A new map of wind patterns is so visually stunning it’s easily mistaken for art.
This interactive visualization of wind patterns — modeled from the U.S. National Weather Service’s Global Forecast System database — provides nearly current weather conditions on the global scale. And it’s beautiful.
In an interactive form, this data set allows the user to move the globe around (simply drag with your mouse) and zoom in and out (use your scroll wheel). After a few seconds the colors appear in snaking lines, depicting wind patterns at varying speeds. Gentle breezes are thin lines of green, strong winds are light streaks of yellow, and the strongest current are thick lines of red and purple.
A screen capture of the Earth’s north pole at 5,500 meters. The thick purple line is the polar jet stream.
Adjustable parameters also allow the user to view the wind patterns at various heights in the atmosphere, from 100 meters (noted as 1000 hPa in the program) to 26,500 meters (10 hPa) above the Earth’s surface. Simply click on the word “earth” in the lower left-hand corner of the web browser.
At the surface the map is a mirage of blue and green — with fairly gentle wind patterns in green. Circling patterns over the oceans are cyclones. They rotate clockwise over the southern Indian ocean and counter-clockwise over the northern Pacific ocean. If you turn your eyes toward land, you can compare the light summer winds across Australia with the swirling gusts off the northeast coast of Japan.
But you can also graze the jet streams, where thick bands of purple and red dance among the less violent green and yellow streaks. The wavy polar jet stream is entering the U.S. near Seattle, dropping southward near the Rocky Mountains, and then turning northward again just beyond the Great Lakes. It creates a temperature boundary, where south of the jet stream is warm and north of the jet stream is cold.
Users can view seven different altitudes using eight different map projections. This surprising new look at our own world is stunning in its artistic and educative beauty.
Before and after views of the March 17, 2013 impact taken by the LRO camera. Credit: NASA/GSFC/Arizona State University
Where there’s smoke, there’s fire, or in this instance, a new hole in the moon. NASA’s Lunar Impact Monitoring Program recorded the brightest meteoroid impact ever in its 8-year history on March 17 this year. The flash of light, as luminous as a 4th magnitude star and lasting about one second, was caught on video striking the moon in the Sea of Rains (Mare Imbrium) not far from the prominent crater Copernicus. Some time after the event, the Lunar Reconnaissance Orbiter(LRO) swept in for a closer look and spied a brand new impact crater.
Since 2005 the program has detected over 300 flashes which are presumed to be from meteoroid impacts.
Bright impact flash made by a foot-wide rock that struck the moon on March 17, 2013. The moon was a crescent in the evening sky at the time. The impact occurred in the dark, earthlit part of the moon away from the sun-lit crescent. Click photo to see video about the event. Credit: NASA
Based on the flash brightness and duration of the St. Pat’s Day smack, the space boulder measured between one to 1.5 feet long (0.3-0.4 meters) and struck the moon traveling at 56,000 mph with a force of 5 tons of TNT. Scientists predicted then that the impact could produce a crater up to 65 feet (20 meters) in diameter.
Left: Fresh material brought to the surface makes the new 59-foot-wide crater look like it was spray painted white. Credit: NASA/GSFC/Arizona State University. Right: The meteoroid strike occurred near the familiar crater Copernicus in the Sea of Rains (Mare Imbrium). Credit: Bob King
Well, guess what? When LRO dropped by for a look and compared images taken of the flash site before and after March 17. Staring it in the face was a brand new crater 59 feet across (18 meters). Wow! Just look at how reflective the crater and its rays of ejecta appear. That’s all unweathered, fresh dust and rock excavated from beneath the surface courtesy of 5 tons of extraterrestrial TNT. While impressive from LRO’s 31-mile altitude, the “St. Pat” crater is unfortunately invisible in even the largest telescopes from Earth.
Over time, cosmic rays, solar irradiation and micrometeoroids darken and redden the lunar soil. Millions of years from now, the once brilliant crater will blend into the moonscape. Can you imagine how bright larger craters like Tycho and Copernicus must have looked once upon a time?
Now it’s the Chinese Yutu rover’s turn to take a photo of the lander. Credit: CCTV
The March 17 impact wasn’t the first new crater seen by LRO, but it does appear to be one of the largest. The LRO camera team has been systematically searching its archive of before and after images for many more lunar landscape changes. Some of those results – including these photos – were presented at the American Geophysical Union Fall Meeting last week; more new craters will be announced in the near future.
