The Transiting Exoplanet Survey Satellite (TESS) is the next step in the search for planets outside of our solar system, including those that could support life. The mission will find exoplanets that periodically block part of the light from their host stars, events called transits.
TESS will survey 200,000 of the brightest stars near the sun to search for transiting exoplanets. The mission is scheduled to launch in 2018.
The TESS launch date is NLT June 2018 (the current working launch date is April 2018).
Music: "Prototype" and "Trial" both from Killer Tracks. Credit: NASA’s Goddard Space Flight Center
NASA Goddard Space Flight Center
Skywatchers in the western hemisphere will see a rare sight on Monday: over the course of several hours, the silhouette of the planet Mercury will appear to cross the face of the Sun. The “transit” of Mercury results from the precise alignment of the orbits of Mercury and Earth that only happens either 13 or 14 times per century; usually the orbital alignment is weak, and as seen from our planet Mercury “misses” the Sun’s disk as it orbits once every 88 days. But on Monday, the view through a properly-shielded telescope will reveal the innermost planet as a dark, perfectly circular spot that moves completely across the Sun in exactly seven and a half hours.
Because of the specifics of our respective orbits, Mercury transits only happen in either the months of May or November, with average dates of 8th May and 10th November. May transits happen less frequently than November transits because during May, Mercury is closer to its largest distance from the Sun, while in November the opposite is true. As a result, the range of possible angles between the Sun and Mercury, as seen from Earth, is smaller in November than May. While the interval between successive November transits can be either 7, 13 or 33 years, May transits are less common, with successive appearances in either 13- or 33-year intervals.
Observations of Mercury transits reach back to at least the seventeenth century. Observations from earlier than this are unlikely because the apparent size of Mercury’s silhouette against the Sun is too small for the unaided eye to resolve. This is why the first recorded Mercury transit — by the French astronomer Pierre Gassendi on 7 November 1631 — dates to after Galileo Galilei’s invention of the telescope in about 1609. Johannes Kepler earlier understood that Mercury’s orbit should periodically take it in front of the Sun, but he died in 1630 before being able to observe a predicted transit.
While these events once had great scientific interest, they are now mainly curiosities that delight astronomy aficionados. Rarer still are transits of Venus across the Sun, the last of which took place in 2012. These events come in pairs separated by 113 years, meaning that most people alive now will not be around to see the next one in December 2117.
Who can see Monday’s event? That depends on the hour of day and which side of the Earth faces the Sun at the time. The map below indicates which parts of the world see either all, some, or none of the transit:
You’ll need at least a good pair of binoculars or a telescope — properly shielded with a heavy filer to prevent eye damage — to even sense Mercury during the transit. It will look like a small, perfectly round and completely opaque black dot against the bright solar photosphere. Mercury is distinguishable in this sense from sunspots, which are irregular in shape, can be partially transparent, and of much larger sizes. This image compares Mercury during a transit (bottom-center) with a sunspot near the solar limb (upper right).
NOTE: DO NOT LOOK AT THE SUN THROUGH A TELESCOPE WITHOUT A FULL-APERTURE SOLAR FILTER! Doing so can cause permanent blindness! Instead, try projecting the image of the sun from a telescope or binoculars onto white paper. This method avoids bringing dangerous, strongly-focused sunlight anywhere near one’s eyes.
Better still: Watch the transit live online! Find live streaming coverage from Slooh, NASA TV, Celestron telescopes, Sky and Telescope magazine, and the Virtual Telescope.
(Top image credit: Sky & Telescope magazine; map and transit image: Fred Espenak)
Engineers at NASA's Langley Research Center in Hampton, Virginia, used lasers inside the 14- by 22-Foot Subsonic Tunnel to map how air flows over a Boeing Blended Wing Body (BWB) model – a greener, quieter airplane design under development. The name for the technique is called particle image velocimetry. If you look closely you can see the light bouncing off tracer particles. Cameras record the movement of those particles as the laser light pulses across the model. This allows researchers to accurately measure the flow over the model once the images are processed. A smoother flow over the wing means less fuel will be needed to power the aircraft.
Image credit: NASA/David C. Bowman
From enabling astronauts to practice moon landings to aircraft crash testing to drop tests for Orion, NASA's gantry has come full circle.
The gantry, a 240-foot high, 400-foot-long, 265-foot-wide A-frame steel structure located at Langley Research Center in Hampton, Va., was built in 1963 and was used to model lunar gravity. Originally named the Lunar Landing Research Facility (LLRF), the gantry became operational in 1965 and allowed astronauts like Neil Armstrong and Edwin "Buzz" Aldrin to train for Apollo 11's final 150 feet before landing on the moon.
