Grasshopper – Jupiter Broadcasting https://www.jupiterbroadcasting.com Open Source Entertainment, on Demand. Mon, 22 Feb 2016 02:46:59 +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 Grasshopper – Jupiter Broadcasting https://www.jupiterbroadcasting.com 32 32 Exoplanet & Bee Venom | SciByte 86 https://original.jupiterbroadcasting.net/33896/exoplanet-bee-venom-scibyte-86/ Tue, 19 Mar 2013 20:47:03 +0000 https://original.jupiterbroadcasting.net/?p=33896 We take a look at an exoplanets atmosphere, HIV killing bee venom, ancient sundials, viewer feedback, and much more!

The post Exoplanet & Bee Venom | SciByte 86 first appeared on Jupiter Broadcasting.

]]>

post thumbnail

We take a look at an exoplanets atmosphere, HIV killing bee venom, ancient sundials, viewer feedback, spacecraft updates, Curiosity news, and as always take a peek back into history and up in the sky this week.

Direct Download:

MP3 Audio | OGG Audio | Video | Torrent | YouTube

RSS Feeds:

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

Support the Show:

[asa]B00BEZTMQ8[/asa]
[asa]B009SPZ11Q[/asa]


Show Notes:

Exoplanet Atmosphere

  • A team led by an astrophysicist at the American Museum of Natural History in New York City, has found hints of ammonia, methane, carbon dioxide and acetylene in an exo-planets’ atmosphere in the sharpest spectrum ever obtained of an extrasolar planet
  • Searching for Exoplanets
  • In the past, astronomers inferred the existence of exoplanets and their gases by looking for subtle changes in the light streaming from the planet’s star
  • Now, with improved instruments, a team has detected light coming directly from a planet light-years away
  • The data have high enough resolution to reveal not only the presence but the abundance of carbon monoxide and water in the planet’s atmosphere
  • Such information could shed light on how the planet formed
  • Studies could also reveal the presence of life on a distant planet, but this planet’s size and orbit have already ruled it out as a habitable world
  • The System
  • In 2008 the first image of a multi planet system outside the solar system, showing three gas giants orbiting the star HR 8799
  • The results suggest the HR 8799 system is like a scaled-up Solar System
  • HR 8799 is about 130 light-years from Earth, in the constellation Pegasus
  • The planets are scorching hot, making them bright enough for astronomers to detect directly
  • In 2010, the researchers imaged a fourth planet around HR 8799, a new study focused on one of these planets, HR 8799c.
  • HR 8799c
  • Five to 10 times as massive as Jupiter, HR 8799c sits about eight times farther away from its star than Jupiter does from the sun
  • Because of that great distance, the astronomers could block the star’s light and record infrared light
  • Even with water present on this world, it is incredibly hostile to life
  • Like Jupiter, it has no solid surface, and it has a temperature of more than a thousand degree
  • The Studies
  • Because different gases absorb and emit light in distinct ways, the team could identify carbon monoxide and water but found no methane, which scientists had thought might be present.
  • In another new study researchers simultaneously collected infrared light from the atmospheres of all four planets
  • The chemistry of each planet varies different from anything in our own solar system
  • Although the teams looked at different wavelengths of light, which pick up different types of molecules, the two studies appear consistent
  • By peering at just one planet, one team obtained more detailed data that allowed the researchers to get a sense of how much carbon and oxygen is in HR 8799c’s atmosphere
  • Knowing the ratio of carbon to oxygen in the atmosphere may reveal how the planet formed
  • Planetary Formation Theories
  • Astronomers have two competing theories of how planets arise from the disk of gas and dust encircling a young star
  • In the gravitational instability model, some of the gas and dust suddenly clumps and collapses, simultaneously creating a planet’s core and atmosphere
  • In this scenario, the chemical composition of a planet should match that of its star
  • In the other model, known as core accretion, planets are built in two-steps
  • First, material from the disk accumulates into a core, later the core captures gases swirling in the disk to form an atmosphere.
  • In this case, the carbon-to-oxygen ratio of the planet may differ from the star because the accretion of cores may deplete the disk of certain elements
  • What This Planet\’s Data Tells Us
  • Compared with its star, HR 8799c appears to have slightly more carbon relative to oxygen, suggesting the planet originated via core accretion
  • It is surmises that when the disk around HR 8799 formed, water froze into particles of ice, the bits of ice then collided to form the planet’s core, leaving behind little water vapor, and therefore less oxygen, when the planet accumulated its atmosphere later on
  • Other researchers are not convinced by this conclusion saying “We don’t really understand planetary formation enough to make a strong case either way,”
  • The Future
  • Either Way the data from both new studies may help astronomers refine their simulations of planetary formation
  • Not that astronomers have directly imaged planets around three distant stars researchers are poised to capture light from many more planets
  • Project 1640, is looking for Jupiter-sized planets around some 200 stars
  • “Ultimately, with better instruments, people will be able to use these methods on Earthlike planets.”
  • Multimedia
  • YouTube Remote Reconnaissance of Another Solar System | AMNHorg
  • Video Clip Nearby Stars with planets| AMNHorg
  • Video Clip HR 8799 System| AMNHorg
  • Further Reading / In the News
  • Exoplanet Atmospheres Provide Clues to Solar System Formation | UniverseToday.com
  • Distant planets\’ atmospheres revealed | Atom & Cosmos | ScienceNews.org

