To find the perfect perch for Earth observation research, just look up – about 240 miles up. The International Space Station serves as an optimal platform for studying our dynamic planet, where spectacular views support science.
With currently active instruments and facilities like High Definition Earth Viewing, Crew Earth Observations, Lightning Imaging Sensor, SAGE-III and Meteor, researchers on the ground are able to use the station’s unique (and useful!) vantage point to track Earth’s weather patterns, obtain images documenting changes on the planet’s surface, understand the origin of meteors falling towards Earth, and better understand the atmosphere.
The space station’s 90-minute orbit allows it to cover 90% of the Earth’s populated surfaces. That means we are able to study A LOT of that big blue marble.
Let’s talk a little about how the space station serves as a platform for Earth observation:
Each day, as the space station passes over regions of the Earth, crew members photograph the area below as a part of the Crew Earth Observations Facility investigation, one of the longest-running experiments on the orbiting laboratory. Crew members are able to photograph large-scale weather events like the recent Hurricane Harvey from the space station’s Cupola. These little science postcards from space can be used by researchers and the public to learn more about our home planet.
Want to see a picture of your hometown from space? Search for it in the Gateway to Astronaut Photography of Earth (GAPE).
The High Definition Earth Viewing (HDEV) experiment streams live video of Earth for online viewing. This investigation not only provides hours and hours of footage of the Earth below, but also demonstrates how the technology holds up against the harsh environment of space. High school students helped design some of the cameras' components, through the High Schools United with NASA to Create Hardware (HUNCH) program, and student teams perform most of the HDEV operation. (Whoa! Check out HUNCH and STEM on Station for more opportunities for student involvement!)
Useful for weather forecasting, hurricane monitoring, and observations of large-scale climate phenomena such as El Niño, RapidScat used radar pulses reflected off the ocean to measure wind speed and direction over the ocean.
RapidScat completed its successful two-year mission, outlasting its original decommission date before suffering a power loss. Although RapidScat is no longer transmitting data back to Earth, the station hosts many other Earth-observation tools the Cyclone Intensity Measurements from the ISS (CyMISS) an experiment that seeks to develop detailed information on tropical storm structure to better estimate storm intensity, which will help government agencies to better prepare communities for impending natural disasters; and the Cloud-Aerosol Transport System (CATS), a previously-flown lidar instrument which measured atmospheric profiles of aerosols and clouds to better understand their properties and interactions, as well as provided data useful to improving climate change models.
Learn more about RapidScat’s mission conclusion HERE! Take a look at CATS mission data HERE!
Watch more inspiring videos and learn about how we’re capturing the beauty of Earth HERE.
Crew members are able to photograph large-scale weather events like the recent Hurricane Harvey from the space station’s Cupola. These little science postcards from space can be used by researchers and the public to learn more about our home planet.
Plants in space!
Future long-duration missions into the solar system will require a fresh food supply to supplement crew diets, which means growing crops in space. Growing food in such a harsh environment also teaches us a little bit about growing in harsh environments here on Earth.
Here are a few plant-based investigations currently happening aboard the orbiting laboratory:
Veggie is a chamber on the space station that helps scientists grow, harvest and study different space crops. This experiment is called VEG-03D and they’ve been able to grow six rounds of crops so far.
SpaceX's 13th Commercial Resupply vehicle carried many valuable items to the orbiting laboratory, including Plant Gravity Perception, an investigation that uses the European Modular Cultivation System (EMCS) to simulate gravity to help plants grow its roots downward, and shoots upwards. The shoots need to face upwards, towards the light, so they can absorb sunlight and nutrients. Without this, plants wouldn’t know which way to grow. Yikes!
Learn more about Plant Gravity Perception HERE!
The Advanced Plant Habitat is a large chamber that supports commercial and fundamental plant research for at least one year of continuous use. A great feature to this habitat is that the astronauts can view the plant’s progress through a window on the door.
Whether astronauts are taking pictures of the planet or growing crops in space, all science aboard the space station plants seeds for a better life on Earth. Biology investigations directly grow our knowledge of agricultural techniques for harsh environments and imagery from space can give us a clearer idea of our planet’s health and emerging weather patterns.
