Einstein – Jupiter Broadcasting https://www.jupiterbroadcasting.com Open Source Entertainment, on Demand. Mon, 22 Feb 2016 02:46:30 +0000 en-US hourly 1 https://wordpress.org/?v=5.5.3 https://original.jupiterbroadcasting.net/wp-content/uploads/2019/04/cropped-favicon-32x32.png Einstein – Jupiter Broadcasting https://www.jupiterbroadcasting.com 32 32 Embarrassed Einstein | Tech Talk Today 182 https://original.jupiterbroadcasting.net/83632/embarrassed-einstein-tech-talk-today-182/ Thu, 11 Jun 2015 09:58:36 +0000 https://original.jupiterbroadcasting.net/?p=83632 Was “the biggest” recent government hack in history the result of out of date software & crappy detection systems? We share the details. Plus a look back at the best Star Trek games of all time, a browser extension that reads that Terms of Service for you & Kaspersky labs gets hacked! Direct Download: MP3 […]

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Was “the biggest” recent government hack in history the result of out of date software & crappy detection systems? We share the details.

Plus a look back at the best Star Trek games of all time, a browser extension that reads that Terms of Service for you & Kaspersky labs gets hacked!

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ISEE-3 Back To Life | SciByte 132 https://original.jupiterbroadcasting.net/58377/isee-3-back-to-life-scibyte-132/ Tue, 27 May 2014 21:27:19 +0000 https://original.jupiterbroadcasting.net/?p=58377 Hello everyone and welcome back to SciByte! We take a look at resurrecting a space probe, classroom decorations, brain control, viewer feedback, a three year look back at SciByte, Curiosity news, and as always take a peek back into history and up in the sky this week. Direct Download: MP3 Audio | OGG Audio | […]

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Hello everyone and welcome back to SciByte!

We take a look at resurrecting a space probe, classroom decorations, brain control, viewer feedback, a three year look back at SciByte, Curiosity news, and as always take a peek back into history and up in the sky this week.

Direct Download:

MP3 Audio | OGG Audio | HD Video | Video | Torrent | YouTube

RSS Feeds:

MP3 Feed | OGG Feed | Video Feed | Torrent Feed | iTunes

Show Notes:

Bringing an Abandoned Satellite Back to Life and Use

  • An independent team of engineers recovering old imagery on magnetic tape reels from the first lunar orbiter missions decided to accomplish a landmark achievement: to turn on, command and maneuver a NASA spacecraft long ago abandoned
  • Original mission : Sun/Earth Explorer 3 (ISEE-3)
  • Originally the mission was cooperative effort between NASA and ESRO/ESA to study the interaction between the Earth’s magnetic field and the solar wind.
  • Examine in detail the structure of the solar wind near the Earth and the shock wave that forms the interface between the solar wind and Earth\’s magnetosphere
  • Investigate motions of and mechanisms operating in the plasma sheets, and continue the investigation of cosmic rays and solar flare emissions in the interplanetary region near 1 AU
  • Second mission: International Cometary Explorer
  • On June 10, 1982, after completing its original mission, ISEE-3 was repurposed. It was renamed the International Cometary Explorer (ICE)
  • The primary scientific objective of ICE was to study the interaction between the solar wind and a cometary atmosphere
  • ICE carried no cameras. It instead carried instruments for measurements of energetic particles, waves, plasmas, and fields
  • It was sent on a trajectory intercepting that of Comet Giacobini-Zinner and on 11 September 1985, the craft passed through the plasma tail of Comet Giacobini-Zinner
  • It transited between the Sun and Comet Halley in late March 1986, when other spacecraft were in the vicinity of Comet Halley, ICE flew through the tail
  • Heliospheric mission
  • This phase of the mission was approved by NASA in 1991, which consisted of investigations of coronal mass ejections in coordination with ground-based observations
  • End of mission
  • On May 5, 1997, NASA ended the ICE mission, and ordered the probe shut down, with only a carrier signal left operating
  • Further contact
  • In 1999, NASA made brief contact with ICE to verify its carrier signal and discovered that it had not been powered off after the last contact
  • On September 18, 2008 a status check revealed that all but one of its 13 experiments were still functioning, and it still has enough propellant
  • Bringing It Back to Life?
  • Earlier in 2014, officials with the Goddard Space Flight Center had said that the Deep Space Network equipment necessary to transmit signals to the spacecraft had been decommissioned in 1999, and that replacing it was not economically feasible
  • An independent team of engineers recovering old imagery on magnetic tape reels from the first lunar orbiter missions decided to accomplish a landmark achievement: to turn on, command and maneuver a NASA spacecraft long ago abandoned
  • They began to study the feasibility and challenges involved in reviving the \’dead\’ satellite
  • A team webpage said, \”We intend to contact the ISEE-3 (International Sun-Earth Explorer) spacecraft, command it to fire its engine and enter an orbit near Earth, and then resume its original mission…If we are successful we intend to facilitate the sharing and interpretation of all of the new data ISEE-3 sends back via crowdsourcing.\”
  • Crowdsourcing
  • To cover the costs of writing the software to communicate with the probe, searching through the NASA archives for the information needed to control the spacecraft, and buying time on the dish antennas
  • On May 15, 2014, the project reached its crowdfunding goal, and they further met a \’stretch\’ goal of $150,000
  • Window of Opportunity
  • The team needed to contact the spacecraft before the end of May because the next close approach to the Earth won’t be until 30-40 years
  • The ISEE-3/ICE spacecraft was never really designed to be an interplanetary cruiser and thus the thrusters on board are very small
  • The project members are working on deadline: if they get the spacecraft to change its orbit by late May or early June 2014, it can use the Moon\’s gravity to get back into a useful halo orbit.
  • The team estimates that if they wait until mid-June to do the course correction that it will take 17 hours of thrusting to get the course change of about 40 meters/second that they will need at that time
  • Hardware and Software
  • It has been 30 years since the original project was started and and documents and magnetic tapes have disappeared.
  • The software and hardware to program, command and transmit to ISEE-3 are long gone
  • Amateur radio operators now have technology sufficient to acquire the signal and through the internet are also a part of the recovery effort
  • Even without the original hardware transmitter, today’s high-speed electronics are able to emulate in software the hardware from 36 years ago
  • Project members obtained the needed hardware (power amplifier, modulator/demodulator and installed it on the 305-meter Arecibo dish antenna on May 19, 2014
  • Technical Progress
  • This is an ongoing process and the team has dug some of the pertinent information out of 35 year old IEEE or AIAA papers that are publicly available
  • Most of the best information the team found was from the people who worked on the project in the 1980\’s when the spacecraft was fully operational
  • They also obtained several documents from NASA as part of the development of thier Space Act Agreement
  • Since there is no computer on board the ISEE-3 spacecraft the task is actually much easier since we are going to be directly commanding various subsystems
  • Non-Reimbursable Space Act Agreement
  • Although NASA is not funding the project, it made advisors available and gave approval to try to establish contact
  • On May 21, 2014, NASA announced that it had signed a Non-Reimbursable Space Act Agreement with the ISEE-3 Reboot Project
  • \”This is the first time NASA has worked such an agreement for use of a spacecraft the agency is no longer using or ever planned to use again,\” officials said
  • Multimedia
  • Twitter | ISEE3 Reboot Project (ISEE3Reboot)
  • YouTube | ISEE-3 Reboot | Mike Loucks
  • YouTube | ISEE-3 Reboot Project – Recovering a 30 year old space probe Scott Manley
  • Further Reading / In the News
  • NASA Signs Agreement with Citizen Scientists Attempting to Communicate with Old Spacecraft | NASA.gov
  • ISEE-3 Reboot Project Status and Schedule for First Contact | Space College
  • Guest Post: No turning back, NASA ISEE-3 Spacecraft Returning to Earth after a 36 Year Journey | UniverseToday.com
  • International Cometary Explorer – Wikipedia, the free encyclopedia
  • ISEE-3 Reboot Project | Astronomy News | NinePlanets.org
  • ISEE-3 Reboot Project: Stretch Goal – NASA Watch
  • ISEE-3 Reboot Project by Space College, Skycorp, and SpaceRef | RocketHub