— NEWS BYTE —

Bees Against HIV

  • Nanoparticles carrying a toxin found in bee venom can destroy human immunodeficiency virus (HIV) while leaving surrounding cells unharmed
  • What it Does
  • Bee venom contains a potent toxin called melittin that can poke holes in the protective envelope that surrounds HIV, and other viruses
  • The new study shows that melittin loaded onto these nanoparticles does not harm normal cells, because added protective bumpers to the nanoparticle surface
  • When the nanoparticles come into contact with normal cells, which are much larger in size, the particles simply bounce off
  • HIV, on the other hand, is even smaller than the nanoparticle, so HIV fits between the bumpers and makes contact with the surface of the nanoparticle, where the bee toxin awaits
  • The advantage of this approach is that the nanoparticle attacks an essential part of the virus\’ structure. In contrast, most anti-HIV drugs inhibit the virus\’s ability to replicate.
  • Drawbacks
  • This anti-replication strategy does nothing to stop initial infection, and some strains of the virus have found ways around these drugs and reproduce anyway.
  • Where it does work, because it attacks the inherent physical property of HIV, theoretically, there isn\’t any way for the virus to adapt to this treatment
  • The potential for using nanoparticles with melittin as therapy for existing HIV infections, especially those that are drug-resistant
  • Other Uses
  • The hope is that in places where HIV is running rampant, people could use this gel as a preventive measure to stop the initial infection
  • Since melittin attacks double-layered membranes indiscriminately, this concept is not limited to HIV.
  • Many viruses, including hepatitis B and C, rely on the same kind of protective envelope and would be vulnerable to melittin-loaded nanoparticles
  • In addition to antiviral therapy, the paper\’s senior author has shown melittin-loaded nanoparticles to be effective in killing tumor cells.
  • Further Reading / In the News
  • Nanoparticles loaded with bee venom kill HIV | MedicalXPress.com

— TWO-BYTE NEWS —

Worlds Oldest Egyptian Sundials

  • Telling Time in Ancient Egypt
  • During archaeological excavations in the Kings\’ Valley in Upper Egypt a team of researchers found one of the world\’s oldest ancient Egyptian sundials
  • During this year\’s excavations the researchers found a flattened piece of limestone (so-called Ostracon) on which a semicircle in black color had been drawn
  • The semicircle is divided into twelve sections of about 15 degrees each.
  • A dent in the middle of the approximately 16 centimeter long horizontal baseline served to insert a wooden or metal bolt that would cast a shadow to show the hours of the day
  • Small dots in the middle of each section were used for even more detailed time measuring
  • It was found in an area of stone huts that were used in the 13th century BC to house the men working at the construction of the graves, possibly used to measure their work hours
  • The division of the sun path into hours also played a crucial role in the so-called netherworld guides that were drawn onto the walls of the royal tombs
  • These guides are illustrated texts that chronologically describe the nightly progression of the sun-god through the underworld.
  • The sundial could also have served to further visualize this phenomenon.
  • Multimedia
  • Image Ancients Egyptian sun dial | Phys.org | Credit: University of Basel
  • Further Reading / In the News
  • One of the world\’s oldest sun dial dug up in Kings\’ Valley | Phys.org