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Almost thirty years ago, on Feb. 14, 1990, our Voyager 1 spacecraft turned back toward its home for one last look. 40 astronomical units (almost 4 billion miles) from the Sun, Voyager snapped the first-ever “family portrait” of our solar system.
One image in particular highlights our own planet’s fragility in the vast cosmic arena that we call home. This image of Earth, a tiny point of light, is contained in a camera artifact that resembles a beam of sunlight.
The late Carl Sagan referred to this image of Earth in the title of his 1994 book, Pale Blue Dot. Sagan wrote: "That's here. That's home. That's us. On it everyone you love, everyone you know, everyone you ever heard of, every human being who ever was, lived out their lives. … There is perhaps no better demonstration of the folly of human conceits than this distant image of our tiny world. To me, it underscores our responsibility to deal more kindly with one another, and to preserve and cherish the pale blue dot, the only home we've ever known.”
We placed a message aboard Voyager 1 and 2 — a kind of time capsule intended to communicate a story of our world to extraterrestrials. The Voyager message is carried by a phonograph record: a 12-inch gold-plated copper disk containing sounds and images selected to portray the diversity of life and culture on Earth.
The Golden Record includes 115 images and a variety of natural sounds, such as those made by surf, wind and thunder, birds, whales and other animals. Musical selections from different cultures and eras were also added, as well as spoken greetings from Earth-people in fifty-five languages and printed messages from President Carter.
The Golden Record represents the whole of humanity, mounted to a feat of human engineering on a long voyage through interstellar space.
You can listen to the sounds of Earth on the golden record here and take a moment to appreciate our pale blue dot.
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Ten years ago, on March 6, 2009, a rocket lifted off a launch pad at Cape Canaveral Air Force Station in Florida. It carried a passenger that would revolutionize our understanding of our place in the cosmos--NASA’s first planet hunter, the Kepler space telescope. The spacecraft spent more than nine years in orbit around the Sun, collecting an unprecedented dataset for science that revealed our galaxy is teeming with planets. It found planets that are in some ways similar to Earth, raising the prospects for life elsewhere in the cosmos, and stunned the world with many other first-of-a-kind discoveries. Here are five facts about the Kepler space telescope that will blow you away:
NASA retired the Kepler spacecraft in 2018. But to this day, researchers continue to mine its archive of data, uncovering new worlds.
*All images are artist illustrations. Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com
This weekend marks the 400th anniversary of Shakespeare’s death, and we’re highlighting the moons of Uranus; some of which are named after characters from his works.
While most of the moons orbiting other planets take their names from Greek mythology, Uranus’ moons are unique in bing named for Shakespearean characters, along with a couple of them being named for characters from the works of Alexander Pope.
Using the Hubble Space Telescope and improved ground-based telescopes, astronomers have discovered a total of 27 known moons around Uranus.
Shakespearean work: The Tempest
Miranda, the innermost and smallest of the five major satellites, has a surface unlike any other moon that’s been seen. It has a giant fault canyon as much as 12 times as deep as the Grand Canyon, terraced layers and surfaces that appear very old, and others that look much younger.
Shakespearean work: The Tempest
Ariel has the brightest and possibly the youngest surface among all the moons of Uranus. It has a few large craters and many small ones, indicating that fairly recent low-impact collisions wiped out the large craters that would have been left by much earlier, bigger strikes. Intersecting valleys pitted with craters scars its surface.
Shakespearean work: A Midsummer Night’s Dream
Oberon, the outermost of the five major moons, is old, heavily cratered and shows little signs of internal activity. Unidentified dark material appears on the floors of many of its craters.
Shakespearean works: Cordelia - King Lear; Ophelia - Hamlet
Cordelia and Ophelia are shepherd moons that keep Uranus’ thin, outermost “epsilon” ring well defined.
Between them and miranda is a swarm of eight small satellites unlike any other system of planetary moons. This region is so crowded that astronomers don’t yet understand how the little moons have managed to avoid crashing into each other. They may be shepherds for the planet’s 10 narrow rings, and scientists think there must be still more moons, interior to any known, to confine the edges of the inner rings.
