Showing posts with label Jet Propulsion Laboratory. Show all posts
Showing posts with label Jet Propulsion Laboratory. Show all posts

Saturday, November 02, 2013

Project 1794/WS 606A, a/k/a The Avrocar: the U.S.-made UFO

By Jack Brummet, Alien Lore/UFO Ed.















The Avrocar in storage at the Smithsonian Institution in 1984. 

Project Project 1794/WS 606A, a/k/a The Avrocar, never really went anywhere or got past its early test phases.  In the end, it ended up being a hovercar proptotype.

The test models suffered from dangerous oil leaks that resulted in three fires, and eventually the staff were afraid of the machine, even when they were safely nestled in an observation booth of bullet-proof glass and quarter-inch-thick steel.   A final, and disastrous engine test in 1956 involved a Viper jet engine "running wild" and convinced the agencies involved that a less dangerous test vehicle was necessary.

A second Avrocar logged about 75 flight hours, but was also a failure; it couldn't lift itself safely more than a few feet off the ground, and its bulbous design  caused unbearable heat and screaming exhaust noise, which made it impractical for the military.  One person pointed out that, although it was a technical failure, its design was a rubber water skirt shy of being the world's first hovercraft










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Friday, August 01, 2008

Alien Lore No. 136::::::Water found!::::::Is there/was there life on Mars?

In a release yesterday by Dwayne Brown (NASA HQ), Guy Webster (Jet Propulsion Laboratory), and Sara Hammond (University of Arizona), NASA has confirmed finding water on the Planet Mars. The full release follows below.


July 31, 2008 - NASA Spacecraft Confirms Martian Water, Mission Extended
TUCSON, Ariz. -- Laboratory tests aboard NASA's Phoenix Mars Lander have identified water in a soil sample. The lander's robotic arm delivered the sample Wednesday to an instrument that identifies vapors produced by the heating of samples.

"We have water," said William Boynton of the University of Arizona, lead scientist for the Thermal and Evolved-Gas Analyzer, or TEGA. "We've seen evidence for this water ice before in observations by the Mars Odyssey orbiter and in disappearing chunks observed by Phoenix last month, but this is the first time Martian water has been touched and tasted."

With enticing results so far and the spacecraft in good shape, NASA also announced operational
funding for the mission will extend through Sept. 30. The original prime mission of three months ends in late August. The mission extension adds five weeks to the 90 days of the prime mission.

"Phoenix is healthy and the projections for solar power look good, so we want to take full advantage of having this resource in one of the most interesting locations on Mars," said Michael Meyer, chief scientist for the Mars Exploration Program at NASA Headquarters in Washington.

The soil sample came from a trench approximately 2 inches deep. When the robotic arm first reached that depth, it hit a hard layer of frozen soil. Two attempts to deliver samples of icy soil on days when fresh material was exposed were foiled when the samples became stuck inside the scoop. Most of the material in Wednesday's sample had been exposed to the air for two days, letting some of the water in the sample vaporize away and making the soil easier to handle.

"Mars is giving us some surprises," said Phoenix principal investigator Peter Smith of the University of Arizona. "We're excited because surprises are where discoveries come from. One surprise is how the soil is behaving. The ice-rich layers stick to the scoop when poised in the sun above the deck, different from what we expected from all the Mars simulation testing we've done. That has presented challenges for delivering samples, but we're finding ways to work with it and we're gathering lots of information to help us understand this soil."

Since landing on May 25, Phoenix has been studying soil with a chemistry lab, TEGA, a microscope, a conductivity probe and cameras. Besides confirming the 2002 finding from orbit of water ice near the surface and deciphering the newly observed stickiness, the science team is trying to determine whether the water ice ever thaws enough to be available for biology and if carbon-containing chemicals and other raw materials for life are present.

The mission is examining the sky as well as the ground. A Canadian instrument is using a laser beam to study dust and clouds overhead.

"It's a 30-watt light bulb giving us a laser show on Mars," said Victoria Hipkin of the Canadian Space Agency.

A full-circle, color panorama of Phoenix's surroundings also has been completed by the spacecraft.

"The details and patterns we see in the ground show an ice-dominated terrain as far as the eye can see," said Mark Lemmon of Texas A&M University, lead scientist for Phoenix's Surface Stereo Imager camera. "They help us plan measurements we're making within reach of the robotic arm and interpret those measurements on a wider scale."

The Phoenix mission is led by Smith at the University of Arizona with project management at NASA's Jet Propulsion Laboratory in Pasadena, Calif., and development partnership at Lockheed Martin in Denver. International contributions come from the Canadian Space Agency; the University of Neuchatel, Switzerland; the universities of Copenhagen and Aarhus in Denmark; the Max Planck Institute in Germany; and the Finnish Meteorological Institute.

For more about Phoenix, click here.
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Saturday, March 03, 2007

Fantastic new photos of Saturn from the Cassini-Huygens mission

All photography credits are NASA/Jet Propulsion Laboratory/Space Science Institute. The photos were all shot by the Cassini spacecraft a couple miles from Saturn (well, 800,000 miles, actually).


Click to enlarge - "Magnificent blue and gold Saturn floats obliquely as one of its gravity-bound companions, Dione, hangs in the distance. The darkened rings seem to nearly touch their shadowy reverse images on the planet below. This view looks toward the unlit side of the rings from about 9 degrees above the ring plane. The rings glow feebly in the scattered light that filters through them. Dione is 1,126 kilometers (700 miles) across. The image was taken in visible light with the Cassini spacecraft wide-angle camera on Feb. 4, 2007, at a distance of approximately 1.2 million kilometers (800,000 miles) from Saturn. Image scale is 75 kilometers (47 miles) per pixel. "


Click to enlarge - this clip from a movie sequence captures Saturn's rings "during a ring plane crossing--which Cassini makes twice per orbit--from the spacecraft's point of view. The movie begins with a view of the sunlit side of the rings. As the spacecraft speeds from south to north, the rings appear to tilt downward and collapse to a thin plane, and then open again to reveal the un-illuminated side of the ring plane, where sunlight filters through only dimly. "


click to enlarge - "Surely one of the most gorgeous sights the solar system has to offer, Saturn sits enveloped by the full splendor of its stately rings. Taking in the rings in their entirety was the focus of this particular imaging sequence. Therefore, the camera exposure times were just right to capture the dark-side of its rings, but longer than that required to properly expose the globe of sunlit Saturn. Consequently, the sunlit half of the planet is overexposed. Between the blinding light of day and the dark of night, there is a strip of twilight on the globe where colorful details in the atmosphere can be seen. Bright clouds dot the bluish-grey northern polar region here. In the south, the planet's night side glows golden in reflected light from the rings' sunlit face. "
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