— VIEWER FEEDBACK —

ESTCube

  • Karl Sakrits
  • Estonia is sending up their first satellite, a CubeSat, made by University students to test the electric solar wind sail
  • CubeSat
  • The CubeSat standard for nanosatellites was followed during the engineering of ESTCube-1,
  • The CubeSat standard has three different sizes corresponding to size 1U, 2U and 3U. Base side lengths are the same but height is 2 to 3 times bigger than 1U CubeSats
  • Mass is also set in CubeSat standard, the highest possible mass for 1U CubeSat is 1300 grams, 2U CubeSat 2600 grams and 3U CubeSat 4000 grams
  • CubeSat base side length must be 100.0 +/- 0.1 millimeters and satellite height must be 113.5±0.1 mm
  • Purpose
  • Although its main purpose was to educate students, the satellite does have a scientific purpose.
  • On board of the satellite is an electric solar wind sail (e-sail) which was created by a Finnish scientist Pekka Janhunen, which will be the first real experimentation of the e-sail
  • Subsystems
  • ADCS – attitude determination and control system, determines and modifies satellite\’s alignment
  • CAM – onboard camera for taking pictures of the Earth and the unreeled tether
  • CDHS – command and data handling system, the satellite\’s main onboard computer
  • COM – communications system for up- and downlinks
  • EPS – electrical power system, provides electrical power for the satellite
  • PL – payload, the satellite\’s experiment module, that contains the tether and everything else related to the experiment
  • STR – satellite\’s structure
  • Solar Wind Sail
  • 10 meters of e-sail 50 to 20 micrometers thick wire of high-technology structure so-called Heytether will be deployed from the satellite.
  • The deployment of the Heytether can be detected by decrease of the satellite\’s speed of rotation or by a on-board camera
  • To control the loaded solar wind sail elements interaction with the plasma surrounding the earth and the effect it has on the spacecraft spinning speed the spacecraft has two on-board nanotechnologic electron emitters/gun
  • The electron emitters are connected to the e-sail element and by shooting out electrons it loads the e-sail element positively to 500 volts
  • The positive ions in the plasma push the e-sail element and have an influence on the satellites rotation speed
  • The effect of the e-sail is measured by the change in rotation speed
  • The camera is used to take a picture of Earth and the successfully deployed Heytether.
  • Mission
  • ESTCube-1 will be sent to orbit by the European Space Agency\’s rocket Vega in spring of 2013
  • Half an hour after the satellites deployment from the start capsule satellites antennas will be opened and radio transmitter and important subsystems will be switched on
  • The first days or weeks will be used to test the satellite and set it to work on full capacity
  • They will then orient the satellite so the on-board camera will be faced to earth so that they can try to take a picture of Estonia
  • They will rotate the satellite on an axis with a speed of 1 revolution per second
  • The E-sail element will deploy from the satellite by a centrifugal force and will confirm the deployment via the on-board camera
  • Then they will activate the electron emitter and loading the e-sail, measuring the e-sails and Lorentz force by satellites revolutions per second
  • If possible they will use the negatively charged e-sail to take the satellite off orbit and burn it in the earths atmosphere
  • Should everything go perfect the mission could be completed within a few weeks to a month
  • Communication
  • Communicating with the satellite will be held by two International Amateur Radio Unions three registered frequencies [437.250 MHz, 437.505 MHz]
  • The maximum possible connection speed is 19,200 bits per second, only to be used when the satellite has been given a specific order
  • Important satellite parameters will be transmitted every 3 to 5 minutes, and periodic but slow communication can be done on a telegraphic signal
  • A 9600 baud connection speed and AX.25 standard is used, a slower communication frequency which allow a maximum of 25 kiloherz bandwidth, fast connection will only be used when the satellite has been given a specific
  • Software
  • FreeRTOS on the satellite\’s Command and Data Handling System and camera module
    TinyOS on the satellite\’s communication module
  • Financing and costs
  • This option is the cheapest possibility to send a satellite into orbit is offered by European Space Agency
  • Estonia is an associated member of ESA most of the launch expenses (about 70,000 euros) will be covered from Estonian member fee for educational expenses
  • The total expense, with launch cost, for the project are approximately 100,000 euros
  • Multimedia
  • YouTube estcube dissection2 | taavi torim
  • YouTube Packing ESTCube-1 for shipping. Tallinn TV Tower 21.1.2013. | AjattaraQuad
  • ESTCube.eu | Video Library
  • Twitter
  • ESTCube @ESTCube
  • Further Reading / In the News
  • ESTCube.eu

