the central region, which is very complex and disturbed, scientists have been able to distinguish two nuclei, remains of the two different galaxies that are currently colliding to form a new one. IRAS 22491-1808 is amongst the most luminous of these types of galaxies, and is considered to be mid-way through its merging stage.
The centre of this appealing object also shows several intense star-forming knots which, as seen in the picture, actually outshine the nuclei in optical wavelengths. To pick out the two merging nuclei in IRAS 22491-1808, scientists have had to observe it in infrared wavelengths, where they are more distinct. Other traces of the galactic collision are the three very noticeable tails in the image — two linear and one circular. The tail extending towards the bottom of the image from the main body exhibits a red clump of star formation at its base.