— NEWS BYTE —

Distracted by Classroom Decorations?

  • New research from Carnegie Mellon University shows that too much materials covering a classroom wall may end up disrupting attention and learning in young children
  • The Low Down
  • Researchers looked at whether classroom displays affected children\’s ability to maintain focus during instruction and to learn the lesson content
  • They found that children in highly decorated classrooms were more distracted, spent more time off-task and demonstrated smaller learning gains than when the decorations were removed
  • The Study
  • 24 kindergarten students were placed in laboratory classrooms for six introductory science lessons on topics they were unfamiliar with
  • Three lessons were taught in a heavily decorated classroom, and three lessons were given in a sparse classroom.
  • Results
  • The results showed that while children learned in both classroom types, they learned more when the room was not heavily decorated
  • Children\’s accuracy on the test questions was higher in the sparse classroom (55 percent correct) than in the decorated classroom (42 percent correct).
  • When the researchers tallied all of the time children spent off-task in both types of classrooms, the rate of off-task behavior was higher in the decorated classroom (38.6 percent time spent off-task) than in the sparse classroom (28.4 percent time spent off-task)
  • The Future
  • The researchers are interested in finding out if the visual displays were removed, whether the children\’s attention would shift to another distraction
  • Additional research is needed to know what effect the classroom visual environment has on children\’s attention and learning in real classrooms
  • They say that they do not suggest by any means that this is the answer to all educational problems but that teachers should consider whether some of their visual displays may be distracting
  • Further Reading / In the News
  • Heavily decorated classrooms disrupt attention and learning in young children | ScienceDaily.com

— TWO-BYTE NEWS —

Flying With Only A Thought

  • Scientists have now demonstrated the feasibility of flying via brain control, with astonishing accuracy
  • First Breakthrough
  • Seven subjects took part in the flight simulator tests
  • They had varying levels of flight experience, including one person without any practical cockpit experience whatsoever
  • The accuracy with which the test subjects stayed on course by merely thinking commands would have sufficed, in part, to fulfill the requirements of a flying license test
  • Several of the subjects also managed the landing approach under poor visibility
  • In The Future
  • Scientists are now focusing in particular on the question of how the requirements for the control system and flight dynamics need to be altered to accommodate the new control method
  • Normally, pilots feel resistance in steering and must exert significant force when the loads induced on the aircraft become too large
  • This feedback is missing when using brain control
  • The researchers are thus looking for alternative methods of feedback to signal when the envelope is pushed too hard, for example
  • Further Reading / In the News
  • Using thoughts to control airplanes | ScienceDaily.com

— VIEWER FEEDBACK —

Jupiter\’s Great Red Spot Shrinking?