— Updates —

Space Shuttle Atlantis

— SPACECRAFT UPDATE—

SpaceX’s Grasshopper Hops Higher

  • GrassHopper
  • Grasshopper stands 10 stories tall and consists of a Falcon 9 rocket first stage tank, Merlin 1D engine, four steel and aluminum landing legs with hydraulic dampers, and a steel support structure
  • The goal of Grasshopper is to eventually create a reusable first stage for SpaceX’s Falcon 9 rocket, which would be able to land safely instead of falling back into the ocean and not being usable again
  • On March 7, 2013, the vertical and takeoff and landing (VTVL) vehicle, rose 24 stories, 263 ft / 80m, hovered for approximately 34 seconds and then landed safely, and more accurately than ever before
  • Previous Tests
  • This is Grasshopper’s fourth in a series of test flights, with each test demonstrating exponential increases in altitude
  • September 2012 | Flew to 8.2 ft / 2.5 meters
  • November 2012 | Flew to 17.7 ft / 5.4 meters
  • December 2012 | Flew to 131 ft / 40 meters
  • Multimedia
  • Ring of Fire | spacexchannel
  • Further Reading / In the News
  • SpaceX Grasshopper Takes a Leap Into a \’Ring of Fire\’ | UniverseToday.com

— CURIOSITY UPDATE —

  • Analyzing the Drill Sample
  • Curiosity obtained her first drill sample and passed that sample on to her onboard analytical lab instruments, called CheMin and SAM
  • These powerful instruments can tell about what minerals are present in these rocks and whether they contain the ingredients necessary to sustain life as we know it.
  • When the rover science team combine the data from remote sensing and contact science instruments from CheMin and SAM, we get a picture of an ancient watery environment, which would have been habitable had life been present in it.
  • At that site of Opportunity rover, the sedimentary rocks record evidence of an environment that was only wet on a very intermittent basis, and when it was, the waters that were there were highly acidic, very salty, and not favorable for the survival of organic compounds.
  • CheMin instrument, tells us that the minerals that are present in this lakebed sedimentary rock at John Klein are very different from just about anything we\’ve ever analyzed before on Mars and was deposited in a freshwater environment
  • The SAM instrument is telling us that these rocks contained all of the ingredients necessary for a habitable environment
  • The science team found carbon, sulfur and oxygen, all present and a number of other elements in states that life could have taken advantage of.
  • Image Mosaic
  • The mosaic of images from the Mast Camera (Mastcam) on NASA\’s Mars rover Curiosity shows Mount Sharp in raw color as recorded by the camera.
  • This mosaic was assembled from dozens of images from the 100-millimeter-focal-length telephoto lens camera mounted on the right side of the Mastcam instrument
  • Raw color shows the scene\’s colors as they would look in a typical smart-phone camera photo, before any adjustment.
  • White-balancing helps scientists recognize rock materials based on their experience looking at rocks on Earth
  • White balancing yields an overly blue hue in images that have very little blue information, such as Martian landscapes, because the white balancing tends to overcompensate for the low inherent blue content.
  • Multimedia
  • YouTube Curiosity Rover Report (Mar. 15, 2013) | Rover Hits Paydirt | JPLnews
  • Image Galleries at JPL and Curiosity Mulimedia
  • Social Media
  • Curiosity Rover @MarsCuriosity
  • Further Reading / In the News