Because the moon's gravity is only 1/6 as strong as Earth's, the gantry had a suspension system that supported 5/6 of the total weight of the Lunar Excursion Module Simulator (LEMS), the device the astronauts used to perform the tests. This supportive suspension system imitated the moon's gravitational environment. Additionally, many of the tests were conducted at night to recreate lighting conditions on the moon.
Neil Armstrong with the LEMS at the Lunar Landing Research Facility. This picture (below) was taken in February 1969 - just five months before Armstrong would become the first person to set foot on the surface of the moon.
Aircraft Crash Test Research
After the Apollo program concluded, a new purpose emerged for the gantry – aircraft crash testing. In 1972, the gantry was converted into the Impact Dynamics Research Facility (IDRF) and was used to investigate the crashworthiness of General Aviation (GA) aircraft and rotorcraft. The facility performed full-scale crash tests of GA aircraft and helicopters, system qualification tests of Army helicopters, vertical drop tests of Boeing 707 and composite fuselage sections and drop tests of the F-111 crew escape capsule.
The gantry was even used to complete a number of component tests in support of the Mars Sample Return Earth Entry Vehicle.
With features including a bridge and a 72-foot vertical drop tower, the gantry was able to support planes that weighed up to 30,000 pounds. Engineers lifted aircraft as high as 200 feet in the air and released them to determine how well the craft endured the crash. Data from the crash tests were used to define a typical acceleration for survivable crashes as well as to establish impact criteria for aircraft seats. The impact criteria are still used today as the Federal Aviation Administration standard for certification.
In 1985, the structure was named a National Historic Landmark based on its considerable contributions to the Apollo program.
Revitalized Space Mission
The gantry provides engineers and astronauts a means to prepare for Orion's return to Earth from such missions. With its new mission, the gantry also received a new name – the Landing and Impact Research (LandIR) Facility.
Although originally capable of supporting only 30,000 pounds, the new bridge can bear up to 64,000 pounds after the summer 2007 renovations. Other renovations include a new elevator, floor repairs and a parallel winch capability that allows an accurate adjustment of the pitch of the test article. The new parallel winch system increases the ability to accurately control impact pitch and pitching rotational rate. The gantry can also perform pendulum swings from as high as 200 feet with resultant velocities of over 70 miles per hour.
The gantry makes researching for the optimal landing alternative for NASA's first attempted, manned dry landing on Earth possible. Orion's return on land rather than water will facilitate reuse of the capsule. A water landing would make reuse difficult due to the corrosiveness of salt water.
The testing process involves lifting the test article by steel cables to a height between 40 and 60 feet and swinging it back to Earth. Although the airbags appear most promising, the gantry has the capability to perform different kinds of tests, including a retro rocket landing system and a scale-model, water landing test using a four-foot-deep circular pool. So far, three types of tests have been conducted in support of the Orion program, each progressing from the previous to more realistic features.
The first test consisted of dropping a boilerplate test article that was half the diameter of what Orion will be. For the second round of testing, engineers added a welded structure to the top, with a shape more comparable to Orion to examine the article's tendency to flip or remain upright.
Hydro-Impact
The on-going tests for Orion continue with impacts on water. This is to ensure astronaut safety during a return to Earth mission. Similar to the Apollo program, Orion will re-enter Earth’s atmosphere at very high speeds and after slowing down, deploy parachutes to further slow the descent into the ocean. At NASA Langley Research Center, engineers use the hydro-impact research to determine the stresses on the vehicle and examine its behavior during a mock splashdown.
NASA centers across the country, including the Langley Research Center in Hampton, Virginia, are opening their doors Monday, Feb. 12, to media and social media for 'State of NASA' events.
Activities include a speech from acting NASA Administrator Robert Lightfoot, and unique opportunities for a behind-the-scenes look at the agency's work. These events follow President Trump's Fiscal Year 2019 budget proposal delivery to the U.S. Congress.
Events at NASA centers will include media tours and presentations on the agency's exploration goals for the Moon, Mars and worlds beyond, the innovative technologies developed and under development, as well as the scientific discoveries made as NASA explores and studies Earth and our universe, and advancements toward next-generation air travel.
Lightfoot will provide a 'State of NASA' address to the agency's workforce at 1 p.m. EST from Marshall Space Flight Center in Huntsville, Alabama. His remarks will air live on NASA Television and the agency's website, https://www.nasa.gov/live. Following the presentation, NASA centers will host tours of their facilities for media and social media guests.