  • Twitter | Michael Thalleen ‏@ThalleenM
  • Jupiter\’s Great Red Spot Shrinks to Smallest Size Ever Seen
  • The Great Red Spot
  • “Recent Hubble Space Telescope observations confirm that the spot is now just under 10,250 miles (16,500 km) across, the smallest diameter we’ve ever measured,” said Amy Simon of NASA’s Goddard Space Flight Center
  • Using historic sketches and photos from the late 1800s, astronomers determined the spot’s diameter then at 25,475 miles (41,000 km) across
  • Changes
  • Starting in 2012 amateur observations revealed a noticeable increase in the spot’s shrinkage rate
  • They showed that the spot’s “waistline” is getting smaller by just under 620 miles (1,000 km) per year while its north-south extent has changed little
  • This has caused the spot to become more circular in shape
  • Cause
  • There are no firm answers yet as to what is causing the drastic downsizing,
  • New observations however show that very small eddies are feeding into the storm which may be responsible for the accelerated change by altering the internal dynamics of the Great Red Spot
  • The storm appears to be conserving angular momentum by spinning faster the same way an ice skater spins up when they pulls in their arms
  • The faster winds might also help shrink the spot further or bring about its rejuvenation.
  • Multimedia
  • YouTube | Jupiter\’s Great Red \’Shrinking\’ Spot Spied By Hubble | VideoFromSpace
  • Further Reading / In the News
  • [Hubble Sees Jupiter\’s Red Spot Shrink to Smallest Size Ever | UniverseToday.com(https://www.universetoday.com/111907/hubble-sees-jupiters-red-spot-shrink-to-smallest-size-ever/)

— Updates —

SciByte

  • Hosts
  • Jeremy | Co-Hosted for ep 1-13
  • Nikki | Summer SciByte | August 06, 2013; August 13, 2013; August 27, 2013; July 23, 2013; SciByte September 03, 2013
  • Chris | Episodes 14+ [minus a few \”Summer SciByte\” or \”Summer SciByte Style\” with Nikki]
  • Formats Over the Years
  • Totally edited video in a virtual studio with Jeremy
  • Totally video in a virtual studio with Chris
  • Video once a month and \”Enhance Audio\” with Chris
  • \”Enhanced Audio\” with Chris
  • Google Hangout\’s with Nikki
  • Science as an Adjective, a Noun, and a Verb
  • Adjective = \’describing\’ a word; Noun = person, place, thing, animal, idea; Verb = conveys an action
  • \”Science is Sad\” | Large Hadron Collider | SciByte 8
  • Watching Science Progres
  • Private Space Travel Advances | From an idea, to engineering, to testing, to implementation [i.e. SpaceX and Virgin Galactic]
  • Mars Landers | Opportunity (continuing science and solar panel ‘cleaning’ events) and Curiosity (Confirmation of running/standing water in Mars history, ancient habitable locations, drilling into rocks, switching to searching for the building blocks of life)
  • Watching science progress | Alzheimer\’s research, Voyager 1, Exoplanets, medical research helping senses
  • Breaking Science | \’Faster Than Light Neutrinos\’, Higgs-Boson Particle
  • Further Reading / In the News
  • SciByte | JupiterBroadcasting.com

— CURIOSITY UPDATE —

  • The Image from Mars Hand Lens Imager (MAHLI)
  • Shows the rock target \”Windjana\” and its immediate surroundings after inspection of the site by the rover
  • The researchers drilled a test hole and a sample collection hole produced the mounds of drill cuttings that are markedly less red than the other visible surfaces
  • This preparatory \”mini drill\” hole, to lower right from the open hole, was drilled on Sol 615 (April 29, 2014) and subsequently filled in with cuttings from the sample collection drilling.
  • The open hole from sample collection is 0.63 inch (1.6 centimeters) in diameter. It was drilled on Sol 621 (May 5, 2014).
  • The vigorous activity of penetrating the rock with the rover\’s hammering drill also resulted in slides of loose material near the rock
  • Gathering Samples
  • Since then, the 1 ton robot carefully scrutinized the resulting 2.6 inches (6.5 centimeters) deep borehole, the scientists then hit the fresh bore hole with a pinpoint series of parting laser blasts
  • The mound of dark grey colored drill tailings, much darker and greyer that the exterior of the rock, that are piled around for an up close examination of the texture and composition with the MAHLI camera and spectrometers
  • The team has successfully delivered pulverized and sieved samples to the pair of onboard miniaturized chemistry labs [Chemistry and Mineralogy instrument (CheMin) and Sample Analysis at Mars instrument (SAM)] for chemical and compositional analysis.
  • Researchers decided that one drill campaign into Kimberley was enough, so the rover will not be drilling into any other rock targets at this location
  • There will be further analysis of the ‘Windjana’ sample along the way since there’s plenty of leftover sample material stored in the CHIMRA sample processing mechanism to allow future delivery of samples when the rover periodically pauses during driving.
  • The Future
  • It may be a very long time before the next drilling when the rover arrives at the foothills of Mount Sharp
  • The current location, Windjama, lies some 2.5 miles (4 kilometers) southwest of Yellowknife Bay
  • It still has about another 4 kilometers to go to reach the foothills of Mount Sharp sometime later this year
  • Multimedia
  • Images – Mars Science Laboratory | mars..jpl.nasa.gov
  • Image Galleries at JPL and Curiosity Mulimedia
  • Social Media
  • Curiosity Rover @MarsCuriosity
  • Further Reading / In the News
  • Curiosity says \’Goodbye Kimberley\’ after Parting Laser Blasts and Seeking New Adventures Ahead | UniverseToday.com

SCIENCE CALENDAR

Looking back

  • May 29, 1919 : 95 years ago : Einstein\’s Relativity Theory Proved : A solar eclipse permitted observation of the bending of starlight passing through the sun\’s gravitational field, as predicted by Albert Einstein\’s theory of relativity. Separate expeditions of the Royal Astronomical Society travelled to Brazil and off the west coast of Africa. Both made measurements of the position of stars visible close to the sun during a solar eclipse. These observations showed that, indeed, the light of stars was bent as it passed through the gravitational field of the sun. This was a key prediction of Albert Einstein\’s theory that gravity affected energy as in addition to the familiar effect on matter. The verification of predictions of Einstein\’s theory, proved during the solar eclipse was a dramatic landmark scientific event.