SCIENCE CALENDAR

Looking back

  • March 23, 2001 : 12 years ago : Mir destroyed : The Russian space station, Mir, ended 15 years in orbit by burning up in Earth\’s atmosphere as the way chosen to end its life. Mir, launched in 1986, had far exceeded its original planned five year lifespan. The Russian government decided in Oct 2000 that its poor condition could no longer justify the expense to maintain its use. A docked Progress tanker had been remotely commanded by mission controllers to fire rockets and lower its orbit and cause re-entry into the atmosphere. The debris that did not burn up during reentry fell harmlessly into the Pacific Ocean at the planned target zone between New Zealand and Chile. For safety, airlines had rerouted Pacific flights in anticipation of the event, and ships had been warned earlier

Looking up this week

The post Exoplanet & Bee Venom | SciByte 86 first appeared on Jupiter Broadcasting.

]]>
Painful Math & Canadian Rovers | SciByte 70 https://original.jupiterbroadcasting.net/27201/painful-math-canadian-rovers-scibyte-70/ Thu, 08 Nov 2012 22:54:38 +0000 https://original.jupiterbroadcasting.net/?p=27201 We take a look at Painful Math, Canadian robotic rovers, using the Kinect in science, updates on spacecraft, stories, and Curiosity!

The post Painful Math & Canadian Rovers | SciByte 70 first appeared on Jupiter Broadcasting.

]]>

post thumbnail

We take a look at Painful Math, Canadian robotic rovers, using the Kinect in science, updates on spacecraft, stories, and Curiosity, viewer feedback, and as always take a peek back into history and up in the sky this week.

Direct Download:

MP3 Download | Ogg Download | Video | YouTube

RSS Feeds:

MP3 Feed | Ogg Feed | iTunes Feed | Video Feed

Support the Show:

[asa]B008QZ5PY2[/asa]
[asa]0345529413[/asa]


   

Show Notes:

Math Hurts

  • Mathematics anxiety can prompt a response in the brain similar to when a person experiences physical pain, according to new research
  • The low down
  • Using brain scans, scholars determined that the brain areas active when highly math-anxious people prepare to do math overlap with the same brain areas that register the threat of bodily harm
  • Anticipation of doing math prompts a similar brain reaction as when they experience pain
  • Significance
  • Researchers found it was the anticipation of having to do math, and not actually doing math itself, that looked like pain in the brain.
  • Brain activation does not happen during math performance, suggesting that it is not the math itself that hurts it is the anticipation of math is painful
  • Scholars worked with 14 adults who were shown to have math anxiety based on their responses to a series of questions about math
  • Additional tests showed that these individuals were not overly anxious in general; instead, their heightened sense of anxiety was specific to math-related situations.
  • Volunteers were tested in an fMRI machine, which allowed researchers to examine brain activity as they did math, they were given mathematical equations to verify like the validity of the following equation: (12 x 4) – 19 = 29
  • Subjects were also shown short word puzzles. For these puzzles, people saw a series of letters (for example: yrestym) and had to determine if reversing the order of the letters produced a correctly spelled English word.
  • fMRI scans showed that the anticipation of math caused a response in the brain similar to physical pain
  • The higher a person’s anxiety about math, the more anticipating math activated the posterior insula—a fold of tissue located deep inside the brain just above the ear that is associated with registering direct threats to the body as well as the experience of pain.
  • Math anxiety levels were not associated with brain activity in the insula or in any other neural region when volunteers were doing math.
  • For those with math anxiety, a painful sense of dread may begin long before a person sits down to take a math test.
  • Of Note
  • current work is also consistent with other research which showed that the mere anticipation of doing mathematics changes functioning in the brains of people with high levels of math anxiety
  • Mathematics anxiety can begin as early as first grade
  • The value of seeing math anxiety not just as a proxy for poor math ability, but as an indication there can be a real, negative psychological reaction to the prospect of doing math.
  • The reaction needs to be addressed like any other phobia rather than simply piling on math homework for students who are anxious about math, students need active help to become more comfortable with the subject
  • For instance, that writing about math anxieties before a test can reduce one’s worries and lead to better performance.
  • Further Reading / In the News
  • When people worry about math, the brain feels the pain | MedicalXPress.com

