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

Monday, June 16, 2014

Amusingly Cryptic Warning Signs from NASA’s Jet Propulsion Laboratory, Autotuned

https://soundcloud.com/brainpicker/lazer-bypass-nasa-jpl

Warning signs from various locations around NASA's Jet Propulsion Laboratory, read and autotuned by Story Pirates artistic director Lee Overtree.

Background, photos, and full story here.

Shared with permission from NASA / David Delgado

Monday, February 20, 2012

UK NPL takes the lead in redefining the kilogram

New research, published by the UK's National Physical Laboratory (NPL), takes a significant step towards changing the international definition of the kilogram, which is currently based on a lump of platinum-iridium kept in Paris.

NPL has produced technology capable of accurate measurements of Planck's constant, the final piece of the puzzle in moving from a physical object to a kilogram based on fundamental constants of nature.

The techniques are described in a paper published in Metrologia on the 20th February.

The international system of units (SI) is the most widely used system of measurement for commerce and science. It comprises seven base units (metre, kilogram, second, Kelvin, ampere, mole and candela). Ideally these should be stable over time and universally reproducible, which requires definitions based on fundamental constants of nature. The kilogram is the only unit still defined by a physical artifact.

In October 2011, the General Conference on Weights and Measures (CGPM) agreed that the kilogram should be redefined in terms of Planck's constant (h). It deferred a final decision until there was sufficient consistent and accurate data to agree a value for h. This paper describes how this can be done with the required level of certainty.

It provides a measured value of h and extensive analysis of possible uncertainties that can arise during experimentation. Although these results alone are not enough, consistent results from other measurement institutes using the techniques and technology described in this paper will provide an even more accurate consensus value and a change to the way the world measures mass – possibly as soon as 2014.

Planck's constant is a fundamental constant of nature which relates the frequency (colour) of a particle of light (a photon) to its energy. By using two quantum mechanical effects discovered in the last 60 years: the Josephson effect and the quantum Hall effect, electrical power can be measured in terms of Planck's constant (and time).

A piece of kit called the watt balance - first proposed by Brian Kibble at the National Physical Laboratory in 1975 - relates electrical power to mechanical power. This allows it to make very accurate measurements of Planck's constant in terms of the SI units of mass, length and time.

The SI units of length and time are already fixed in terms of fundamental and atomic constants. If the value of h is fixed, the watt balance would provide a method of measuring mass.

Dr Ian Robinson, who leads the project at the National Physical Laboratory, explains how the watt balance works: "The watt balance divides its measurement into two parts to avoid the errors which would arise if real power was measured.

The principal can be illustrated by considering a loudspeaker placed on its back. Placing a mass on the cone will push it downwards and it can be restored to its former position by passing a current through the speaker coil.

The ratio of the force generated by the current is fixed for a particular loudspeaker coil and magnet and is measured in the second part of the experiment by moving the speaker cone and measuring the ratio of the voltage produced at the speaker terminals to the velocity of the cone.

When the results of the two parts of the experiment are combined, the product of voltage and current (electrical power) is equated to the product of weight and velocity (mechanical power) and the properties of the loudspeaker coil and magnet are eliminated, leaving a measurement of the weight of the mass which is independent of the particular speaker used."

Measurements of h using watt balances have provided uncertainties approaching the two parts in one hundred million level, which is required to base the kilogram on Planck's constant.

Thanks to improvements highlighted in the paper published today, measurements at the National Research Council in Canada, which is now using the NPL equipment, look set to provide considerably greater accuracy.

Another set of data comes from NIST, the USA's measurement institute. Currently the watt balance at NIST is showing slightly different results and the differences are being investigated. If the results are found to be consistent, it will be the start of the end for the physical kilogram.

A Planck based kilogram would mean a universal standard that could be replicated anywhere at any time. It will also bring much greater long-term certainty to scientists who rely on the SI for precise measurements, or on h itself. The watt balance would provide a means of realising and disseminating the redefined unit of mass.

Dr Robinson concludes: "This is an example of British science leading the world. NPL invented the watt balance and has produced an apparatus and measurements which will contribute to the redefinition. The apparatus is now being used by Canada to continue the work, and we anticipate their results will have lower uncertainties than we achieved, and the principle is used by the US and other laboratories around the world to make their own measurements."