Looking up this week

  • Keep an eye out for …
  • Wed, May 28 | New Moon (exact at 2:40 p.m. EDT)
  • Fri, May 30 | 20-30 min after sunset | | Very low in the W-NW you can see the hairline crescent Moon with Mercury to its right, they both set fairly quickly. You can see Jupiter to the far upper left.
  • Sat, May 31 | ~1hr after sunset | Jupiter stands to the upper right of the Moon in the early evening
  • Sun, Jun 03 | ~1hr after sunset | Jupiter is now to the left and slightly higher than the moon
  • Planets
  • Mercury | Twilight | It is at it\’s highest point for 2014 for mid-N lat, and is fading this week. As twilight deepens, look for it in the W-NW to the lower right of bright Jupiter as it fades this week
  • Venus | Dawn | The \”Morning Star\” is low in the E during dawn, moving to it\’s highest point in the south in late twilight
  • Mars | Is at it\’s highest point in the S in late twilight, it sets in the W around 3 or 4 a.m. DST
  • Jupiter | Twilight | Is in the west at twilight, sinking during the evening and sets around 11 or midnight. Jupiter is on the far side of the Sun from us and is nearly its minimum apparent size that we see
  • Saturn | Evening | Appears SE in the evening moving to it\’s highest point in the S ~11-12

  • Further Reading and Resources

  • Sky&Telescope | Sky at a Glance
  • SpaceWeather.com
  • StarDate.org
  • For the Southern hemisphere: SpaceInfo.com.au
  • Constellations of the Southern Hemisphere : astronomyonline.org
  • Royal Astronomical Society of New Zealand : rasnz.org.nz
  • AstronomyNow
  • HeavensAbove

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Apollo 11 & James Cameron | SciByte 40 https://original.jupiterbroadcasting.net/18543/apollo-11-james-cameron-scibyte-40/ Tue, 03 Apr 2012 22:33:51 +0000 https://original.jupiterbroadcasting.net/?p=18543 We take a look at recovering Apollo 11 hardware, James Cameron's ocean dive, sprinting planets, Lego science, coffee, Hubble image competition, and more!

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We take a look at recovering Apollo 11 hardware, James Cameron’s ocean dive, sprinting planets, Lego science, coffee, Einstein’s writings, Hubble image competition, viewer feedback and as always take a peek back into history and up in the sky this week.

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Show Notes:

Apollo 11 Engines found at the bottom of the ocean

*— NEWS BYTE — *

James Cameron dives deep

*— TWO-BYTE NEWS — *

Runaway planets

  • The low down
  • In 2005, astronomers found evidence of a runaway star that was flying out of the Milky Way galaxy at a speed of 1.5 million mph (2.4 million kph).
  • In the seven years since, 16 of these hypervelocity stars have been found
  • Significance
  • A new study has found that planets themselves could be ejected from their star, and even escaping the Milky Way at a speedy to 30 million miles per hour, or a fraction of the speed of light
  • A typical runaway planet would likely dash outward at 7 to 10 million mph (11.3 to 16.1 million kph),
  • Under the right circumstances, a few could have their speeds boosted to up to 30 million mph (48.3 million kph)
  • At those speeds they could be the fastest large solid objects, and could cross the diameter of the Earth in 10 sec
  • These hypervelocity planets could escape the Milky Way and travel through interstellar space
  • * Of Note*
  • Planets that are in tight orbits around a runaway star could travel with them, and be visible from dimming as it transits
  • This is the first time that scientists are discussing searching for planets around hypervelocity stars
  • Further Reading / In the News
  • ‘Warp-Speed’ Planets Flung Out of Galaxy on Wild Ride @ space.com

Lego’s can help build bones too

  • The low down
  • Bone has excellent mechanical properties for its weight
  • Synthetic bone has a range of applications; from the obvious, such as medical implants, to a material used in building construction
  • Researchers at Cambridge making synthetic bone have turned to legendary children’s toy Lego for a helping hand.
  • Significance
  • To ‘grow’ a synthetic bone like substance, the researchers first dip a sample into a beaker of calcium and protein, then rinse it in some water and dip in into another beaker of phosphate and protein
  • The process must be repeated over and over to build up the structure, which is time consuming and tedious
  • So the team looked into ways of automating the process, ideally a robot that could simply run while the team worked on other things and/or overnight
  • One solution for acquiring a robot was to purchase an expensive kit off the shelf from a catalog
  • Looking for a cheaper solution the team realized Lego could be the simplest, and cheapest, solution
  • So the team decided to build cranes from a Lego Mindstorms robotics kit
  • They programmed it to perform basic tasks on repeat, using microprocessors, motors, and sensors
  • The sample is tied to string at the end of the crane which then dips it in the different solutions
  • * Of Note*
  • The researchers are also working on hydroxyapatite–gelatin composites to create synthetic bone, of interest because of its low energy costs and improved similarity to the tissues they are intended to replace.
  • Multimedia
  • YouTube VIDEO : Google Science Fair 2012: How can robots aid scientific research ? ( with LEGO) |Google Science Fair
  • YouTube VIDEO :
  • IMAGE : @
  • Social Media
  • Twitter Results for [#]()
  • Further Reading / In the News
  • Growing bones with Lego @ University of Cambridge
  • Growing bones with Lego @ physorg.com