Want to learn more about all of Uranus’s moons? Visit: http://solarsystem.nasa.gov/planets/uranus/moons
Check out THIS blog from our Chief Scientist Ellen Stofan, where she reflects on the life and legacy of William Shakespeare on the 400th anniversary of his death on April 23, 1616.
Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com
Our view from space shows our planet is changing, but to really understand the details of these changes and what they mean for our future, scientists need a closer look. Over the next six months, we’re taking you on a world tour as we kick off major new field research campaigns to study regions of critical change from land, sea and air.
You can follow the Earth Expeditions on Facebook, Twitter and their Blog.
CORAL (Coral Reef Airborne Laboratory)
This three-year CORAL mission will use advanced airborne instruments and in-water measurements to survey a portion of the world’s coral reefs. The mission will assess the conditions of these threatened ecosystems to better understand their relation to the environment, including physical, chemical and human factors. With a new understanding of reef condition, the future of this global ecosystem can be predicted.
OMG (Oceans Melting Greenland)
Oceans Melting Greenland (OMG) mission will pave the way for improved estimates of sea level rise by addressing the question: To what extent are the oceans melting Greenland’s ice from below? This mission will observe changing water temperatures and glaciers that reach the ocean around all of Greenland from 2015 to 2020. This year, the OMG mission will fly over the periphery of Greenland to take measurements of the heights and extents of Greenland’s coastal glaciers that reach the ocean and release expendable sensors to measure the temperature and salinity of coastal waters. The OMG field campaign will gather data that will help scientists both understand how the oceans are joining with the atmosphere in melting the vast ice sheet and to predict the extent and timing of the resulting sea level rise.
NAAMES (North Atlantic Aerosols and Marine Ecosystems Study)
About half the carbon dioxide emitted into Earth’s atmosphere each year ends up in the ocean, and plankton absorb a lot of it. The NAAMES mission studies the world’s largest plankton bloom and how it gives rise to small organic particles that leave the ocean and end up in the atmosphere, ultimately influencing clouds and climate. This mission will be taking measurements from both ship and aircraft in the North Atlantic.
KORUS-AQ (Korea U.S.-Air Quality)
Air quality is a significant environmental concern around the world. Scientists are developing new ways to untangle the different factors that contribute to poor air quality. KORUS-AQ is a joint field study between NASA and the Republic of Korea to advance the ability to monitor air pollution from space. The campaign will assess air quality across urban, rural and coastal South Korea using observations from aircraft, ground sites, ships and satellites to test air quality models and remote sensing methods. Findings from this study will help develop observing systems using models and data to improve air quality assessments for decision makers.
ABoVE (Arctic Boreal Vulnerability Experiment)
The ABoVE mission covers 2.5 million square miles of tundra, forests, permafrost and lakes in Alaska and Northwestern Canada. Scientists from the mission are using satellites and aircraft to study this formidable terrain as it changes in a warming climate. Teams of researchers will also go out into the field to gather additional data. The mission will investigate questions about the role of climate in wildfires, thawing permafrost, wildlife migration habits, insect outbreaks and more.
ATom (Atmospheric Tomography)
The ATom mission takes flight through Earth’s atmosphere to understand how short-lived greenhouse gases like ozone and methane contribute to climate change. In late July through August 2016, a suite of instruments aboard our DC-8 flying laboratory will be hopping down the Pacific Ocean from Alaska to the southern tip of South America. It will then travel north up the Atlantic to Greenland to measure more than 200 gases and particles in the air and their interactions all around the world.
ORACLES (Observations of Clouds above Aerosols and their Interactions)
Southern Africa produces almost a third of the world’s vegetative burning, which sends smoke particles up into the atmosphere, where they eventually mix with stratocumulus clouds over the southeastern Atlantic Ocean. Little is known about how these particles impact the clouds, which play a key role in both regional and global surface temperatures and precipitation. The ORACLES mission is a five-year ground and air campaign aimed at better understanding their interactions and improve on current climate models.
