Category Astronomy/Space

Large, Distant Comets more Common than previously thought

A new study suggests that distant "long-period" comets -- which take more than 200 years to orbit the sun -- are more common than previously thought. This illustration shows how the researchers used data from NASA's Wide-field Infrared Survey Explorer (WISE) spacecraft to determine the nucleus sizes of several of these distant comets. They subtracted a model of how dust and gas behave in comets in order to obtain the core size. Credit: NASA/JPL-Caltech

A new study suggests that distant “long-period” comets — which take more than 200 years to orbit the sun — are more common than previously thought. This illustration shows how the researchers used data from NASA’s Wide-field Infrared Survey Explorer (WISE) spacecraft to determine the nucleus sizes of several of these distant comets. They subtracted a model of how dust and gas behave in comets in order to obtain the core size. Credit: NASA/JPL-Caltech

Comets that take more than 200 years to make one revolution around the sun are notoriously difficult to study. Because they spend most of their time far from our area of the solar system, many “long-period comets” will never approach the sun in a person’s lifetime...

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Venus’s turbulent atmosphere

1. The atmospheric superrotation at the upper clouds of Venus. While the superrotation is present in both day and night sides of Venus, it seems more uniform in the day (AKATSUKI-UVI image at 360 nm, right side), while in the night this seems to become more irregular and unpredictable (composite of Venus Express/VIRTIS images ar 3.8 μm, left). Credit: JAXA, ESA, J. Peralta (JAXA) and R. Hueso (UPV/EHU) 2. Examples of new types of cloud morphology discovered on the night side of Venus thanks to Venus Express (ESA) and the infrared telescope IRTF (NASA): stationary waves (Venus Express, up-left corner), "net" patterns (IRTF, up-right), mysterious filaments (Venus Express, down-left) and dynamical instabilities (Venus Express, down-right). CREDIT ESA, NASA, J. Peralta (JAXA) and R. Hueso (UPV/EHU)

1. The atmospheric superrotation at the upper clouds of Venus. While the superrotation is present in both day and night sides of Venus, it seems more uniform in the day (AKATSUKI-UVI image at 360 nm, right side), while in the night this seems to become more irregular and unpredictable (composite of Venus Express/VIRTIS images ar 3.8 μm, left). Credit: JAXA, ESA, J. Peralta (JAXA) and R. Hueso (UPV/EHU)
2. Examples of new types of cloud morphology discovered on the night side of Venus thanks to Venus Express (ESA) and the infrared telescope IRTF (NASA): stationary waves (Venus Express, up-left corner), “net” patterns (IRTF, up-right), mysterious filaments (Venus Express, down-left) and dynamical instabilities (Venus Express, down-right).
CREDIT: ESA, NASA, J. Peralta (JAXA) and R...

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Cosmologists Produce new Maps of Dark Matter Dynamics

Cosmologists produce new maps of dark matter dynamics

Slice through the celestial equator showing the radial component of the velocity field (in kilometres per second). Blue regions are falling towards us and red regions are flying away from us. Galaxies of the Sloan Digital Sky Survey main galaxy sample are overplotted. In the centre of the slice, the infalling dynamics of the Sloan Great Wall, one of the largest structure of the known universe, can be observed. Credit: University of Portsmouth

New maps of dark matter dynamics in the Universe have been produced by a team of international cosmologists.Using advanced computer modelling techniques, the team has translated the distribution of galaxies into detailed maps of matter streams and velocities for the first time...

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Turbulence in planetary cores excited by tides

© Thomas Le Reun / Institut de Recherche sur les Phénomènes Hors Equilibre (IRPHE, CNRS/Aix Marseille Université/Centrale Marseille).  Left: simulation of a cubic parcel located in the liquid core of a planet disturbed by tidal effects. By focusing their electronic analysis on this reduced domain, researchers have accessed regimes similar to planetary regimes. The flow takes the shape of superimposed waves that interact non-linearly until forming three-dimensional wave inertia turbulence (see vertical vorticity field in the center), by contrast with models where flow becomes larger-scale turbulence structures aligned with the axis of rotation (see vertical vorticity field on the right).

© Thomas Le Reun / Institut de Recherche sur les Phénomènes Hors Equilibre (IRPHE, CNRS/Aix Marseille Université/Centrale Marseille). Left: simulation of a cubic parcel located in the liquid core of a planet disturbed by tidal effects. By focusing their electronic analysis on this reduced domain, researchers have accessed regimes similar to planetary regimes. The flow takes the shape of superimposed waves that interact non-linearly until forming three-dimensional wave inertia turbulence (see vertical vorticity field in the center), by contrast with models where flow becomes larger-scale turbulence structures aligned with the axis of rotation (see vertical vorticity field on the right).

 
Veritable shields against high-energy particles, planets’ magnetic fields are produced by i...
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