Left: The lander’s new location in northern Mare Imbrium. Right: LRO scientists have so far nailed down the lander’s position somewhere inside the red box on the rim of a small crater with exposed rocky outcrops. Picture is about 1,750 feet side to side. Credit: NASA
While we’re on the topic of flyover discoveries, NASA will photograph the Chinese Yutu rover and lander when LRO orbits over western Mare Imbrium on Dec. 24 and 25. As it turns out, the lander didn’t land in Sinus Iridium as reported earlier but in nearby Mare Imbrium, a good distance east of the original site but still within the official “landing box”.
Fortuitously, this location turns out to be a great spot to examine young lavas not sampled during the Apollo missions. All the Apollo rocks ranged in age from 3.1 to 3.8 billion years old. Based on crater counts and the flow’s relatively fresh appearance, Yutu sits at the northern edge of a lava sheet dated at between 1 and 2.5 billion years. In lunar years, that’s fresh!
Flow lobes in the lavas of Mare Imbrium. Chang’e 3 landed at the extreme northern end of this sequence of lavas, which are very young in lunar terms. Credit: NASA / Apollo 15
Younger flows experience less erosion, so the lunar bedrock isn’t buried beneath as much rock as at the Apollo sites. Where Yutu sits, the lunar soil or regolith goes down some 6-7 feet (2 meters) instead of 10-26 feet (3-8 meters) at other landing sites. That means easier excavation of much sought after lunar bedrock. We may even be seeing blocks of bedrock littered about the ~35 foot wide crater (10 meters) in one of the first photos sent back to Earth by the Chinese lander.
The boulders strewn about the crater rim at the Chang’e 3 landing site might be samples of lunar bedrock. Credit: CCTV
For a great analysis of the Chang’e 3 landing site, I recommend reading A New Site to Explore on the Moonby lunar geologist Paul D. Spudis
The Expedition 38 crew tests spacesuits in preparation for December spacewalks to replace a pump for the International Space Station's cooling system. In the spacesuits are NASA astronauts Mike Hopkins (left) and Rick Mastracchio. Japanese astronaut Koichi Wakata is in the foreground, with Russian commander Oleg Kotov behind. Credit: NASA TV
The week before Christmas will be full of spacewalk preparations for Expedition 38 as they get ready to remove and replace a malfunctioning pump aboard the International Space Station.
NASA astronauts Rick Mastracchio and Mike Hopkins will participate in the spacewalks, NASA said today (Dec. 17), with Japanese astronaut Koichi Wakata handling robotic operations during the Dec. 21, Dec. 23 and Dec. 25 activities.
A new pump is needed to regulate temperatures in an external ammonia cooling loop that shut down automatically Wednesday (Dec. 11) when it got too cold. The loop keeps equipment at the right temperature on station. While the astronauts have been fine for the past week, several redundant systems and some experiments are offline. Luckily for the crew, other astronauts previously installed three spare pumps on station, which you can see in the graphic below.
Locations of spare pumps on the International Space Station as of December 2013. Credit: NASA
Spacewalks are always a risky proposition, and NASA has not conducted any since Italian astronaut Luca Parmitano experienced a leak in an American spacesuit in July. As such, the agency spent several days trying to fix the cooling loop by other means.
A faulty control valve made the pump malfunction on Wednesday. The valve normally mixes warm ammonia that flows past external radiators on station with cooler ammonia that was put through those radiators. NASA first tried to control the valve from the ground, then focused its attention on an isolation control valve upstream from the pump that the agency hoped could serve as a backup. The isolation valve, however, was only designed to be closed or opened fully — not positioned in between.
As of 11 a.m. EST (4 p.m. UTC) today, NASA was working on a software patch to try to freeze the valve in different positions to manually regulate the flow of ammonia.
“The fidelity that we have here on the ground to precisely control when that valve starts moving and stops is on the order of about 0.2 seconds, 0.3 seconds, somewhere in that range. We really need the fidelity to be much higher than that,” said Judd Frieling, the Expedition 38 lead flight director, in an update on NASA Television.
“We need it to be on the order of 0.1 seconds. So the way we can reliably produce that is by putting some software on the computers on board that basically allows us to get that finer control. So engineers and coders, overnight, have been working on a software — we call it a patch — software fix, to one of the computers that controls that valve.”
NASA planned to upload the patch to the station this afternoon (EST) to see if it was possible to control the isolation valve by telling it to move, then cutting the power when it got to a certain spot. The agency did not say how successful that fix was, but will likely address that in a media briefing tomorrow at 3 p.m. EST (8 p.m. UTC).
Cooling problems have occurred on station before. The most recent failure was a leak in May, which the Expedition 35 crew fixed just days before some of the astronauts went home. A more prominent failure on the same cooling loop occurred in 2010, when Expedition 24 astronauts performed three spacewalks to replace a faulty pump.