Sorry some coffee lovers

  • The low down
  • While stimulants may improve unengaged workers’ performance, a new University of British Columbia study suggests that for others, caffeine and amphetamines can have the opposite effect, causing workers with higher motivation levels to slack off.
  • Significance
  • Researchers studied the impacts of stimulants on “slacker” rats and “worker” rats, and sheds important light on why stimulants might affect people differently
  • For slacker rats, amphetamine sharpened the mental work ethic, making them more likely to choose the harder task.
  • For workers; however, amphetamine caused the animals to choose the easier option more.
  • Researchers can’t yet explain why stimulants would cause workers to choose the easier task
  • One possibility is that hard workers are already performing optimally, so any chance to the system could cause a net decrease in productivity.
  • * Of Note*
  • This study indicates that people being treated with stimulants would better benefit from a more personalized treatment programs.
  • Further Reading / In the News
  • Slacker rat, worker rat @ sciencenews.org
  • Coffee, other stimulant drugs may cause high achievers to slack off: research @ medicalxpress.com

Einsteins library

  • The low down
  • Albert Einstein’s complete archive is gradually becoming available through the Einstein Archives Online
  • The archive when fully uploaded will have more than 80,000 documents.
  • The archive will contain everything from manuscripts containing the famous E=mc^2 equation written in Einstein’s handwriting to postcards to his mother
  • * Of Note*
  • Einstein was an excellent student, who left school because he couldn’t handle the strict discipline and authority.
  • Further Reading / In the News
  • Einstein Was a Good Student, New Online Archive Suggests @ space.com

SPACECRAFT UPDATE

You could bring about the next great Hubble picture

  • The low down
  • Since 1990, Hubble has made more than a million observations
  • The main way to get Hubble data is the Hubble Legacy Archive website, where a search box lets you look for objects based on their name or coordinates or even which camera on Hubble
  • Realize that Hubble has not been able to observe all objects in the night sky and that scientists get the first chance to work with their data, releasing it to the public a year after they have been made
  • Significance
  • Over a million observations of the Universe have been made by the Hubble Space Telescope. Spacetelescope.org is asking the public to sift through the archives, adjust the colors of their favorite photos with an online tool, and submit to the contest
  • You can search Hubble’s archive for hidden treasures even if you don’t have advanced knowledge
  • It is recommend that people narrow their search to give only results from ACS, WFC3 and WFPC2 – Hubble’s general purpose cameras, as not all of Hubble’s observations are images
  • An interactive tool on the website allows you to look at the image in more detail, and carry out basic image processing such as adjusting the zoom and changing the contrast and colour balance
  • You can save your work as a JPEG
  • The process is entirely browser-based, however you can download the image in a FITS format so you use more advanced software to process the images
  • * Of Note*
  • Images from Hubble are look at the image in more detail, and carry out basic image processing such as adjusting the zoom and changing the contrast and colour balance, containing far more information that the eye can see
  • The beautiful iconic Hubble images seen by the public have been extensively tweaked and optimised by hand, in order to reveal as much of the data as possible
  • Multimedia
  • VIDEO : Hubblecast 53: Hidden Treasures in Hubble’s Archive @ spacetelescope.org
  • Further Reading / In the News
  • Hubble’s Hidden Treaures Website
  • Hubble Legacy Archive
  • What is image processing?
  • Hubble Treasures Contest : iPad and iPod Touch up for Grabs
  • Join the 2012 Hubble’s Hidden Treasures Competition

*— VIEWER FEEDBACK — *

SCIENCE CALENDER

Looking back

  • Apr 07, 1927 : 85 years ago : First Television Broadcast : In 1927, the first public display of a long distance television transmission was viewed by a group of newspaper reporters and dignitaries in the auditorium of AT&T Bell Telephone Laboratories, New York. The research at AT&T was led by Herbert Ives, who introduced the system to the audience, followed by a broadcast speech by the then Secretary of Commerce, Herbert Hoover from Washington, D.C.. Both the live picture and voice were transmitted by wire, over telephone lines. Hoover said,“Today we have, in a sense, the transmission of sight for the first time in the world’s history,” and also, “Human genius has now destroyed the impediment of distance in a new respect, and in a manner hitherto unknown.” The accomplishment was heralded with great acclaim by the press
  • Apr 06, 1930 : 82 years ago : Twinkies!!! : In 1930, Hostess Twinkies snack cakes were invented by James “Jimmy” A. Dewar, plant manager at Continental Baking Company, Chicago as an inexpensive product at the time of the Great Depression. He realized the factory had baking pans for sponge cakes used only during the summer strawberry season, and that they could be made useful year-round for a new product: sponge cakes injected with a banana creme filling. They originally sold at two for a nickel. Vanilla creme was substituted during the WW II banana shortage. The name is said to have come to him based on a billboard he saw for “Twinkle Toe” shoes.

Looking up this week

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]]> Dark Matter | SciByte 3 https://original.jupiterbroadcasting.net/9221/dark-matter-scibyte-3/ Tue, 07 Jun 2011 20:32:00 +0000 https://original.jupiterbroadcasting.net/?p=9221 We take a look dark matter and dark energy, why some scientists still believe they exist, where the theories came from, and how they affect the universe.

