Beautiful! :)

Beautiful!!!

The Pleiades in Infrared 

WOW! Yep, an amazing #lightning strike! :)

Southern Maryland Lightning Storm by Keith Burke

Beautiful #lightning shot!

Solar System: Things to Know  This Week

This week, we’re looking at MAVEN’s exploration of Mars, the Orionid meteor showers, Mercury’s “great valley” and more.

1. Celebrating MAVEN

MAVEN, the Mars Atmospheric and Volatile Evolution, was the second mission selected for our Mars Scout program and the first to explore the planet’s upper atmosphere . It launched on November 18, 2013 and entered orbit around Mars on September 21, 2014. 

+ MAVEN Quick Facts

2. Jupiter Moon Dance

This time-lapse sequence of Hubble Space Telescope images shows Jupiter’s moon Europa as it moved across the planet’s face over the course of 19 minutes. Europa is at the bottom center on Jupiter’s disk, the Great Red Spot to the left and Europa’s shadow to its right. The video was created by combining six snapshots taken in ultraviolet light with Hubble’s Wide Field Camera 3.

+ Learn more

3. The Orionid Meteor Shower

Orionid shower peaks November 28. Look for the constellation Orion in the Southeast sky by 9 p.m. Using binoculars, look for the Orion Nebula. 

4. Comet Warming Up!! 

Comet 45P/Honda-Mrkos-Pajdu áková will brighten to expected stunning binocular visibility in mid to late December, but is near Venus on November 23rd.

+ Track the Comet

5. Mercury’s “Great Valley”

A newly discovered “great valley” in the southern hemisphere of Mercury provides more evidence that the planet closest to the sun is shrinking. Using stereo images from our MESSENGER spacecraft to create a high-resolution map, scientists have discovered that revealed the broad valley – more than 620 miles (1,000 kilometers) long – extending into the Rembrandt basin, one of the largest and youngest impact basins on Mercury. About 250 miles (400 kilometers) wide and 2 miles (3 kilometers) deep, Mercury’s great valley is smaller than Mars’ Valles Marineris, but larger than North America’s Grand Canyon and wider and deeper than the Great Rift Valley in East Africa.

+ Learn more

Discover the full list of 10 things to know about our solar system this week HERE.

Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com

These new type of satellites are revolutionizing how scientists will keep an eye on the Earth for years to come!  Check out the CYGNSS one!  :) 

6 Tiny Satellites That Are Changing How We See Earth

HARP: Hyper-Angular Rainbow Polarimeter

What’s better than taking a picture of a cloud to figure out its size and shape? Taking a bunch of pictures all around it. That way you get a three-dimensional view without having to worry about missing something. The HARP CubeSat is going to do just that: make observations of cloud droplets and tiny airborne particles like soot and dust with a modified camera lens from multiple angles. This will give us a full rendering of what’s going on inside the clouds, specifically, how those airborne particles act as “seeds” for water vapor to condense on and form cloud droplets. Since so many of those particles are in the air as a result of man-made pollution, we want to understand how they may be affecting clouds, weather and climate.

RAVAN: Radiometer Assessment using Vertically Aligned Nanotubes

Anyone who’s worn a black shirt on a summer day knows how much sunlight and heat it absorbs. The RAVAN 3-unit CubeSat, however, carries “blacker than black” technology – carbon nanotubes set up like a bundle of drinking straws that suck up nearly all the sunlight and energy that reach them to the point that your black shirt seems merely dark grey in comparison. Flying in low Earth orbit, RAVAN’s super sensitive instrument will detect tiny changes in the amount of sunlight and energy passing into and out of the top of the atmosphere. The amount of energy passing through the top of the atmosphere is where the net accounting of Earth’s energy budget happens – one of the major measurements we need in order to understand the effects of greenhouse gases on global warming and climate change. 

MiRaTA: Microwave Radiometer Technology Acceleration

That long skinny piece coming out of the bottom right side under the solar panel? That’s a measuring tape. It’s doubling as a communications antenna on the MiRaTA CubeSat that will be a mini-weather station in space. This 3-unit, shoe box-sized satellite is testing out new, miniaturized technology to measure temperature, water vapor, and cloud ice in the atmosphere. They’ll be tracking major storms, including hurricanes, as well as everyday weather. If this test flight is successful, the new, smaller technology will likely be incorporated into major – large – weather satellite missions in the future that are part of our national infrastructure.

IceCube

The aptly named IceCube will measure – you guessed it – ice in our atmosphere. Unlike the droplets that make up rain, ice is one of the harder things to measure from space. IceCube is a 3-unit CubeSat about the size of a loaf of bread outfitted with a new high-frequency microwave radiometer, an instrument that measures naturally occurring radiation emitted by stuff in the atmosphere – cloud droplets, rain, and the ice particles at the tops of clouds. This will be the first space test of the new microwave radiometer that has to balance its tiny size and low power with being sensitive enough to detect cloud ice. 

CYGNSS: Cyclone, Global Navigation Satellite System

What do GPS signals do when they’re not talking to your phone? A lot of them are just bouncing harmlessly off the planet’s surface – a fact that the CYGNSS mission is taking advantage of to measure wind speed over the ocean. Eight identical small satellites, each about the size of a microwave oven, flying in formation carry custom modified GPS receivers pointed at the oceans. When the water is smooth – not windy – the GPS signals reflect back uniformly, like the moon on a pond reflected as if in a mirror. When the water is choppy – windy – the signals reflect back in in the same direction but distorted, like the moon reflection on a choppy pond being distorted by ripples. Flying eight satellites in formation means the CYGNSS mission can measure wind speed across more of the ocean at once, which will help with understanding tropical storms and hurricanes. 

