Once again NASA has been caught shutting down a live transmission from the International Space Station (ISS) to hide evidence of aliens & UFOs in space. This time it appears NASA cut the live feed after a large four-armed UFO appeared in the video.
The incident adds to mounting evidence that despite denials, the agency maintains a rigid policy of non-disclosure of evidence of extraterrestrial life and intelligence. The latest UFO sighting was reported by Ufologist Streetcap1 on Thursday, October 20, The live video shows a strange craft loitering in the distance apparently monitoring the International Space Station. The strange craft has multiple arms extending from its main body.
The video shows sunlight reflecting from the body and arms of the UFO, causing it to glisten in deep space. The glistening of the mysterious object due to reflection of sunlight proves it was a real, solid, metallic object flying or hovering in space in the vicinity of the ISS. But as the UFO begins to glisten brightly in the sun, NASA interrupts transmission with its infamous blue screen.
Clouds on Pluto? Dwarf Planet’s Weather Gets Weirder
Scientists may have spotted more than a half dozen clouds in Pluto’s hazy atmosphere, researchers announced today (Oct. 18).
NASA’s New Horizons spacecraft flew by Pluto in July 2015, revealing a
bounty of unexpected details about the frozen world. For instance, the
mission discovered that Pluto possesses a complex, layered atmosphere.
“We’ve noticed a large number of concentric layers of haze, more than
two dozen,” New Horizons principal investigator Alan Stern, of the
Southwest Research Institute in Boulder, Colorado, said during a news
conference here at the 2016 American Astronomical Society’s Division of
Planetary Science meeting. “These haze layers stretch very high into the
sky — more than a half million feet, or 200 kilometers.” [Photos of Pluto and Its Moons]
Preliminary images of Pluto hinted at the presence of a cloud in the dwarf planet’s atmosphere. Now, Stern and his colleagues have revealed seven bright features that might be clouds in that world’s exotic skies.
Images: Scientists from NASA’s New Horizons mission have
identified some cloud candidates in the atmosphere of Pluto, using
images taken by the New Horizons Long Range Reconnaissance Imager and
Multispectral Visible Imaging Camera, during the spacecraft’s July 2015
flight through the Pluto system. None of the features can be confirmed
as clouds with stereo imaging, but the scientists say they are
suggestive of possible, rare condensation clouds. Credit: NASA/JHUAPL/SwRI
GOING OUT IN A BLAZE OF GLORY: CASSINI’S GRAND FINALE
With the conclusion of the international Cassini mission set for September 15, 2017, the spacecraft is poised to soon begin a thrilling two-part endgame.
Cassini will enter the first part of this denouement on November 30, 2016, when the spacecraft begins a series of 20 passes just beyond the outer edge of the main rings. These weekly loops around Saturn are called the F ring orbits, and they send the spacecraft high above and below the planet’s poles. During these orbits, Cassini will approach to within 4,850 miles (7,800 kilometers) of the center of the narrow F ring, with its wispy and ever-changing structure.
“During the F ring orbits we expect incredible views of the rings, along with the small moons and other structures embedded in them, as we’ve never seen them before,” said Linda Spilker, Cassini project scientist at NASA’s Jet Propulsion Laboratory, Pasadena, California. “The last time we got this close to the rings was during arrival at Saturn in 2004, and we saw only their backlit side. Now we have dozens of opportunities to examine their structure at extremely high resolution on both sides.”
Cassini’s final phase – called the Grand Finale – begins in earnest in April 2017. A close flyby of Saturn’s giant moon Titan will reshape the spacecraft’s orbit so that, instead of passing outside the rings, it passes through the gap between the rings and the planet. The spacecraft is expected to make 22 plunges through this gap – an unexplored space only about 1,500 miles (2,400 kilometers) wide – beginning with its first dive on April 27.
During the Grand Finale, Cassini will make the closest-ever observations of Saturn, mapping the planet’s magnetic and gravity fields with exquisite precision and returning ultra-close views of the atmosphere. Scientists also hope to gain new insights into Saturn’s interior structure, the precise length of a Saturn day, and the total mass of the rings – which may finally help settle the question of their age. The spacecraft will also directly analyze dust-sized particles in the main rings and sample the outer reaches of Saturn’s atmosphere – both first-time measurements for the mission.
The mission will come to a dramatic end on Sept. 15, 2017, after more than 13 years studying Saturn, its rings and moons – and nearly 20 years since launch. On that day, Cassini will dive into Saturn, returning data about the chemical composition of the planet’s upper atmosphere until its signal is lost, after which the spacecraft to burn up like a meteor.
“While it will be sad to say goodbye, Cassini’s final act is like getting a whole new mission in its own right,” said Spilker today at the joint 48th meeting of the American Astronomical Society’s Division for Planetary Sciences and 11th European Planetary Science Congress in Pasadena, California. “The scientific value of the F ring and Grand Finale orbits is so compelling that you could imagine an entire mission to Saturn designed around what we’re about to do.”