ACT-America (Atmospheric Carbon and Transport – America)
The ACT-America mission will conduct five airborne campaigns across three regions in the eastern United States to study the transport of atmospheric carbon. This region serves as an ideal study area for its productive biosphere, agricultural activity, gas and oil extraction and consumption, dynamic seasonally varying weather patterns and the most extensive carbon cycle and meteorological observing networks on Earth. Using space borne, airborne and ground-based measurements, this mission will enable more accurate and precise estimates for climate management and prediction by studying sources and sinks of greenhouse gases, which act as a thermal blanket for Earth.
Remember to follow the Earth Expeditions on Facebook, Twitter and their Blog.
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Ever wonder what it’s like to be a NASA astronaut? On Thursday, Oct. 29, NASA Astronaut Peggy Whitson will answer your questions! She’ll explain how it takes the NASA Village to help train for her mission to space, what the challenges of living in space are and what it’s like to be a NASA astronaut.
Fun facts about NASA Astronaut Peggy Whitson:
Astronaut Whitson was selected as an Astronaut Candidate in April 1996, and started training in August of the same year.
After completing two years of training and evaluation, she served as the lead for the Crew Test Support Team in Russia from 1998 to 1999.
Astronaut Whitson completed two six-month tours of duty aboard the International Space Station.
She has accumulated 377 days in space between two missions, which is the most for any woman.
Astronaut Whitson has performed a total of six career spacewalks, adding up to 39 hours and 46 minutes! She is also one of only a handful of people to perform spacewalks in both Russian and US spacesuits.
She is scheduled to launch in late 2016 as part of the Expedition 50/51.
Firsts:
Science Officer of the International Space Station
Female Commander for the International Space Station
Female to serve as Chief of the Astronaut Office
Follow her on social media to see how it takes a NASA Village to train her for her upcoming mission: Tumblr, Facebook and Twitter.
Rolling, rolling, rolling.
(via GIPHY)
Ion thrusters are being designed for a wide variety of missions – from keeping communications satellites in the proper position to propelling spacecraft throughout our solar system. But, what exactly is ion propulsion and how does an ion thruster work? Great question! Let’s take a look:
Regular rocket engines: You take a gas and you heat it up, or put it under pressure, and you push it out of the rocket nozzle, and the action of the gas going out of the nozzle causes a reaction that pushes the spacecraft in the other direction.
Ion engines: Instead of heating the gas up or putting it under pressure, we give the gas xenon a little electric charge, then they’re called ions, and we use a big voltage to accelerate the xenon ions through this metal grid and we shoot them out of the engine at up to 90,000 miles per hour.
Something interesting about ion engines is that it pushes on the spacecraft as hard as a single piece of paper pushes on your hand while holding it. In the zero gravity, frictionless, environment of space, gradually the effect of this thrust builds up. Our Dawn spacecraft uses ion engines, and is the first spacecraft to orbit two objects in the asteroid belt between Mars and Jupiter.
To give you a better idea, at full throttle, it would take our Dawn spacecraft four days to accelerate from zero to sixty miles per hour. That may sounds VERY slow, but instead of thrusting for four days, if we thrust for a week or a year as Dawn already has for almost five years, you can build up fantastically high velocity.
Why use ion engines? This type of propulsion give us the maneuverability to go into orbit and after we’ve been there for awhile, we can leave orbit and go on to another destination and do the same thing.
As the commercial applications for electric propulsion grow because of its ability to extend the operational life of satellites and to reduce launch and operation costs, we are involved in work on two different ion thrusters of the future: the NASA Evolutionary Xenon Thruster (NEXT) and the Annular Engine. These new engines will help reduce mission cost and trip time, while also traveling at higher power levels.
Learn more about ion propulsion HERE.
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Venus is an EXTREME world, and we’re calling on YOU to help us explore it! NASA Jet Propulsion Laboratory is running a public challenge to develop an obstacle avoidance sensor for a possible future Venus rover.