"This research will underpin the world's measurement system and ensure the long term stability of the very top level of mass measurement. Although the man on the street won't see much difference - you'll still get the same 1kg bag of potatoes – these standards will ultimately be used to calibrate the world's weighing systems, from accurate scientific instruments, right down the chain to domestic scales."

Thursday, October 21, 2010

NASA Jet Propulsion LAb Webcam: Building Mars Rover Curiosity

Click on the picture to visit Curiosity Cam

Curiosity Cam takes you inside the clean room at NASA's Jet Propulsion Laboratory in Pasadena, Calif., so you can watch the next Mars rover being built.

Technicians assembling and testing the Mars Science Laboratory, aka Curiosity, are covered head-to-toe in "bunny suits."

These white smocks, booties and facemasks help protect against Earthly contaminants hitching a ride to Mars.

The camera may be turned off periodically for maintenance. The rover may occasionally be out of view as it is moved around the clean room. When Curiosity Cam is off air, you will see a slideshow of Mars and rover images.

Wheels Spinning


Engineers just installed six new wheels on the Curiosity rover, and rotated all six wheels at once on July 9, 2010.

This milestone marked the first in a series of "tune ups" to get the rover ready for a drive in the clean room where it is being assembled at NASA's Jet Propulsion Laboratory in Pasadena, Calif.

Curiosity is the centerpiece of NASA's Mars Science Laboratory mission, which is expected to launch in late 2011, and touch down wheels-first in summer 2012.

For more information about the mission, see: http://mars.jpl.nasa.gov/msl/.

Credit: NASA/JPL-Caltech

Wednesday, October 7, 2009

Nasa's Spitzer Space Telescope discovers Giant Ring around Saturn

Nasa's Spitzer Space Telescope has discovered the biggest but never-before-seen ring around the planet Saturn.

Jet Propulsion Laboratory said the ring lies at the far reaches of the Saturnian system and its orbit is tilted 27 degrees from the planet's main ring plane.

The ring is made of a thin array of ice and dust particles.


JPL spokeswoman Whitney Clavin said the ring is very diffuse and does not reflect much visible light but the infrared Spitzer telescope was able to detect it.

Although the ring dust is very cold - minus 316 degrees Fahrenheit - it shines with thermal radiation.

The bulk of the ring material starts about 3.7 million miles from the planet and extends outward about another 7.4 million miles.

Sunday, June 21, 2009

NASA reveals the South Pole of the Moon

The highest-resolution topography map to date of the Moon’s south pole has been generated by scientists at Nasa’s jet propulsion laboratory in Pasadena, Californina.

It uses data collected by the Deep Space Network’s Goldstone solar system radar located in the Mojave Desert and provides contiguous topographic detail over an areaof approximately 311 miles by 249 miles

NASA/AP

Thursday, May 28, 2009

Curiosity: NASA's next Mars Rover

Flagship Mars Rover Gets Name: Curiosity

NASA's next rover, the Mars Science Laboratory, finally has its new name: Curiosity.

The name comes courtesy of Clara Ma, a 12-year-old sixth-grade student at Sunflower Elementary school in Lenexa, Kan.

"We have been eager to call the rover by name," said Pete Theisinger, who manages the JPL team building and testing Curiosity. "Giving it a name worthy of this mission's quest means a lot to the people working on it."

The rover is expected to launch in 2011.

Friday, April 10, 2009

The wraps are off Kepler














NASA's planet hunting Kepler telescope launched March 6. Before it can find planets, its protective dust cover had to be jettisoned. that has been done, NASA announced yesterday.

"The cover released and flew away exactly as we designed it to do," said Kepler Project Manager James Fanson of NASA's Jet Propulsion Laboratory, Pasadena, Calif. "This is a critical step toward answering a question that has come down to us across 100 generations of human history รข€" are there other planets like Earth, or are we alone in the galaxy?"

Kepler's mission is to spend more than three years gazing at more than 100,000 stars in our Milky Way galaxy for signs of Earth-size planets. Some of the planets are expected to orbit in a star's "habitable zone," a warm region where water could pool on the surface.

The mission's science instrument, called a photometer, contains the largest camera ever flown in space. Its 42 charge-coupled devices (CCDs) will detect slight dips in starlight, which occur when planets passing in front of their stars partially block the light from Kepler's view.