Martian ‘Spiders’ in Sharper Look, Thanks to Volunteers
This image shows spidery channels eroded into Martian ground. It
is an example from high-resolution observation of more than 20 places
that were chosen in 2016 on the basis of about 10,000 volunteers’
examination of lower-resolution images of larger areas near Mars’ south
These sharper looks use the High Resolution Imaging Science
Experiment (HiRISE) camera on NASA’s Mars Reconnaissance Orbiter. The
volunteers, through the Planet Four: Terrains website, categorize surface features in images from the same orbiter’s Context Camera (CTX).
This image is a portion of HiRISE observation ESP_047487_1005,
taken on Sept. 12, 2016, of a site at 79.4 degrees south latitude, 18.8
degrees east longitude. The ground area shown is about half a mile (0.8
This terrain type, called spiders or
“araneiform” (from the Latin word for spiders), appears in some areas of
far-southern Mars that are covered by sheets of frozen carbon dioxide
(“dry ice”) during the winter. When the slab ice thaws from the
underneath side in the spring, carbon dioxide gas trapped beneath the
ice builds pressure until it rushes toward a fissure or vent where it
bursts out. The venting gas carries dust and sand that it picks up as it
carves these channels.
At this location, the spiders are surrounded by ground called “basketball terrain” because of its texture.
and CTX are two of six instruments on the Mars Reconnaissance Orbiter,
which began examining Mars in 2006. The University of Arizona, Tucson,
operates HiRISE, which was built by Ball Aerospace & Technologies
Corp., Boulder, Colorado. NASA’s Jet Propulsion Laboratory, a division
of Caltech in Pasadena, California, manages the Mars Reconnaissance
Orbiter Project for NASA’s Science Mission Directorate, Washington.
Lockheed Martin Space Systems, Denver, built the orbiter and
collaborates with JPL to operate it. ~ NASA.gov
Titan, also known as the mermaid moon, is the largest satellite of Jupiter. It is the only known moon in our solar system that has a dense atmosphere, and the only object other than Earth where evidence of surface liquid has been found; however, the liquid on Titan is made of methane, not water.
We already estimated that there were about 100 billion galaxies in the observable universe, but new research shows that this estimate is at least 10 times too low!
First, what is the observable universe? Well, it is the most distant part of the universe we can see from Earth because, in theory, the light from these objects have had time to reach Earth.
In a new study using surveys taken by the Hubble Space Telescope and other observatories, astronomers came to the surprising conclusion that there are at least 10 times more galaxies in the observable universe than previously thought. This places the universe’s estimated population at, minimally, 2 trillion galaxies!
The results have clear implications for galaxy formation, and also helps shed light on an ancient astronomical paradox – why is the sky dark at night?
Most of these newly discovered galaxies were relatively small and faint, with masses similar to those of the satellite galaxies surrounding the Milky Way.
Using deep-space images from the Hubble Space Telescope and other observatories, astronomers converted the images into 3-D, in order to make accurate measurements of the number of galaxies at different epochs in the universe’s history.
In addition, they used new mathematical models, which allowed them to infer the existence of galaxies that the current generation of telescopes cannot observe. This led to the surprising conclusion that in order for the numbers of galaxies we now see and their masses to add up, there must be a further 90% of galaxies in the observable universe that are too faint and too far away to be seen with present-day telescopes.
The myriad small faint galaxies from the early universe merged over time into the larger galaxies we can now observe.
That means that over 90% of the galaxies in the universe have yet to be studied! In the near future, the James Webb Space Telescope will be able to study these ultra-faint galaxies and give us more information about their existence.
So back to the question…Why is the sky dark at night if the universe contains an infinity of stars? Researchers came to the conclusion that indeed there actually is such an abundance of galaxies that, in principle, every patch in the sky contains part of a galaxy.
However, starlight from the galaxies is invisible to the human eye and most modern telescopes due to other known factors that reduce visible and ultraviolet light in the universe. Those factors are the reddening of light due to the expansion of space, the universe’s dynamic nature, and the absorption of light by intergalactic dust and gas. All combined, this keeps the night sky dark to our vision.
The Butterfly Nebula from Hubble : The bright clusters and nebulae of planet Earths night sky are often named for flowers or insects. Though its wingspan covers over 3 light-years, NGC 6302 is no exception. With an estimated surface temperature of about 250,000 degrees C, the dying central star of this particular planetary nebula has become exceptionally hot, shining brightly in ultraviolet light but hidden from direct view by a dense torus of dust. This sharp close-up of the dying stars nebula was recorded in 2009 by the Hubble Space Telescopes Wide Field Camera 3, and is presented here in reprocessed colors. Cutting across a bright cavity of ionized gas, the dust torus surrounding the central star is near the center of this view, almost edge-on to the line-of-sight. Molecular hydrogen has been detected in the hot stars dusty cosmic shroud. NGC 6302 lies about 4,000 light-years away in the arachnologically correct constellation of the Scorpion . via NASA