TROPICS: Time-Resolved Observations of Precipitation structure and storm Intensity with a Constellation of Smallsats

An important way to improve forecasts of hurricane and tropical cyclone intensity is to see what’s going on inside and around them while they’re happening. That’s the goal of the TROPICS mission, 12 CubeSats that will fly in formation to track the temperature and humidity of storm environments. The TROPICS CubeSats will get very frequent measurements, similar to X-rays, that cut through the overall cloud-cover so we can see the storm’s underlying structure. The storm structures known as the eyewall – tall clouds, wind and rain around the eye – and rainbands – the rainy parts of the spiral arms – give us clues about whether a storm is primed to intensify into a category 4 or 5 storm, something everyone in their path needs to know.

Learn more the world of small satellites at: https://www.nasa.gov/mission_pages/smallsats

Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com

Excellent! #nature #milkyway

Milky Way above Crater Lake National Park, Oregon | by Sean Pierce

So exciting!!  GOES-R scheduled for launch today (11/19) at 542 PM EST.  Great new technology, improved imagery, MORE imagery, NEW total lightning detection, and much more.  Learn more about GOES-R by visiting                  www.goes-r.gov . 

You can watch the launch on NASA TV.  Check your local cable/satellite provider or you can watch online through USTREAM or via nasa.gov ‘s NASA TV website.  Enjoy! 

READY FOR LAUNCH: CU BOULDER INSTRUMENT SUITE TO ASSESS SPACE WEATHER

A multimillion dollar University of Colorado Boulder instrument package expected to help scientists better understand potentially damaging space weather is now slated to launch aboard a National Oceanic and Atmospheric Administration satellite on Saturday, Nov. 19.

Designed and built by CU Boulder’s Laboratory for Atmospheric and Space Physics (LASP), the instrument suite known as the Extreme Ultraviolet and X-ray Irradiance Sensors (EXIS) is the first of four identical packages that will fly on four NOAA weather satellites in the coming decade. EXIS will measure energy output from the Sun that can affect satellite operations, telecommunications, GPS navigation and power grids on Earth as part of NOAA’s next-generation Geostationary Operational Environmental Satellites-R Series (GOES-R).

“We are ready for launch and are looking forward to a successful mission,” said LASP Senior Research Scientist Frank Eparvier, principal investigator on the EXIS project. “These extremely sensitive instruments will help scientists better understand solar events and help to mitigate the effects of space weather on Earth.”

NASA’s contract with CU Boulder on behalf of NOAA to design, build, test, deliver and scientifically support the four instrument packages is for roughly $105 million. The GOES-R satellite was built by Lockheed Martin Space Systems Co. in Littleton, Colorado and will be launched on an Atlas V rocket built by United Launch Alliance, headquartered in Centennial, Colorado.

EXIS consists of two LASP instruments, including XRS, an X-ray sensor that can determine the strength of solar flares and provide rapid alerts to scientists, said Eparvier. Large solar flares, equivalent to the explosion of millions of atomic bombs, can trigger “proton events” that send charged atomic particles flying off the Sun and into Earth’s atmosphere in just minutes. They can damage satellites, trigger radio blackouts and even threaten the health of astronauts by penetrating spacecraft shielding, he said.

“The XRS gives the first alert that a solar flare is occurring, providing NOAA with details on its timing, magnitude and direction within seconds,” said Eparvier.

The second EXIS instrument, EUVS, will monitor solar output in the extreme ultraviolet portion of the electromagnetic spectrum, which is completely absorbed by Earth’s upper atmosphere, said Eparvier. When the extreme UV light wavelengths penetrate the upper atmosphere during active periods on the Sun, they can break apart, ionize and change the properties of the atmosphere through which satellites fly and radio waves propagate.

Fluctuations in extreme UV wavelengths from the Sun ionize the upper atmosphere and interfere with communications like cell phones and GPS signals, said Eparvier. In addition, such fluctuations can create satellite drag, causing spacecraft to slowly fall out of orbit and burn up months or years before such events are anticipated.

“Modern technology has made us vulnerable to extreme variations in space weather that can have significant effects on Earth communications,” Eparvier said. “Extreme solar activity can cause problems for power companies all around the world, for example, in part because they all are interconnected.”

NOAA’s GOES satellites are a series of weather satellites that help scientists make timely and accurate weather forecasts. Two GOES satellites are now in geostationary orbit at a height of about 22,000 miles, with one focusing on the east part of the Americas overlapping with another focusing on the west. Satellites in geostationary orbits complete one revolution in the same amount of time it takes for the Earth to rotate once on its polar axis, allowing them to “stare” at a portion of Earth, said Eparvier.

LASP also built key solar instruments for NASA’s Van Allen Probes mission launched in 2012 to study Earth’s radiation belts, and designed and built a $32 million instrument package for NASA’s Solar Dynamics Observatory that launched in 2010.

More than 100 LASP personnel ranging from scientists and engineers to technicians, programmers and students have worked on the EXIS program since 2006. CU Boulder’s LASP will support EXIS on the four NOAA GOES satellite missions through spacecraft integration, testing, launch and commissioning, said Eparvier.

Each instrument package, roughly the size of a large microwave oven and weighing 66 pounds, is three times heavier than normal due to extra shielding that protects them from high-energy particle penetration. LASP’s Mike Anfinson is the EXIS project manager.

Lovely #lightning shot!!! #weather #sky

tropical sky by Alexandr Popovsky

Wow is right!! Great composite! #lightning

Сomposite shot of a thunderstorm in Gurgaon (India) on April 5, 2017. Here are 89 photos! WOW! credit: Jan Wellmann