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This week on SciByte …
We take a look dark matter and dark energy, why even though we can’t see them directly some scientists still believe they exist, where the theories for them came from, what they are, and how they affect the universe.

We’ll also take a look at a few satellites and studies looking for either direct or in-direct evidence of these mysterious phenomenon.

All that and more, on SciBye!

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Show Notes:

Fritz Zwicky  

  • Found a total of 120 supernovae, over a stretch of 52 years.  Involved in using Tpe 1A supernovae as ‘standard’ candles.  In 1937 posited that galaxy clusters could act as gravitational lenses like previously discovered Einstein effect, confirmed in 1979.
  • The first person to provide evidence and infer the presence of dark matter
  • Virial Theorem – for a stable, self-gravitating, spherical distribution of equal mass objects (stars, galaxies, etc), the total kinetic energy of the objects is equal to minus 1/2 times the total gravitational potential energy. In other words, the potential energy must equal the kinetic energy, within a factor of two.

Dark Matter

  • most stars in spiral galaxies orbit at roughly the same speed which suggest that either Newtonian gravity does not apply universally or that, conservatively, upwards of 50% of the mass of galaxies was contained in the relatively dark galactic halo [stars and globular clusters surrounding the galaxy]
  • Astrophysicists predicted the mass would be low in density, but high in temperature (~million degrees Celsius)
  • Theory states there should be about double the amount of matter in the local Universe compared to what is observed
  • the majority of this missing mass should be located in large-scale cosmic structures called filaments – a bit like thick shoelaces
  • Through A Universe Darkly” – A Cosmic Tale of Ancient Ethers, Dark Matter, and the Fate of the Universe

Dark Energy

  • Edwin Hubble first noticed that the Universe was actually expanding, in 1932.
  • Believed to be behind the acceleration of the expansion of the Universe
  • Visual representation of the expansion of the Universe
  • Is Einstein’s vision of gravity, general relativity, incorrect on large cosmological scales?
  • Does “empty space” possess its own energy?

Measuring the Expansion of the Universe [ Hubble constant, or H0 ]

  • Named after Edwin Hubble who first measured the expansion of the universe nearly a century ago
  • Einsteins ‘biggest blunder’ not actually a blunder
  • Type Ia supernovae : produces consistent peak luminosity because of the uniform mass of white dwarfs that explode via the accretion mechanism
  • Cepheid variable stars are the backbone of the distance ladder because their pulsation periods, which are easily observed, correlate directly with their luminosities
  • Large Magellanic Cloud (LMC) and Small Magellanic Cloud (SMC), two of the nearby satellite galaxies of our own Milky Way Galaxy, since they contain large number of Cepheids, they can be used to calibrate the distance scale
  • Redshift / Blueshift : How fast are things moving away from us? [Red=away]

Cosmic Microwave Background (CMB)

  • Cosmic Background Radiation Image
  • The radiant heat left over from the Big Bang. (first observed in 1965)
  • properties of the radiation contain a wealth of information about physical conditions in the early universe and a great deal of effort has gone into measuring those properties since its discovery.
  • The hot spots and cold spots, which differ in temperature by only millionths of a degree, can be interpreted as very slight differences in the crowding together of matter in the young universe. Hot spots had slightly more matter than average; cold spots a bit less

Wilkinson Microwave Anisotropy Probe

  • 3D model [proposed to NASA in 1995, launched in 2001]
  • cooled microwave radiometers measure the properties of the cosmic microwave background radiation over the full sky
  • Measuring the temperature of the microwave sky to an accuracy of one millionth of a degree revealing conditions as they existed in the early universe
  • using differences in temperature measured from opposite directions (anisotropy).
  • Orbits at Lagrange point 2 :provides for a very stable thermal environment and near 100% observing efficiency since the Sun, Earth, and Moon are always behind the instrument’s field of view

Anisotropy

  • property of being directionally dependent
  • defined as a difference, when measured along different axes, in a material’s physical or mechanical properties [light coming through a polarizer]

Wilkinson Microwave Anisotropy Probe results

  • Complete census of the universe finds that dark matter (not made up of atoms) make up 23.3% (to within 1.3%)
  • Accuracy and precision determined that dark energy makes up 72.1% of the universe (to within 1.5%), causing the expansion rate of the universe to speed up.
  • making accurate measurements of the cosmic microwave background fluctuations, WMAP is able to measure the basic parameters of the Big Bang model including the density and composition of the universe
  • Microwave light seen by WMAP from when the universe was only 380,000 years old, shows that, at the time, neutrinos made up 10% of the universe, atoms 12%, dark matter 63%, photons 15%, and dark energy was negligible. In contrast, estimates from WMAP data show the current universe consists of 4.6% percent atoms, 23% dark matter, 72% dark energy and less than 1 percent neutrinos.
  • Mapped the Cosmic Microwave Background (CMB) radiation (the oldest light in the universe)
  • WMAP definitively determined the age of the universe to be 13.73 billion years old to within 1% (0.12 billion years)
  • Reported the first direct detection of pre-stellar helium, providing an important test of the big bang prediction. [Jan26, 2010]
  • Nailed down the curvature of space to within 1% of “flat” Euclidean
  • Started to sort through the possibilities of what transpired in the first trillionth of a trillionth of a second, ruling out well-known textbook models for the first time

