In March, Jupiter, it’s moons and moon shadows will all be visible in the sky. Find out when and where to look up:
Jupiter dominates the evening sky this month, rising at sunset and setting at dawn. On March 8, Jupiter reaches what is called “opposition”. Imagine that Jupiter and the sun are at opposite ends of a straight line, with the Earth in between. This brings Jupiter its closest to Earth, so it shines brighter and appears larger in telescopes.
On the nights of March 14 – 15, March 21 – 22 and March 29, two of Jupiter’s moons will cross the planet’s disk.
When the planet is at opposition and the sun shines on Jupiter’s moons, we can see the moon’s shadow crossing the planet. There are actually 11 of these double shadow transits in March!
The next six months will be awesome times for you to image Jupiter when it’s highest in the sky; near midnight now, and a little earlier each night through the late summer.
Even through the smallest telescopes or binoculars, you should be able to see the two prominent belts on each side of Jupiter’s equator made up of the four Galilean moons: Io, Europa Ganymede and Calisto. If you have a good enough view, you may even see Jupiter’s Red Spot!
Our Juno spacecraft will arrive at Jupiter on July 4th of this year and will go into orbit around the giant planet. Right now, the Juno mission science team is actively seeking amateur and professional images of the planet. These images are uploaded to a Juno website, and the public is invited to discuss points of interest in Jupiter’s atmosphere.
Locations will later be voted on and the favorites will be targets for JunoCam, the spacecraft’s imaging camera. Once JunoCam has taken the images, they’ll be posted online. Imaging participants can then process these raw mission images and re-upload them for others to view.
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What a way to spend Christmas!
Inhabitat’s Week in Green: Paris climate talks, and more!
Consider the following:
1) No known species of reindeer can fly. But there are 300,000 species of living organisms yet to be classified, and while most of these are insects and germs, this does not COMPLETELY rule out flying reindeer which only Santa has ever seen.
2) There are 2 billion children (persons under 18) in the world. BUT since Santa doesn’t (appear) to handle the Muslim, Hindu, Jewish and Buddhist children, that reduces the workload to 15% of the total - 378 million according to Population Reference Bureau. At an average (census) rate of 3.5 children per household, that’s 91.8 million homes. One presumes there’s at least one good child in each.
3) Santa has 31 hours of Christmas to work with, thanks to the different time zones and the rotation of the earth, assuming he travels east to west (which seems logical).
This works out to 822.6 visits per second. This is to say that for each Christian household with good children, Santa has 1/1000th of a second to park, hop out of the sleigh, jump down the chimney, fill the stockings, distribute the remaining presents under the tree, eat whatever snacks have been left, get back up the chimney, get back into the sleigh and move on to the next house.
Assuming that each of these 91.8 million stops are evenly distributed around the earth (which, of course, we know to be false but for the purposes of our calculations we will accept), we are now talking about .78 miles per household, a total trip of 75-½ million miles, not counting stops to do what most of us must do at least once every 31 hours, plus feeding and etc.
This means that Santa’s sleigh is moving at 650 miles per second, 3,000 times the speed of sound. For purposes of comparison, the fastest man- made vehicle on earth, the Ulysses space probe, moves at a poky 27.4 miles per second - a conventional reindeer can run, tops, 15 miles per hour.
4) The payload on the sleigh adds another interesting element. Assuming that each child gets nothing more than a medium-sized lego set (2 pounds), the sleigh is carrying 321,300 tons, not counting Santa, who is invariably described as overweight.
On land, conventional reindeer can pull no more than 300 pounds. Even granting that ‘flying reindeer’ (see point #1) could pull TEN TIMES the normal amount, we cannot do the job with eight, or even nine.
We need 214,200 reindeer. This increases the payload - not even counting the weight of the sleigh - to 353,430 tons. Again, for comparison - this is four times the weight of the Queen Elizabeth.
5) 353,000 tons traveling at 650 miles per second creates enormous air resistance - this will heat the reindeer up in the same fashion as spacecraft re-entering the earth’s atmosphere. The lead pair of reindeer will absorb 14.3 QUINTILLION joules of energy. Per second. Each.
In short, they will burst into flame almost instantaneously, exposing the reindeer behind them, and create deafening sonic booms in their wake. The entire reindeer team will be vaporized within 4.26 thousandths of a second.
Santa, meanwhile, will be subjected to centrifugal forces 17,500.06 times greater than gravity. A 250-pound Santa (which seems ludicrously slim) would be pinned to the back of his sleigh by 4,315,015 pounds of force.> In conclusion - If Santa ever DID deliver presents on Christmas Eve, he’s dead now.
(NOTE: This appeared in the SPY Magazine (January, 1990) )
Fusion power would completely revolutionize energy production on our planet. Indeed, it would reshape our entire world, allowing us to produce vast amounts of energy with little waste or cost. In essence, fusion reactors work by mimicking our Sun in that they fuse two hydrogen atoms into a single helium atom. Conversely, nuclear fission breaks a single atom into two atoms.
Ultimately, the fusion reaction releases ten times more energy per mass as our regular fission reactors, and it does so without all the harmful nuclear waste.
Unfortunately, such reactions come with a few problems. As University of Texas physicist Dr. Swadesh M. Mahajan notes, “Getting net energy from fusion is such a goddamn difficult undertaking. We know of no materials that would be able to handle anywhere near that amount of heat.”
