Electron magnetic reconnection's scheme

An article published in the journal “Nature” describes the discovery of a new type of magnetic reconnection. A team of researchers used data collected by NASA’s Magnetospheric Multiscale (MMS) space probes to discover this phenomenon occurring in a boundary layer between the supersonic solar wind and the Earth’s magnetic field called magnetosheath. What was called electron magnetic reconnection is very different from the standard phenomenon and converts magnetic energy into high speed electron jets.

The Falcon 9 rocket with a Block 5 first stage blasting off (Image courtesy SpaceX. All rights reserved)

A few hours ago the Bangabandhu-1 was launched from Cape Canaveral on a Falcon 9 rocket with a first stage in its new version, called Block 5, at its debut. After about 33 minutes it separated from the rocket’s last stage and starte the series of maneuvers that will bring it into a geostationary orbit.

The Block 5 version of the first stage, also called a booster, includes a lot of improvements for the Falcon 9 rocket. SpaceX didn’t reveal all the details but a lot of information were provided by the company’s executives or leaked anyway. Various advancements concern performance, meeting NASA’s demands for manned launches, but above all with concern re-use possibilities, a crucial factor in Elon Musk’s company plans.

Artist's impression of 2004 EW95 (Image ESO/M. Kornmesser)

An article published in the journal “The Astrophysical Journal Letters” describes the study of an asteroid cataloged as 2004 EW95 which confirmed it has anomalous characteristics, being the first in the Kuiper belt to show a considerable carbon content. A team of astronomers used ESO’s VLT to study an asteroid that probably formed in the belt between Jupiter and Mars before being pushed to the outer solar system.

Diagram of solar Rossby waves (Image courtesy MPS/NASA/HormesDesign)

An article published in the journal “Nature Astronomy” describes the evidence of the presence of gigantic waves called Rossby waves on the Sun’s surface. A team of scientists led by the Max Planck Institute for Solar System Research (MPS) and the University of Göttingen discovered these vortices that have sizes comparable to those of the Sun itself, confirming a hypothesis that was proposed decades ago because they exist naturally in rotating fluids.

Artist's representation of WASP-96b (Image courtesy Engine House. All rights reserved)

An article published in the journal “Nature” describes a research on the exoplanet WASP-96b. It’s a hot Saturn, meaning a gas giant with a Saturn-like mass and an orbit close to its star which has as a consequece a high temperature on its surface. A team of researchers led by Nikolay Nikolov of the British University of Exeter used the FORS2 spectrograph mounted on ESO’s VLT to study WASP-96b discovering strong traces of sodium, an observation possible only in the absence of clouds in its atmosphere.