OrbitalHub

NASA dixit:

“Astronomers studying the star RZ Piscium have found evidence suggesting its strange, unpredictable dimming episodes may be caused by vast orbiting clouds of gas and dust, the remains of one or more destroyed planets.

Young stars are often prodigious X-ray sources. Observations using the European Space Agency’s XMM-Newton satellite, show that RZ Piscium is, too. Its total X-ray output is roughly 1,000 times greater than our Sun’s. Ground-based observations show the star’s surface temperature to be about 9,600 degrees Fahrenheit (5,330 degrees Celsius), only slightly cooler than the Sun’s. They also show RZ Piscium is enriched in the tell-tale element lithium, which is slowly destroyed by nuclear reactions inside stars and serves as a clock indicating the elapsed time since a star’s birth.

Ground-based telescopes also reveal large amounts of dust and hydrogen-rich gas in the system, suggesting that large blobs of this material are orbiting the star and causing the brightness dips.

The best explanation that accounts for all of the available data, say the researchers, is that the star is encircled by debris representing the aftermath of a disaster of planetary proportions. It’s possible the star’s tides may be stripping material from a close substellar companion or giant planet, producing intermittent streams of gas and dust, or that the companion is already completely dissolved. Another possibility is that one or more massive gas-rich planets in the system underwent a catastrophic collision in the astronomically recent past.”

Music: “Frozen Wonder” from Killer Tracks

Video credit: NASA’s Goddard Space Flight Center/CI Lab

NASA dixit:

“Our solar system now is tied for most number of planets around a single star, with the recent discovery of an eighth planet circling Kepler-90, a Sun-like star 2,545 light years from Earth. The planet was discovered in data from NASA’s Kepler space telescope.

The newly-discovered Kepler-90i — a sizzling hot, rocky planet that orbits its star once every 14.4 days — was found by researchers from Google and The University of Texas at Austin using machine learning. Machine learning is an approach to artificial intelligence in which computers “learn.” In this case, computers learned to identify planets by finding in Kepler data instances where the telescope recorded signals from planets beyond our solar system, known as exoplanets.”

Video credit: NASA Ames Research Center

NASA dixit:

“NASA’s Parker Solar Probe is in the midst of intense environmental testing at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, in preparation for its journey to the Sun. These tests simulate the noise and shaking the spacecraft will experience during its launch from Cape Canaveral, Florida, scheduled for 2018.

Parker Solar Probe’s integration and testing team must check over the spacecraft and systems to make sure everything is still in optimal working condition after experiencing these rigorous conditions – including a check of the solar arrays, which will provide electrical power to the spacecraft.

Parker Solar Probe will explore the Sun’s outer atmosphere and make critical observations that will answer decades-old questions about the physics of stars. The resulting data will also help improve how we forecast major eruptions on the Sun and subsequent space weather events that can impact life on Earth, as well as satellites and astronauts in space. The mission is named for Eugene N. Parker, whose profound insights into solar physics and processes have helped shape the field of heliophysics.”

Joy Ng (USRA): Producer

Sarah Frazier (ADNET SYSTEMS): Writer

Lee Hobson (APL): Videographer

Music credit: ‘Push Away’ by Andrew Michael Britton [PRS], David Stephen Goldsmith [PRS], Mikey Rowe [PRS] from Killer Tracks.

Video credit: NASA’s Goddard Space Flight Center

ESA dixit:

“The teams involved in ESA’s Herschel space observatory reflect on the mission and its legacy. Herschel launched in May 2009 and studied the cool Universe in infrared and sub-millimetre wavelengths for nearly four years.

Highlights included surveying the glow of cold cosmic dust embedded in interstellar clouds of gas to unlock the secrets of star formation, and peering back in time to when the Universe was less than one billion years old to study galaxy evolution. The observatory also traced out the presence of water in star-forming clouds, detected it for the first time in the seeds of future stars and planets, and identified the delivery of water from interplanetary debris to planets in our Solar System.

Although the Herschel mission has now reached retirement, its legacy continues and it will remain a primary reference for astronomers for many years to come. “

Video credit: ESA

ESA dixit:

“It’s the perfect meeting of old and new. Astronomers have combined recent data from ESA’s Gaia mission with a simple analysis technique from the 18th century to discover a massive star cluster that had previously escaped detection. Subsequent investigations are helping to reveal the star-forming history of our Galaxy, the Milky Way. “

Video credit: ESA

ESA dixit:

“INTEGRAL (from INTErnational Gamma-Ray Astrophysics Laboratory) observes the ever-changing, powerful, and violent cosmos. It is the first space observatory that can simultaneously observe objects in gamma rays, X-rays, and visible light. The spacecraft travels in a geosynchronous highly eccentric orbit with high perigee in order to provide long periods of uninterrupted observation with nearly constant background and away from the radiation belts. Over time, the perigee and apogee have changed, as has the plane of the orbit.

In 2015, spacecraft operators conducted four thruster burns that were carefully designed to ensure that the satellite’s eventual entry into the atmosphere in 2029 will meet the Agency’s guidelines for minimising space debris. The orbital changes introduced during these manoeuvres are highlighted in blue. Making these disposal manoeuvres so early also minimises fuel usage, allowing ESA to exploit the satellite’s lifetime to the fullest.

By revealing both the diffuse emission from our Galaxy, the Milky Way, and the population of individual sources that shine brightly at these energies in our Galaxy and beyond, INTEGRAL has broadened our understanding of the high-energy Universe.”

Video credit: ESA/ScienceOffice.org