Find out how scientists tackled that issue at: http://futurism.com/links/fusion-energy-these-promising-projects-are-set-to-revolutionize-our-world/
Scientists find “the holy grail of astronomy” after uncovering a galaxy that is made up of mostly dark matter
Mars will one day have a ring system due to Phobos, the planet’s small moon, being crushed by tidal forces
Blue Origin’s New Shepard rocket successfully launches to the edge of space and lands vertically back on Earth
A new exoplanet called GJ1132b is found 39 light-years away, making it the closest Earth-sized exoplanet ever discovered
Researchers make ultra-thin diamond nanothreads, which could help us build a space elevator
A blue Neptune-like exoplanet, which seems to have skies like Earth, is found orbiting a red dwarf star
A staggering 574 newly discovered massive galaxies are revealed that date back to the beginnings of the universe
New research shows that galaxies were far more efficient at making stars during the first 10% of history than they are now
So there’s this physics journal that uses math and science to discuss the realities of fictional universes in a super legit, peer-reviewed manner?
And they did a thing on Frozen?
Combining research on the film?
With info on how water works and stuff?
Then applied math and chemistry (and other things in which I am not especially well versed) to reach this conclusion:
So.
Rowing robot powers itself by gulping dirty water
New experiments are scheduled to arrive to the International Space Station with the launch of Orbital ATK’s Cygnus cargo spacecraft on Tuesday. These science payloads will study fires, meteors, regolith, adhesion and 3-D printing in microgravity.
What is it? What happens when you set a fire in space? The Spacecraft Fire Experiment-I (Saffire-I) will find out!
How does it work? This experiment will intentionally light a large-scale fire inside an empty Cygnus resupply vehicle after it leaves the space station and before it re-enters Earth’s atmosphere.
Why is it important? The Saffire-I investigation provides a new way to study a realistic fire on an exploration vehicle, which has not been possible in the past because the risks for performing studies on manned spacecraft are too high. Instruments on the returning Cygnus will measure flame growth, oxygen use and more.
What is it? A less heated investigation, Meteor Composition Determination (Meteor) will enable the first space-based observations of meteors entering Earth’s atmosphere from space. Meteors are somewhat rare and are difficult to monitor from the ground because of Earth’s atmosphere.
How does it work? This investigation uses high-resolution video and image analysis of the atmosphere to acquire the physical and chemical properties of the meteoroid dust, such as size, density and chemical composition.
Why is it important? Studying the elemental composition of meteors adds to our understanding of how the planets developed, and continuous measurement of meteor interactions with Earth’s atmosphere could spot previously unforeseen meteors.
What is it? A more “grounded” investigation will study the properties and behavior of regolith, the impact-shatterd “soil” found on asteroids, comets, the moon and other airless worlds.
How does it work? The Strata-1 experimental facility exposes a series of regolith simulants, including pulverized meteorite material, glass beads, and regolith simulants composed of terrestrial materials and stored in multiple transparent tubes, to prolonged microgravity on the space station. Scientists will monitor changes in regolith layers and layering, size sorting and particle migration via video images and close examination after return of the samples to Earth.
Why is it important? The Strata-1 investigation could give us new answers about how regolith behaves and moves in microgravity, how easy or difficult it is to anchor a spacecraft in regolith, how it interacts with spacecraft and spacesuit materials and other important properties.
What is it? From grounded to gripping, another investigation launching takes inspiration from small lizards. Geckos have specialized hairs on their feed called setae that let them stick to vertical surfaces without falling, and their stickiness doesn’t wear off after repeated use. The Gecko Gripper investigation tests a gecko-adhesive gripping device that can stick on command in the harsh environment of space.
How does it work? The gripping device is a material with synthetic hairs much like setae that are much thinner than a human hair. When a force is applied to make the tiny hairs bend, the positively charged part of a molecule within a slight electrical field attracts the negatively charged part of its neighbor resulting in “stickiness.” Once adhered, the gripper can bear loads up to 20 pounds. The gripper can remain in place indefinitely and can also be easily removed and reused.
Why is it important? Gecko Grippers have many applications on current and future space missions, including acting as mounting devices for payloads, instruction manuals and many other small items within the space station. In addition, this technology enables a new type of robotic inspection system that could prove vital for spacecraft safety and repair.
What is it? From adhesion to additive, the new Additive Manufacturing Facility (AMF) will also launch on the flight. Additive manufacturing (3D printing) is the process of building a part layer-by-layer, with an efficient use of the material.
How does it work? The AMF uses this technology to enable the production of components on the space station for both NASA and commercial objectives.
Why is it important? Parts, entire experiments and tools can be created on demand with this technology. The ability to manufacture on the orbiting laboratory enables on-demand repair and production capability, as well as essential research for manufacturing on long-term missions.
These sticky, stony and sizzling investigations are just a sampling of the wide range of science conducted on the orbiting laboratory that benefits future spaceflight and provides Earth-based benefits as well.
You can watch the launch of Orbital ATK’s Cygnus spacecraft online. Stream live coverage starting at 10 p.m. EDT on March 22. Launch is scheduled for 11:05 p.m., which is the start of a 30-minute launch window.
Watch online: nasa.gov/nasatv
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