Australian Student Uncovers the Universe’s Missing Mass

  • Conducted a targeted X-ray search for the hidden matter and within just three months made a very exciting discovery
  • Dark Matter theories have been based solely on numerical models

WiggleZ Dark Energy Survey

  • Einstein Confirmed Again: Dark Energy Present In The Universe
  • Firstly, observed how dark energy opposes gravity by speeding up the overall rate of expansion of the Universe
  • Secondly, observed how dark energy opposes gravity by slowing down the growth of clusters and superclusters with time
  • mapped the distribution of galaxies over an unprecedented volume of the Universe
  • WiggleZ scientists have made a 3-D map of more than 150,000 galaxies near and far to trace the universe’s evolution over time
  • 10min Podcast on WiggleZ

Additional Information:

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]]> Time | SciByte 2 https://original.jupiterbroadcasting.net/8966/time-scibyte-2/ Wed, 01 Jun 2011 03:00:15 +0000 https://original.jupiterbroadcasting.net/?p=8966 We investigate time, how we have measured it’s passage throughout history, philosophically, how it’s affected by gravity, and the very concept of time itself!

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We spend some time looking at time, how we have measured it’s passage throughout history, philosophically, how it’s affected by gravity, and the very concept of time itself.

Plus find out why Einstein proposes that we travel through time at the speed of light, how Atomic clocks work, and is it possible gravitational fields warp time?

All that and more, on SciBye!

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Show Notes:

Concept:
  • “Time is what keeps everything from happening at once.” – Ray Cummings, Sci-Fi Author

Measurement:

  • Smallest units of time = Planck time [time it takes for light to travel the shortest distance current theories can handle]
Philosophy:
  • Why do we always move forward?
Scientific:
  • Is time eternal, or a side effect of “space”?

Philosophy on the Nature of Time:

  • Immanuel Kant believes time is all in our heads, as a necessity to quantify sensory inputs of everyday existence. Also believes in predestination, and that Free Will can only exist outside of Time.
  • Martin Heidegger believes similarly, and that humans should be capable of “stepping out of time” by a specific form of non-associative thinking. The past, present and future can become one within our minds, and experienced in random order. (uhm, excuse me?!?)
  • Henri Bergson believed that Time could not be measured because it is infinite and malleable, and shapes itself to the perceptions of an individual.
  • “Time is an illusion” is a common saying in Buddhist teachings.
  • HG Wells: “There is no difference between time and any of the three dimensions of space except that our consciousness moves along it.” — The Time Machine
  • C. S. Lewis “The future is something which everyone reaches at the rate of 60 minutes an hour, whatever he does, whoever he is.” (but do those min pass by at the same rate)

‘When’ was the Start of the Universe, T=0 point

    • Red Shift / Blue ShiftDoppler Effect light waves act similar to sound waves coming towards you or away from you.  Blue shift = Away; Red shift = Near
    • Type 1A Supernova – PIC – To judge distance and speed [red shift/blue shift]
    • Roughly 13.7 Billion Years ago

Measurement ‘devices’ through history

    • Mayan’s : Mayan Calender created during the Dark Ages in Europe

Calculated

  • Earth orbit @ 365 days [Actual = 365.2422 days, 0.06%]
  • Lunar Month @ 29.53086 days [Actual = 29.53059 days; 0.0009%]
  • Mercury orbit @ 117 days [Actual = 116 days; 0.86%]
  • Venus orbit @ 584 days [Actual = 583.92 days; 0.01%]
  • Mars orbit @ 780 days [actual = 779.936 days; 0.008%]
  • Antikythera mechanism – is an ancient mechanical computer designed to calculate astronomical positions. It was recovered in 1900–1901 from the Antikythera wreck. Its significance and complexity were not understood until decades later. Its time of construction is now estimated between 150 and 100 BC. The degree of mechanical sophistication is comparable to a 19th century Swiss clock. Technological artifacts of similar complexity and workmanship did not reappear until the 14th century, when mechanical astronomical clocks were built in Europe

A day – 24 hours?

  • 2 Radio telescope set  on different points of Earth measure a radio wave from a quasar. They line up once a ‘day’ which is not always 24 hours [changes are in mili seconds]

Atomic Clocks

    • In certain elements [like Cesium] the Electrons will ‘jump’ between orbits and emit a flash of light at precise intervals [Cesium, 9 billion times a sec]  Video
    • Such a clock, if sent on a space shuttle, ticks at a different speed. Because it is further from Earth’s gravitational pull.

EINSTEIN:

    • Einstein proposes that we travel through Time at the speed of light.
    • Einstein: Spacetime is a single entity, not separate things. And because of the mixing of space & time, time ticks differently for separate entities, based on relative speeds.
    • The faster you travel through space, the slower you travel through time.
    • Proven by the Shapiro effect (blip in Mercury’s orbit, measured on opposite sides of the Sun)

Shapiro Effect

  • Gravitational fields warp time
  • blip in Mercury’s orbit, measured on opposite sides of the Sun – VIDEO

If time is flexible based on observation, then all of it always exists…

    • (Incorrect for quantum mechanics)
    • New theories suggest that “spacetime” is granular, and not fixed. On a large scale it looks like a single thing, but it actually flows as it is being created, in the future.

Black holes actually STOP time at their event horizon, to an outside observer.
But an observer falling in would see time speed up around them, the closer they got.