Each of the three emergency spacewalks this month (Dec. 21, 23 and 25) will start at 7:10 a.m. EST (12:10 p.m. UTC) and take about 6.5 hours to perform, NASA added. The activities will be carried live on NASA Television, with coverage starting about an hour before each spacewalk is expected to begin.
A view outside the cupola of the ISS. Credit: NASA.
For the past 13 years, Google has put together their annual “Zeitgeist” lists — “signs of the times” as to what people around the world were interested in, as registered by the internet’s largest search engine. In this compilation video, released by Google today, you’ll see space exploration and astronomical events show up several times. At :17 in the “New Frontiers” section with Voyager 2 entering interstellar space; at :45 the Chelyabinsk meteor flashes across the screen, at :53 the Kirobo robot shows up, at 1:13 Curiosity rolls across Mars, and at 1:14 you can look out the cupola windows of the International Space Station in the “Inspiration” section. You can see what trended in the various charts here.
Antares Launch – Maximum Elevation Map The Antares nighttime launch will be visible to millions of spectators across a wide area of the Eastern US -weather permitting. This map shows the maximum elevation (degrees above the horizon) that the Antares rocket will reach during the Dec 19, 2013 launch depending on your location along the US east coast. Credit: Orbital Sciences
Antares Launch – Maximum Elevation Map
The Antares nighttime launch will be visible to millions of spectators across a wide area of the Eastern US -weather permitting. This map shows the maximum elevation (degrees above the horizon) that the Antares rocket will reach during the Dec 19, 2013 launch depending on your location along the US east coast. Credit: Orbital Sciences[/caption]
UPDATE: The launch of Cygnus has been delayed until no earlier than January 7, 2014 due to the coolant leak at the International Space Station and necessary spacewalks to fix the problem. You can read more about the issue here and here.
WALLOPS ISLAND, VA – Orbital Sciences Corp. is marching forward with plans for a spectacular night blastoff of the firms privately developed Antares rocket and Cygnus cargo spacecraft on Thursday, Dec. 19 from a seaside pad at Wallops Island, Virginia on a mission for NASA that’s bound for the International Space Station (ISS).
The nighttime Antares liftoff is currently scheduled for prime time – at 9:19 p.m. EST from Launch Pad 0A at the Mid-Atlantic Regional Spaceport (MARS) at NASA Wallops Island, Virginia. It should be easily visible to tens of millions of residents along a wide swath of the US East Coast spanning from South Carolina to southern Maine – weather permitting.
Here’s our guide on “How to See the Antares/Cygnus Dec. 19 Night Launch” – with your own eyes – complete with viewing maps and trajectory graphics from a variety of prime viewing locations; including Philadelphia, NYC, Baltimore and historic landmarks in Washington, DC.
Update: launch postponed to mid-January 2014 to allow NASA astronauts to conduct 3 EVA’s to swap out the ammonia pump module and restore full cooling capacity to the ISS
It will be visible to spectators inland as well, stretching possibly into portions of West Virginia and western Pennsylvania.
For example; Here’s the expected view from Rocky’s famous workout on the steps of the Philadelphia Art Museum.
Philadelphia
The viewing maps are courtesy of Orbital Sciences, the private company that developed both the Antares rocket and Cygnus resupply vessel aimed at keeping the ISS fully stocked and operational for science research.
Up top is the map showing the maximum elevation the rocket will reach in the eastern United States. Capitol-East-Front-Steps
The flight is designated the Orbital-1, or Orb-1 mission.
Orb-1 is the first of eight commercial cargo resupply missions to the ISS by Orbital according to its Commercial Resupply Services (CRS) contract with NASA.
Of course you can still view the launch live via the NASA TV webcast.
This marks the maiden night launch of the two stage Antares rocket following a pair of daytime test and demonstration launches earlier this year, in April and September.
It’s important to note that the Dec. 19 liftoff is still dependent on NASA engineers resolving the significant issue with the ammonia cooling system that popped up late last week when a critical flow control valve malfunctioned.
If the pump valve can’t be brought back online, two American astronauts may make two or three unscheduled spacewalks starting later this week.
So in the event spacewalks are required, Antares launch could still slip a few days to the end of the launch window around Dec. 21 or Dec. 22. Thereafter the launch would be postponed until January 2014.
Battery Park, NYC
Here’s your chance to witness a mighty rocket launch – from the comfort of your home and nearby locations along the east coast.
And its smack dab in the middle of the Christmas and holiday season resplendent with shining bright lights.
Weather outlook appears rather promising at this time – 95% favorable chance of lift off.
National Mall, Washington, DC
The rocket was rolled out to the Wallops launch pad this morning by Orbital’s technicians.