— NEWS BYTE —

Canadian Robotic Rovers?

— TWO-BYTE NEWS —

Kinect in Science

  • Researchers in Scotland have devised a means of using a Microsoft Kinect sensing system to allow for hand control of holographic optical tweezers
  • The low down
  • Laser tweezers are laser based devices that allow for manipulation of very small objects; typically at the cellular level
  • A laser beam is projected towards a target, but before reaching it, is split into three separate beams
  • The three beams are broadcast onto the edges of the object to be manipulated and as the beams are moved the object is caused to move in lockstep
  • However fine tuning control of the laser to cause the movement of an object has been less than ideal and researchers to continue looking for alternative means
  • Significance
  • In this new research, the team connected a Microsoft Kinect device to the tweezers and then demonstrated an ability to move microscopic sized objects by moving their hands around in the air.
  • Connecting a Kinect device to their virtual tweezers, the researchers found that they were able to define the space in which they wished to work by using simple hand movements and then to connect, virtually to a particular tiny object
  • The Kinect is not precise enough to capture subtle movements however as it doesn’t allow for force-feedback, or the ability to feel the resistance of an object as its being moved
  • Of Note
  • HoloHands, is not sophisticated enough to allow for serious research work but it is being used as a tool for educational purposes, either as a tool, or implemented as a learning game.
  • Multimedia
  • YouTube HoloHands: Kinect control of holographic optical tweezers | dundeephysics
  • Kinect control of two trapped particles. | C. McDonald
  • Further Reading / In the News
  • Physicists use Kinect to control holographic tweezers (w/ Video) | phys.org

– SPACECRAFT UPDATE –

Shuttles

— Updates —

Space-X’s Grasshopper

  • The low down
  • SpaceX is developing the “Grasshopper” reusable vertical takeoff, vertical landing rocket
  • In September, the 32-meter- (106-ft-) tall Grasshopper made a tiny hop – barely lifting off the pad just to test-fire its engines
  • The Grasshopper has now made a second, bigger hop
  • Phase 1 and 2
  • Reportedly the goal with Grasshopper is to eventually create a reusable first stage for its Falcon 9 rocket that would be able to land safely instead of falling back into the ocean and not being usable again
  • The Grasshopper test program is to have three phases of test launches at SpaceX’s facility in McGregor, Texas
  • Both Phase 1 and 2 flights would last up to 45 seconds.
  • Phase 1 rocket would rise to not more than 240 feet [73 meters]
  • Phase 2 rocket would rise to not more than 670 feet [204 meters]
  • Both Phase 1 and 2 flights would last up to 45 seconds.
  • Phase 3
  • Phase 3 tests have the goal of increasingly higher altitudes with higher ascent speeds and descent speeds altitude test sequence likely would be 1,200 feet [366 meters]; 2,500 feet [762 meters]; 5,000 feet [1,524 meters]; 7,500 feet [2,286 meters]; and 11,500 feet [3,505 meters]
  • The maximum test duration of Phase 3 firings would be approximately 160 seconds. If all goes well the Grasshopper would land back on the launch pad
  • Multimedia
  • YouTube Flight of 10 story tall Grasshopper rocket | Clark Lindsey
  • Social Media
  • SpaceX @SpaceX
  • Further Reading / In the News
  • SpaceX’s 10-Story Re-useable Grasshopper Rocket Takes a Bigger Hop | UniverseToday.com