With a surface temperature in excess of 840 degrees Fahrenheit and a surface pressure 92 times that of Earth, Venus can turn lead into a puddle and crush a nuclear-powered submarine with ease. While many missions have visited our sister planet, only about a dozen have made contact with the surface of Venus before succumbing to the oppressive heat and pressure after just about more than an hour.
The “Exploring Hell: Avoiding Obstacles on a Clockwork Rover” challenge is seeking the public’s designs for a sensor that could be incorporated into the design concept. The winning sensor could be the primary mechanism by which the rover detects and navigates around obstructions.
Open Date: February 18, 2020 ––––––––– Close Date: May 29, 2020
Observers all over the world are hoping to catch a glimpse of Comet NEOWISE before it speeds away into the depths of space, not to be seen again for another 6,800 years.
For those that are, or will be, tracking Comet NEOWISE there will be a few particularly interesting observing opportunities this week.
Over the coming days it will become increasingly visible shortly after sunset in the northwest sky.
The object is best viewed using binoculars or a small telescope, but if conditions are optimal, you may be able to see it with the naked eye. If you’re looking in the sky without the help of observation tools, Comet NEOWISE will likely look like a fuzzy star with a bit of a tail. Using binoculars will give viewers a good look at the fuzzy comet and its long, streaky tail.
Here’s what to do:
Find a spot away from city lights with an unobstructed view of the sky
Just after sunset, look below the Big Dipper in the northwest sky
Each night, the comet will continue rising increasingly higher above the northwestern horizon.
There will be a special bonus for viewers observing comet NEOWISE from the northeast United States near Washington, DC. For several evenings, there will be a brief conjunction as the International Space Station will appear to fly near the comet in the northeast sky. Approximate times and locations of the conjunctions are listed below (the exact time of the conjunction and viewing direction will vary slightly based on where you are in the Washington, DC area):
July 17 : ~10:56 p.m. EDT = NEOWISE elevation: ~08° Space Station elevation: ~14°
July 18 : ~10:08 p.m. EDT = NEOWISE elevation: ~13° Space Station elevation: ~18°
July 19 : ~10:57 p.m. EDT = NEOWISE elevation: ~10° Space Station elevation: ~08°
July 20 : ~10:09 p.m. EDT = NEOWISE elevation: ~17° Space Station elevation: ~07°
It will be a late waning Moon, with the New Moon on July 20, so the viewing conditions should be good as long as the weather cooperates.
Comet NEOWISE is about 3 miles across and covered in soot left over from its formation near the birth of our solar system 4.6 billion years ago - a typical comet.
Comets are frozen leftovers from the formation of the solar system composed of dust, rock and ices. They range from a few miles to tens of miles wide, but as they orbit closer to the sun, they heat up and spew gases and dust into a glowing head that can be larger than a planet. This material forms a tail that stretches millions of miles.
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On Dec. 24, 1963, the Jet Propulsion Laboratory's Deep Space Information Facility was renamed the Deep Space Network. And, it’s been humanity's ear to the skies ever since.
+ History of the Deep Space Network
The best time to view the Ursids, radiating from Ursa Minor, or the little Dipper, will be from midnight on December 21 until about 1a.m. on December 22, before the moon rises.
Our Cassini spacecraft has completed several orbits that take it just outside Saturn’s famous rings. The first ring-grazing orbit began on November 30. The spacecraft will repeat this feat 20 times, with only about a week between each ring-plane crossing.
+ Learn more
Next year North America will see one of the most rare and spectacular of all sky events. Learn how to prepare.
+ 2017 Solar Eclipse Toolkit
Our first mission to return an asteroid sample to Earth will be multitasking during its two-year outbound cruise to the asteroid Bennu. On February 9-20, OSIRIS-REx (Origins, Spectral Interpretation, Resource Identification, and Security-Regolith Explorer) will activate its onboard camera suite and begin its search for elusive “Trojan,” asteroids, constant companions to planets in our solar system as they orbit the sun, remaining near a stable point 60 degrees in front of or behind the planet. Because they constantly lead or follow in the same orbit, they will never collide with their companion planet.
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Explore the universe and discover our home planet with the official NASA Tumblr account
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