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The 11-Jupiter-mass exoplanet called HD106906 b occupies an unlikely orbit around a double star 336 light-years away and it may be offering clues to something that might be much closer to home: a hypothesized distant member of our Solar System dubbed “Planet Nine.” This is the first time that astronomers have been able to measure the motion of a massive Jupiter-like planet that is orbiting very far away from its host stars and visible debris disc.

The exoplanet HD106906 b was discovered in 2013 with the Magellan Telescopes at the Las Campanas Observatory in Chile’s Atacama Desert. However, astronomers did not then know anything about the planet’s orbit. This required something only the Hubble Space Telescope could do: collect very accurate measurements of the vagabond’s motion over 14 years with extraordinary precision.

Computer models of merging neutron stars predicts new signature in the gravitational waves to tell when this happens.

Neutron stars are among the densest objects in the universe. If our Sun, with its radius of 700,000 kilometers were a neutron star, its mass would be condensed into an almost perfect sphere with a radius of around 12 kilometers. When two neutron stars collide and merge into a hyper-massive neutron star, the matter in the core of the new object becomes incredibly hot and dense. According to physical calculations, these conditions could result in hadrons such as neutrons and protons, which are the particles normally found in our daily experience, dissolving into their components of quarks and gluons and thus producing a quark-gluon plasma.

This simulation shows the density of the ordinary matter (mostly neutrons) in red-yellow. Shortly after the two stars merge the extremely dense center turns green, depicting the formation of the quark-gluon plasma.

Invisible structures generated by gravitational interactions in the Solar System have created a “space superhighway” network, astronomers have discovered.

These channels enable the fast travel of objects through space, and could be harnessed for our own space exploration purposes, as well as the study of comets and asteroids.

By applying analyses to both observational and simulation data, a team of researchers led by Nataša Todorović of Belgrade Astronomical Observatory in Serbia observed that these superhighways consist of a series of connected arches inside these invisible structures, called space manifolds — and each planet generates its own manifolds, together creating what the researchers have called “a true celestial autobahn”.

**2021 Space Renaissance [Webinar Series “SPACE SAFETY”](https://spacerenaissance.space/event/webconference-on-space-safety-space-renaissance-congress-2021-civilian-space-development/)**

Sunday December 13th 16:00 UTC

Live streaming on [Facebook Space Renaissance Initiative Group](https://www.facebook.com/events/3842711565750385/)

**With**:

- tommaso sgobba, IAASS — space safety.

- jonathan tate, spaceguard UK — dangerous asteroids monitoring & defense.

- Joe Pelton, GALIX, former Director at International Space University — Space Weather.

- Luigina Feretti, INAF Italy — Protection from Cosmic Radiations.

- stefano antonetti, D-ORBIT italy — space debris.

**Moderates**: Adriano V. Autino, SRI, President.

**Call for Papers**

[Register for free to the Congress](https://2021.spacerenaissance.space/index.php/registration/), and [submit a paper abstract](https://2021.spacerenaissance.space/index.php/call-for-papers-abstract-submission/).

Forget what you thought you knew about the universe.


Embrace the flow, says a duo of mechanical engineers at North Carolina State University—the flow of energy, that is. The mantra you might normally hear from your yoga instructor could be an entirely new way of looking at the universe.

🌌The universe is badass. Let’s explore it together.