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Astronomy / Space Science - 21.03.2023
Astronomy / Space Science - Earth Sciences - 15.03.2023
Astronomy / Space Science - Physics - 24.02.2023
Astronomy / Space Science - Physics - 15.02.2023
Astronomy / Space Science - 27.01.2023
Astronomy / Space Science - Chemistry - 24.01.2023
Astronomy / Space Science - Physics - 12.01.2023
Astronomy / Space Science - 06.01.2023
Astronomy/Space Science
Results 1 - 8 of 8.
Small stars may host bigger planets than previously thought
Stars with less than half the mass of our Sun are able to host giant Jupiter-style planets, in conflict with the most widely accepted theory of how such planets form, according to a new study led by UCL and University of Warwick researchers. Gas giants, like other planets, form from disks of material surrounding young stars.
Stars with less than half the mass of our Sun are able to host giant Jupiter-style planets, in conflict with the most widely accepted theory of how such planets form, according to a new study led by UCL and University of Warwick researchers. Gas giants, like other planets, form from disks of material surrounding young stars.
Scientists have new tool to estimate how much water might be hidden beneath a planet’s surface
In the search for life elsewhere in the scientists have traditionally looked for planets with liquid water at their surface. But, rather than flowing as oceans and rivers, much of a planet's water can be locked in rocks deep within its interior. We wanted to investigate whether these planets, after such a tumultuous upbringing, could rehabilitate themselves and go on to host surface water Claire Guimond Scientists from the University of Cambridge now have a way to estimate how much water a rocky planet can store in its subterranean reservoirs.
In the search for life elsewhere in the scientists have traditionally looked for planets with liquid water at their surface. But, rather than flowing as oceans and rivers, much of a planet's water can be locked in rocks deep within its interior. We wanted to investigate whether these planets, after such a tumultuous upbringing, could rehabilitate themselves and go on to host surface water Claire Guimond Scientists from the University of Cambridge now have a way to estimate how much water a rocky planet can store in its subterranean reservoirs.
Astronomers measure the heartbeat of spinning stars
An international team of scientist have used the MeerKAT radio telescope to observe the pulsing heartbeat of the universe as neutron stars are born and form swirling lightning storms which last for millions of years. Radio pulsars are spinning neutron stars from which we can observe flashes of radio waves in the manner of light pulses from a lighthouse.
An international team of scientist have used the MeerKAT radio telescope to observe the pulsing heartbeat of the universe as neutron stars are born and form swirling lightning storms which last for millions of years. Radio pulsars are spinning neutron stars from which we can observe flashes of radio waves in the manner of light pulses from a lighthouse.
First evidence that black holes are the source of dark energy
Observations of supermassive black holes at the centres of galaxies point to a likely source of dark energy - the 'missing' 70% of the Universe. The measurements from ancient and dormant galaxies show black holes growing more than expected, aligning with a phenomenon predicted in Einstein's theory of gravity.
Observations of supermassive black holes at the centres of galaxies point to a likely source of dark energy - the 'missing' 70% of the Universe. The measurements from ancient and dormant galaxies show black holes growing more than expected, aligning with a phenomenon predicted in Einstein's theory of gravity.
Meteorites reveal likely origin of Earth’s volatile chemicals
Meteorites have told researchers the likely far-flung origin of Earth's volatile chemicals, some of which form the building blocks of life. They found that around half the Earth's inventory of the volatile element zinc came from asteroids originating in the outer Solar System - the part beyond the asteroid belt that includes the planets Jupiter , Saturn , and Uranus.
Meteorites have told researchers the likely far-flung origin of Earth's volatile chemicals, some of which form the building blocks of life. They found that around half the Earth's inventory of the volatile element zinc came from asteroids originating in the outer Solar System - the part beyond the asteroid belt that includes the planets Jupiter , Saturn , and Uranus.
Space collaboration including Sussex scientist makes icy discovery which sheds light on the building blocks of life
In a development believed to shed light on the building blocks of life, an international team of scientists, including Prof Wendy Brown from the University of Sussex, has discovered diverse ices in the darkest, coldest regions of space so-far measured, which are around 500 light years from Earth. The discovery within a molecular cloud was made by scientists from the IceAge project, an international consortium of academics using the James Webb Space Telescope (JWST), to observe the building blocks of life.
In a development believed to shed light on the building blocks of life, an international team of scientists, including Prof Wendy Brown from the University of Sussex, has discovered diverse ices in the darkest, coldest regions of space so-far measured, which are around 500 light years from Earth. The discovery within a molecular cloud was made by scientists from the IceAge project, an international consortium of academics using the James Webb Space Telescope (JWST), to observe the building blocks of life.
Astronomical collaboration maps the structure of our Galaxy’s magnetic field
Almost a decade after starting observations of the sky in the northern hemisphere in the microwave range, the QUIJOTE Collaboration has presented the most accurate description we have of the polarisation of the emission of the Milky Way at these wavelengths. This is a window of observation not previously explored, which provides complementary information to that obtained previously by space mission (Planck and WMAP) dedicated to the study of the cosmic microwave background radiation (CMB), the fossil radiation left behind by the Big Bang.
Almost a decade after starting observations of the sky in the northern hemisphere in the microwave range, the QUIJOTE Collaboration has presented the most accurate description we have of the polarisation of the emission of the Milky Way at these wavelengths. This is a window of observation not previously explored, which provides complementary information to that obtained previously by space mission (Planck and WMAP) dedicated to the study of the cosmic microwave background radiation (CMB), the fossil radiation left behind by the Big Bang.
’little hurricanes’ to weigh and date planets around young stars
Little -hurricanes- that form in the discs of gas and dust around young stars can be used to study certain aspects of planet formation, even for smaller planets which orbit their star at large distances and are out of reach for most telescopes. It's extremely difficult to study smaller planets that are far away from their star by directly imaging them: it would be like trying to spot a firefly in front of a lighthouse.
Little -hurricanes- that form in the discs of gas and dust around young stars can be used to study certain aspects of planet formation, even for smaller planets which orbit their star at large distances and are out of reach for most telescopes. It's extremely difficult to study smaller planets that are far away from their star by directly imaging them: it would be like trying to spot a firefly in front of a lighthouse.