Very nice work. Gravitational lenses are amazing.
Some day in the not too distant future I would think maybe a look at the galaxy being lensed in some thing near to it’s actual structure might be possible.
WOW! Congrats to SpaceX for this first ever landing!
Perhaps you’ve heard about this possible impact with Jupiter which occurred on 17 March. Nobody is quite sure whether this was a comet or an asteroid but it seems something did impact Jupiter.
The video does a great job of showing some of the moons orbiting the planet too!
I am waiting for a local picture that might show this event and will share it when I get it.Hat tip to John Mckeon
The video depicts a demonstration of a series of flight test and maneuvers carried out at NASA’s Armstrong Flight research Center with the G-III aircraft as part of the Adaptive Compliant Trailing Edge experiments. While some of the inputs to the joystick and other flight controls may seem odd or harsh, they are needed to determine how this aircraft reacts with an experimental flap installed. Data is collected and displayed synchronized to the flight maneuvers.
Aurora occurrence on Jupiter has been known for a long time, now for the first time it is being studied in x-ray light. The press release below mentions a composite image, it was two shots of the auroral activity, click the image above to see the second picture.
Jupiter is pretty bright in the sky because we are just past the point were Earth and Jupiter are the closest we are in our orbits an event that happens about every 13 months.
Jupiter is an amazing planet and we are going to be seeing a lot more from it in the coming months as the spacecraft Juno nears the planet.
Here’s the press release from NASA:
Solar storms are triggering X-ray auroras on Jupiter that are about eight times brighter than normal over a large area of the planet and hundreds of times more energetic than Earth’s “northern lights,” according to a new study using data from NASA’s Chandra X-ray Observatory. This result is the first time that Jupiter’s auroras have been studied in X-ray light when a giant solar storm arrived at the planet.
The Sun constantly ejects streams of particles into space in the solar wind. Sometimes, giant storms, known as coronal mass ejections (CMEs), erupt and the winds become much stronger. These events compress Jupiter’s magnetosphere, the region of space controlled by Jupiter’s magnetic field, shifting its boundary with the solar wind inward by more than a million miles. This new study found that the interaction at the boundary triggers the X-rays in Jupiter’s auroras, which cover an area bigger than the surface of the Earth.
These composite images show Jupiter and its aurora during and after a CME’s arrival at Jupiter in October 2011. In these images, X-ray data from Chandra (purple) have been overlaid on an optical image from the Hubble Space Telescope. The left-hand panel reveals the X-ray activity when the CME reached Jupiter, and the right-hand side is the view two days later after the CME subsided. The impact of the CME on Jupiter’s aurora was tracked by monitoring the X-rays emitted during two 11-hour observations. The scientists used that data to pinpoint the source of the X-ray activity and identify areas to investigate further at different time points. They plan to find out how the X-rays form by collecting data on Jupiter’s magnetic field, magnetosphere and aurora using Chandra and ESA’s XMM-Newton.
A paper describing these results appeared in the March 22, 2016 issue of the Journal of Geophysical Research. The authors on the paper are William Dunn (UCL), Graziella Branduardi-Raymont (UCL), Ronald Elsner (NASA’s Marshall Space Flight Center), Marissa Vogt (Boston University), Laurent Lamy (University of Paris Diderot), Peter Ford (Massachusetts Institute of Technology), Andrew Coates (UCL), Randall Gladstone (Southwest Research Institute), Caitriona Jackman (University of Southampton), Jonathan Nichols (University of Leicester), Jonathan Rae (UCL), Ali Varsani (UCL), Tomoki Kimura (JAXA), Kenneth Hansen (University of Michigan), and Jamie Jasinski (UCL).
NASA’s Marshall Space Flight Center in Huntsville, Alabama, manages the Chandra program for NASA’s Science Mission Directorate in Washington. The Smithsonian Astrophysical Observatory in Cambridge, Massachusetts, controls Chandra’s science and flight operations.
Image credit: X-ray: NASA/CXC/UCL/W.Dunn et al, Optical: NASA/STScI
I almost missed this! Almost that is, my internet connection was out for a long time, and came back on just in time. If you missed the live version here is a quick replay from Science@NASA.
The internet connection, back in the nick of time!
My long time readers know of my infatuation with high altitude balloon missions. They are very cost effective method of quality astronomical observations. What balloon missions are not, is simple. It takes an immense amount of planning and technical expertise to run a mission.
Working on a balloon mission is one of those “bucket-list” items for me. Maybe someday.
Anyway, enough day-dreaming, if this new super pressure balloon works out, we could see payloads aloft for 100 days! We can follow the mission along no matter where we are. Those readers who live in the southern hemisphere’s mid-latitudes, such as New Zealand, Argentina, Australia and South Africa might get a look at the balloon during its travels near sunrise/sunset.
The NASA press statement:
After years of tests and development, NASA’s Balloon Program team is on the cusp of expanding the envelope in high-altitude, heavy-lift ballooning with its super pressure balloon (SPB) technology.
NASA’s scientific balloon experts are in Wanaka, New Zealand, prepping for the fourth flight of an 18.8 million-cubic-foot (532,000 cubic-meter) balloon, with the ambitious goal of achieving an ultra-long-duration flight of up to 100 days at mid-latitudes.
Launch of the pumpkin-shaped, football stadium-size balloon is scheduled for sometime after April 1, 2016, from Wanaka Airport, pending final checkouts and flight readiness of the balloon and supporting systems.
Once launched, the SPB, which is made from 22-acres of polyethylene film – similar to a sandwich bag, but stronger and more durable – will ascend to a nearly constant float altitude of 110,000 feet (33.5 km). The balloon will travel eastward carrying a 2,260-pound (1,025 kg) payload consisting of tracking, communications and scientific instruments. NASA expects the SPB to circumnavigate the globe once every one to three weeks, depending on wind speeds in the stratosphere.
“We are thrilled to be back in New Zealand for another test flight of this critical, potentially game-changing technology,” said Debbie Fairbrother, NASA’s Balloon Program Office chief. “This could be the flight for the record books.”
Up to a hundred days at float could shatter the current SPB flight duration record of 54 days, which occurred over Antarctica in 2009. To achieve this goal flying at mid-latitudes, where the balloon endures pressure changes due to the heating and cooling of the day-night cycle, the SPB flight must do what no other balloon has accomplished before.
Longer-duration flights enable longer observations of scientific phenomena, the ability to survey more sources, and more time to observe weak or subtle sources. In addition, mid-latitude flights are essential for making observations at night, a requirement for certain types of scientific investigations. These two aspects greatly enhance the return on science, and combined with the relatively low-cost of balloon missions, SPB could become a competitive platform for a number of scientific investigations that would otherwise need to launch into orbit.
A very cool view around the Mars Pathfinder & Sojourner rover. You just need to move the image around with your mouse.
Hopefully this will work for you, the caption mentioned: Not all browsers support viewing 360 videos/images. NOTE: it takes a few seconds to load, the title screen will disappear when ready.