Cygnus is loaded with approximately 1465 kg (3,230 lbs.) of cargo for the ISS crew for NASA.
NASA Television coverage of the Antares launch will begin at 8:45 p.m. on Dec. 19 – www.nasa.gov/ntv
Stay tuned here for Ken’s Antares launch reports from NASA Wallops Flight Facility, VA.
Hubble image of variable star RS Puppis (NASA, ESA, and the Hubble Heritage Team)
6,500 light-years away in the southern constellation Puppis an enormous star pulses with light and energy, going through the first throes of its death spasms as it depletes its last reserves of hydrogen necessary to maintain a stable, steady radiance. This star, a Cepheid variable named RS Puppis, brightens and dims over a 40-day-long cycle, and newly-released observations with Hubble reveal not only the star but also the echoes of its bright surges as they reflect off the dusty nebula surrounding it.
The image above shows RS Puppis shining brilliantly at the center of its dusty cocoon. (Click the image for a super high-res version.) But wait, there’s more: a video has been made of the variable star’s outbursts as well, and it’s simply mesmerizing. Check it out below:
Assembled from observations made over the course of five weeks in 2010, the video shows RS Puppis pulsing with light, outbursts that are then reflected off the structure of its surrounding nebula. What look like expanding waves of gas are really “light echoes,” radiation striking the densest rings of reflective dust located at farther and farther distances from the star.
According to the NASA image description:
RS Puppis rhythmically brightens and dims over a six-week cycle. It is one of the most luminous in the class of so-called Cepheid variable stars. Its average intrinsic brightness is 15,000 times greater than our sun’s luminosity.
The nebula flickers in brightness as pulses of light from the Cepheid propagate outwards. Hubble took a series of photos of light flashes rippling across the nebula in a phenomenon known as a “light echo.” Even though light travels through space fast enough to span the gap between Earth and the moon in a little over a second, the nebula is so large that reflected light can actually be photographed traversing the nebula. (Source)
RS Puppis is ten times more massive than our Sun, and 200 times larger.
Cepheid variables are more than just fascinating cosmic objects. Their uncanny regularity in brightness allows astronomers to use them as standard candles for measuring distances within our galaxy as well as others — which is trickier than it sounds. Because of its predictable variation along with the echoing light from its surrounding nebula, the distance to RS Puppis (6,500 ly +/- 90) has been able to be calculated pretty accurately, making it an important calibration tool for other such stars. (Read more here.)
Full image credit: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)-Hubble/Europe Collaboration. Acknowledgment: H. Bond (STScI and Penn State University)
Bright, brighter, brightest: these views of Comet ISON after its closest approach to the sun Nov. 28 show that a small part of the nucleus may have survived the comet's close encounter with the sun. Images from the Solar and Heliospheric Observatory. Credit: ESA/NASA/SOHO/GSFC
When Comet ISON entered its zombie stage a few weeks ago, the effects were not only felt in the astronomical community, but also on astronomy tourists as the comet faded from the view of amateurs.
German company “Eclipse-Reisen” (Eclipse Travel) had to make a last-minute change in plans for a Dec. 8 flight for some 75 tourists planning to observe ISON, which morphed into a travelling dust blob after skimming too close to the sun in late November. Fortunately, Comet Lovejoy is still a strong astronomical object, providing an alternate thing to watch.
“Most of the passengers weren’t disappointed. They were more excited to see something new. Only a few journalists cancelled the flight. All photographers and experts fully understood the situation,” a statement from Air Partner to Universe Today said. (The spokespeople were German-speaking, requiring a translation by another party.)
Negative image taken Nov. 14 of Lovejoy’s nucleus and dust fan. Credit: Dr. P. Clay Sherrod
“Comet Lovejoy is no less spectacular and still very exciting like ISON and they were pleased to see it, actually. Although Lovejoy is less bright than ISON, it is weaker by four size classes, its tail is smaller and pale and Lovejoy flies farther past the Earth and the Sun.”
The company had to ask for permission to alter its flight path, and inform the passengers of the last-minute change, all in a few days, but officials added that the flight went off without a hitch.
You can read more information about the company (in German) on its website. In 2014, it plans to run a flight to observe auroras over Iceland, among others.
And if you’re interested in looking back, here’s an archive to all the past Carnivals of Space. If you’ve got a space-related blog, you should really join the carnival. Just email an entry to [email protected], and the next host will link to it. It will help get awareness out there about your writing, help you meet others in the space community – and community is what blogging is all about. And if you really want to help out, sign up to be a host. Send an email to the above address.