Documentary : Chasing Atlantis

Fermi

  • Astronomers using data from NASA’s Fermi Gamma-ray Space Telescope were able to look at distant blazars to help measure the background light from all the stars that are shining now and ever
  • Last time on SciByte
  • Breast Cancer & Mayan Calender | SciByte 69 (October 30, 2012
  • The low down
  • This enabled the most accurate measurement of starlight throughout the universe, which in turn helps establish limits on the total number of stars that have ever shone.
  • The optical and ultraviolet light from stars continues to travel throughout the universe even after the stars cease to shine
  • Fossil radiation field we can explore using gamma rays from distant sources and also provide a stellar density in the cosmos of about 1.4 stars per 100 billion cubic light-years, which means the average distance between stars in the universe is about 4,150 light-years
  • Significance
  • Blazars, which are among the most energetic phenomena in the universe. They are galaxies powered by extremely energetic black holes:
  • To gamma rays, the EBL functions as a kind of cosmic fog, but Fermi measured the amount of gamma-ray absorption in blazar spectra
  • Gamma rays produced in blazar jets travel across billions of light-years to Earth
  • Occasionally, a gamma ray collides with starlight and transforms into an electron and its antimatter counterpart, a positron
  • Once this occurs, the gamma ray light is lost much the same way as fog dims a distant lighthouse.
  • From studies of nearby blazars, scientists have determined how many gamma rays should be emitted at different energies
  • Which gives an upper and lower limit on the amount of stars that have formed
  • Previous estimates have only been an upper limit, this data shows that the upper and lower limits are very close to each other
  • Of Note
  • Measuring the extragalactic background light was one of the primary mission goals for Fermi
  • While Fermi is providing us with a shadow image of the first stars, whereas Webb will directly detect them
  • Multimedia
  • YouTube NASA | Fermi Explores the Early Universe
  • The locations of 150 blazars (green dots) used in the a new by the Fermi Gamma-Ray Telescope. | NASA/DOE/Fermi LAT Collaboration
  • Further Reading / In the News
  • Fermi Measures Light from All the Stars That Have Ever Existed | UniverseToday
  • Light From Universe’s First Stars Seen | Fermi Telescope | Space.com
  • Astronomers spot leftover light from ancient stars | Atom & Cosmos | Science News

— Viewer Feedback —

  • Educational Experience
  • Jusitn Luna asks about my Educational experience, in regards to school applications
  • Graduated with a BA in Physics, minoring in Astrophysics
  • Did all the volunteer work and internships I could both related and unrelated to school
  • Pay careful attention to all resume’s, mistakes creep in very easily, ask someone to look it over
  • What is pertinent to what you are applying for and check the details
  • If you have to do interviews practice
  • New ”Super-Earth” found
  • Michael Henriques pointed out a story about a new “Super Earth” found
  • That story is actually on the docket for next week