Time Travel?
High speed camera moments
Lighter

Busting Water Baloon

Additional Information
CPT – Charge, Parity, and Time Reversal (CPT) Symmetry

WIKI – Shapiro Delay

What Time Is It? (part 1 // part 2 // part 3 // part 4)

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Gravity | SciByte 1 https://original.jupiterbroadcasting.net/8723/gravity-scibyte-1/ Tue, 24 May 2011 23:24:32 +0000 https://original.jupiterbroadcasting.net/?p=8723 We look at the results from Gravity Probe B and how they relate to Einstein’s predictions on mass, space, time and how they all interact with one another.

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This week on SciByte …
We look at the results from Gravity Probe B and how they relate to Einstein’s predictions on mass, space, time and how they all interact with one another. We’ll also open up the guts of that crazy contraption, and discuss some of the impressive tech that made the whole experiment possible to begin with.

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Show Notes:

Gravity?

-Sir Issac Newton [Mathematician]
-1687 – His predictions predicted the existence of Neptune based on the motions of Uranus
-Mercury’s Orbit hower can NOT be explained by Newtonian math alone, but was resolved with Einsteins general theory of relativity in 1915
-Newtonian Calculations however still are accurate enough for most applications
-General Relativity – Albert Einstein [1907-1915] The observed gravitational attraction between masses results from their warping of space and time.
→ Space-Time is not flat, but can be stretched and warped by matter
-What this means, boiled down: Time moves slower under gravity

Gyroscope

-A device for measuring or maintaining orientation, based on the principles of conservation of angular momentum.
Video : Gyroscope
Video : Conservation of Angular Momentum : Spinning Skater

Gravity Probe A

-“A” confirmed the prediction that gravity slows the flow of time, and the observed effects matched the predicted effects to an accuracy of about 70 parts per million. [1976, and lasted <2hours]
-Used a hydrogen maser, a highly accurate frequency standard, to measure the rate change of a clock in lower gravity with high precision.

Gravity Probe B

-A star, a telescope, a spinning sphere [conceived in 1959, launched in 2004, decommissioned in Dec 2010]  [A Star, telescope, and space time]
Gravity Probe B Cutaway
-Reference telescope sighted on IM Pegasi, a binary star in the constellation Pegasus
-Drag Free System
-Solar Radiation Pressure – Particles streaming away from Sun transferring momentum
-Atmospheric Drag [@624KM]
-Compensation done with helium boosters, full 6-degree motion (first ever)
-London moment gyroscopes
-A spinning superconductor generates a magnetic field whose axis lines up exactly with the spin axis of the gyroscopic rotor.
-Are housed in a dewar of superfluid helium @ a temperature of under 2 kelvins (−271 °C, −456 °F)
-A magnetometer determines the orientation of the generated field, which is interpolated to determine the axis of rotation.

** The pointer shifted by just 6,000 milliarcseconds — the width of a human hair as seen from 10 miles away
* At the time, the gyroscopes were the most nearly spherical objects ever made.

~ size of ping pong balls, they are perfectly round to within forty atoms
– Scaled to the size of the Earth, the elevation of the entire surface would vary by no more than 12 feet
* Measured changes in gyroscope the equivalent to an angular separation the width of a human hair viewed from 32 kilometers (20 miles) away over a one-year period. [0.5 milliarcseconds (1.4×10−7 degrees)]

Already Proven?

The Apollo astronauts left retro-reflector mirrors on the Moon, and laser ranging from Earth can now track their positions to millimeters. At that level of precision, the Moon’s motion in orbit has confirmed gravitomagnetism, the source of frame-dragging, to 0.15%, or 130 times better than GP-B.

Precision measurements of the Shapiro effect or gravitational time delay for light, most recently in 2002 by the Cassini space probe

Gravity – no uniform model for all scales

The laws of classical Newtonian physics remain accurate in predicting the behavior of the vast majority of large objects—of the order of the size of large molecules and bigger—at velocities much smaller than the velocity of light

Quantum mechanics

-By Newtonian Standards Atoms can’t exist
-Newtonian physics says that electrons would fall out of orbit into the nuclues
-Electron Orbits in actuality can only exist as very specific points
-Heisenburg Uncertainty principle – can’t know location AND speed

Black holes

-First conceptualized in 1783 by Henry Cavendish
-Infinite Density; Event Horizon [point of no return]

Dark Matter

-Matter that is inferred to exist from gravitational effects on visible matter and background radiation, but is undetectable by emitted or scattered electromagnetic radiation

Dark Energy

-Hypothetical form of energy that permeates all of space and tends to increase the rate of expansion of the universe
Dark Matter/Dark Energy Estimates
-Some estimates state The Universe is made up of 23% Dark Matter; 72% Dark Energy; and Atoms a mere 4.6%

Additional Information :

SPACETIME: From the Greeks to Gravity Probe B
NASA : Gravity Probe B
Sky&Telescope : Gravity Probe B: Relatively Important?
PC Magazine : It Took More Than 50 Years, But NASA Proves That Einstein Was CorrectScientific American : Earth’s Mass and Motion Warps Spacetime as Einstein Said
engadget : NASA concludes Gravity Probe B space-time experiment
National Geographic : Einstein Theories Confirmed by NASA Gravity Probe
NASA Gravity Probe Confirms Two Einstein Theories
Wired : Floating Gyroscopes Vindicate Einstein
spaceRef : NASA’s Gravity Probe B Confirms Two Einstein Space-Time Theories
PCWorld:Experiment Confirms Space-Time Vortex Around Earth, Makes Our Heads Hurt
What’s 96 Percent of the Universe Made Of? Astronomers Don’t Know
YouTube | Lecture 1 | Modern Physics: Quantum Mechanics (Stanford)

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