Artist's conception of Kepler-88. Credit: Center for Astrophysics of the University of Porto
Planets are so very tiny next to stars outside of the solar system, making it really hard to spot exoplanets unless they transit across the face of their star (or if they are very, very big). Often, astronomers can only infer the existence of planets by their effect on the host star or other stars.
That’s especially true of the curious case of Kepler-88 c, which researchers using the Kepler space telescope said was a possible planet due to its effects on the orbit of Kepler-88 b, a planet that goes across the host of its host star. European astronomers just confirmed the Kepler data using the SOPHIE spectrograph at France’s Haute-Provence Observatory.
It’s the first time scientists have successfully used a technique to independently verify a planet’s mass based on what was found from the transit timing variation, or how a planet’s orbit varies from what is expected as it goes across the face of its sun. That means TTV can likely be used as a strong method on its own, advocates say.
Illustration of the Kepler spacecraft (NASA/Kepler mission/Wendy Stenzel)
SOPHIE’s technique relies on measuring star velocity, which also can reveal a planet’s mass by seeing its effect on the star.
“This independent confirmation is a very important contribution to the statistical analyzes of the Kepler multiple planet systems,” stated Magali Deleuil, an exoplanet researcher at Aix-Marseille University who participated in the research. “It helps to better understand the dynamical interactions and the formation of planetary systems.”
Actually, the two planets behave similarly to Earth and Mars in our own solar system in terms of orbits, according to work from a previous team (led by David Nesvorny of the Southwest Research Institute). They predicted the planets have a two-to-one resonance, which is approximately true of our own solar system since Mars takes about two Earth years to orbit the sun.
The theory of Lithopanspermia states that life can be shared between planets within a planetary system. Credit: NASA
With the recent discovery that Europa has geysers, and therefore definitive proof of a liquid ocean, there’s a lot of talk about the possibility of life in the outer solar system.
According to a new study, there is a high probably that life spread from Earth to other planets and moons during the period of the late heavy bombardment — an era about 4.1 billion to 3.8 billion years ago — when untold numbers of asteroids and comets pummeled the Earth. Rock fragments from the Earth would have been ejected after a large meteoroid impact, and may have carried the basic ingredients for life to other solar system bodies.
These findings, from Pennsylvania State University, strongly support lithopanspermia: the idea that basic life forms can be distributed throughout the solar system via rock fragments cast forth by meteoroid impacts.
Strong evidence for lithopanspermia is found within the rocks themselves. Of the over 53,000 meteorites found on Earth, 105 have been identified as Martian in origin. In other words an impact on Mars ejected rock fragments that then hit the Earth.
The researchers simulated a large number of rock fragments ejected from the Earth and Mars with random velocities. They then tracked each rock fragment in n-body simulations — models of how objects gravitationally interact with one another over time — in order to determine how the rock fragments move among the planets.
“We ran the simulations for 10 million years after the ejection, and then counted up how many rocks hit each planet,” said doctoral student Rachel Worth, lead author on the study.
Their simulations mainly showed a large number of rock fragments falling into the Sun or exiting the solar system entirely, but a small fraction hit planets. These estimations allowed them to calculate the likelihood that a rock fragment might hit a planet or a moon. They then projected this probability to 3.5 billion years, instead of 10 million years.
In general the number of impacts decreased with the distance away from the planet of origin. Over the course of 3.5 billion years, tens of thousands of rock fragments from the Earth and Mars could have been transferred to Jupiter and several thousand rock fragments could have reached Saturn.
“Fragments from the Earth can reach the moons of Jupiter and Saturn, and thus could potentially carry life there,” Worth told Universe Today.
The researchers looked at Jupiter’s Galilean satellites: Io, Europa, Ganymede and Callisto and Saturn’s largest moons: Titan and Enceladus. Over the course of 3.5 billion years, each of these moons received between one and 10 meteoroid impacts from the Earth and Mars.
It’s statistically possible that life was carried from the Earth or Mars to one of the moons of Jupiter or Saturn. During the period of late bombardment the solar system was much warmer and the now icy moons of Saturn and Jupiter didn’t have those protective shells to prevent meteorites from reaching their liquid interiors. Even if they did have a thin layer of ice, there’s a large chance that a meteorite would fall though, depositing life in the ocean beneath.
In the case of Europa, six rock fragments from the Earth would have hit it over the last 3.5 billion years.
It has previously been thought that finding life in Europa’s oceans would be proof of an independent origin of life. “But our results suggest we can’t assume that,” Worth said. “We would need to test any life found and try to figure out whether it descended from Earth life, or is something really new.”
The paper has been accepted for publication in the journal Astrobiology and is available for download here.