– CURIOSITY UPDATE –

  • Returning to Earth time
  • After three months working on “Mars time,” the team operating NASA Mars rover Curiosity has switched to a Earth schedule as planned
  • A Martian day, called a sol, is about 40 minutes longer than an Earth day, so the team’s start time for daily planning has been moving a few hours later each week
  • Telecommuting Teams Start
  • In addition more than 200 non-JPL scientists who have spent some time working at JPL since Curiosity’s landing will now continue participating regularly from their home institutions throughout North America and Europe
  • The team has been preparing in recent weeks to use dispersed participation teleconferences and Web connections.
  • X-Ray Analysis
  • Results of the first analysis of Martian soil by the Chemistry and Mineralogy (CheMin) experiment on NASA’s Curiosity rover show the presence of crystalline feldspar, pyroxenes and olivine mixed with some amorphous (non-crystalline) material
  • This makes is similar to volcanic soils in Hawaii
  • NASA’s Mars rover Curiosity has completed initial experiments showing the mineralogy of Martian soil is similar to weathered basaltic soils of volcanic origin in Hawaii
  • The teams used its Chemistry and Mineralogy instrument (CheMin) for quantitative results and new identifications of the minerals in this first X-ray diffraction analysis on Mars
  • Identification of minerals in rocks and soil is crucial for the mission’s goal to assess past environmental conditions and the mineral records the conditions under which it formed.
  • The composition of a rock provides only ambiguous mineralogical information, minerals diamond and graphite, which have the same chemical composition, but strikingly different structures and properties
  • CheMin uses X-ray diffraction, which provides more accurate identifications of minerals than any method previously used on Mars it reads minerals’ internal structure by recording how their crystals distinctively interact with X-rays
  • The sample was processed through a sieve to exclude particles larger than 0.006 inch (150 micrometers), roughly the width of a human hair.
  • The soil material CheMin has analyzed is more representative of modern processes on Mars
  • So far materials Curiosity has analyzed are consistent with our initial ideas of the deposits in Gale Crater recording a transition through time from a wet to dry environment
  • Multimedia
  • YouTube Curiosity Rover Report (Nov. 1, 2012): First CheMin Results | JPLNews
  • Image Galleries at JPL and Curiosity Mulimedia
  • Social Media
  • Curiosity Rover @MarsCuriosity
  • Further Reading / In the News
  • Curiosity rover finds clues to changes in Mars’ atmosphere | UniverseToday.com
  • NASA rover’s first soil studies help fingerprint Martian minerals | phys.org
  • Why Mars Life Hunt Targets Methane | Space.com
  • Curiosity rover finds clues to changes in Mars’ atmosphere | phys.org
  • Curiosity Finds Methane on Mars, or Not – ScienceNOW | ScienceMag.org
  • Curiosity team switches back to Earth time | phys.org

SCIENCE CALENDAR

Looking back

  • Nov 09, 1965 | 47 years ago | Blackout | The biggest electricity grid failure in U.S. history at the time caused a 13-hour blackout in northeast America and parts of Canada. The power lines from Niagara Falls to New York City were operating near their maximum capacity. At about 5:15 pm, a transmission line relay failed. Now there was insufficient line capacity for New York City. New England and New York are interconnected on a power grid, and the power that had been flowing toward New York City had to go elsewhere, instantly. Unable to handle this overload, generator operators shutdown to protect their equipment. Almost the entire grid failed, affecting 80,000 square miles, and 25 million people. In the subways of New York, 800,000 people were trapped

Looking up this week

Solar and Lunar Eclipses

  • Solar Eclipse
  • On Nov. 13, residents of northeastern Australia will get a ‘false-start’ sunrise
  • About an hour after the sun breaks the horizon in the coastal city of Cairns, it will be fully obscured by the moon, whose shadow will darken the sky and bring the stars back into view for 2 minutes there
  • The solar corona should take on a ‘wound up’ circular shape, with a high potential for tongues of pink nuclear fire leaping from the Sun’s edge
  • A three-man crew will be capturing and broadcasting the solar eclipse live with a telescope in northern Australia, which will be the only land area that will witness the total eclipse
  • Parts of New Zealand and Chile will see the sun partially obscured as the moon crosses the sky
  • Lunar Eclipse
  • A lunar eclipse that will take place on Nov. 28.
  • The penumbral lunar eclipse will manifest as a slight but noticeable darkening of the northern half of the moon; the dimming should be easily visible to the naked eye after most of the moon has dipped into the Earth’s penumbra
  • The Eastern United States will miss out on the lunar eclipse, as the moon will already have set there when the eclipse begins
  • The rest of the country can watch at least part of it, with the duration of visibility longest for people on the West Coast and in Alaska
  • Use THIS NASA GRAPHIC to check if you’ll be able to watch the lunar eclipse from their backyard.
  • Multimedia
  • Watch the Nov. 13 Solar Eclipse webcast for free starting at 2:30 p.m. Eastern Standard Time LIVE FEED
  • Lunar eclipse location graphic IMAGE
  • Further Reading / In the News
  • Total Solar Eclipse and Minor Lunar Eclipse to Grace Nov. Skies | Space.com

The post Painful Math & Canadian Rovers | SciByte 70 first appeared on Jupiter Broadcasting.

]]>