At Langley, the news and social media event will run from 1 to 5 p.m. and include:
A look at the SAGE III flight control center. SAGE III is the Stratospheric Aerosol and Gas Experiment III studying Earth's atmosphere from the International Space Station.
A visit to the research aircraft hangar to see aircraft that are used in support of airborne research campaigns, as well as an inflatable heat shield that will enable landing on distant worlds.
A view of the labs where sonic-boom testing is being done to lower their impact so that commercial aircraft can be developed to fly supersonically over land.
A tour in a lab where inflatable space structures are being developed.
Follow the hashtag #StateOfNASA for more!
For the first time, Kepler measured the “shock breakout” of a star, the early flash from the shockwave of a dying red supergiant. The flash comes from a type II supernova, KSN 2011d. Read more
This video is a compilation of ultra-high definition time-lapses of the aurora shot from the space station. Auroras are a space weather phenomenon that occur when electrically-charged electrons and protons collide with neutral atoms in the upper atmosphere. The dancing lights of the aurora provide a spectacular show for those on the ground, but also capture the imaginations of scientists who study the aurora and the complex processes that create them.
One brother is a facts-and-figures guy, the other an adventurer.
They're both deeply fascinated by all things space.
Mikey and Robbie Rouse, 15 and 16, are from Salem, Virginia, and both have Duchenne Muscular Dystrophy, a progressive condition that affects nearly all their voluntary muscles.
On a recent trip to Hampton, Virginia, they visited one of the birthplaces of the American space program — NASA's Langley Research Center.
Mikey, the adventurer, wants to be the first wheelchair astronaut. "And I want to go to Mars," he said during his visit.
Robbie, the facts-and-figures guy, is always thinking of safety first — a quality held sacred by all at NASA.
The brothers' visit to Langley included a tour of the center's hangar, a stop at the Flight Mission Support Center for the ozone-monitoring Stratospheric Aerosol and Gas Experiment III, and presentations on the Hypersonic Inflatable Aerodynamic Decelerator, autonomous technologies, and tests at the Landing and Impact Research Facility.
Deputy Center Director Clayton Turner and Associate Director Cathy Mangum presented Mikey and Robbie with commemorative coins and copies of "A Century at Langley," a pictoral history of the center.
No subject raised during the visit failed to spark the boys' curiosity.
Steve Velotas, associate director for intelligent flight systems, talked with Mikey and Robbie about the ways in which Langley researchers are studying autonmous technologies. Autonomous systems could be used in unmanned aerial vehicles, in-space assembly robots, or even wheelchairs to help those with disabilities navigate more easily.
"I don't trust robots completely," Mikey said.
"We don't either," said Velotas, who then explained that part of the reason Langley scientists are studying autonomous systems is to make sure they work like people want them to.
Evan Horowitz, structures and mechanical systems airworthiness engineer, showed the brothers Langley's historic hangar and talked about some of the past and present missions the facility has supported.
Gemini and Apollo astronauts trained in the hangar's Rendezvous Docking Simulator, and aircraft used for airborne science studies and autonomous flight research are based there.
Mikey and Robbie peppered Horowitz, who often takes tour groups through the hangar, with questions about air pollution and habitable exoplanets.
"This is great," said Horowitz. "Best interaction I've had in months."
The previous day, Mikey and Robbie visited the Virginia Air & Space Center, Langley's official visitors center.
The brothers live with their great-grandmother in Salem and receive daily assistance from a nonprofit called Lutheran Family Services of Virginia. The trip to Hampton was organized by Julie's Abundance Project, a program of Lutheran Family Services of Virginia.
Image Credits: NASA/David C. Bowman
Joe AtkinsonJoe Atkinson NASA Langley Research Center
NASA Astronomy Picture of the Day 2016 April 6
Jupiter has auroras. Like near the Earth, the magnetic field of our Solar System’s largest planet compresses when impacted by a gust of charged particles from the Sun. This magnetic compression funnels charged particles towards Jupiter’s poles and down into the atmosphere. There, electrons are temporarily excited or knocked away from atmospheric gases, after which, when de-exciting or recombining with atmospheric ions, auroral light is emitted. The featured illustration portrays the magnificent magnetosphere around Jupiter in action. In the inset image released last month, the Earth-orbiting Chandra X-ray Observatory shows unexpectedly powerful X-ray light emitted by Jovian auroras, depicted in false-colored purple. That Chandra inset is superposed over an optical image taken at a different time by the Hubble Space Telescope. This aurora on Jupiter was seen in October 2011, several days after the Sun emitted a powerful Coronal Mass Ejection (CME).
NASA also uses symbols for specific projects within the agency. Each space shuttle crew designs a patch that represents what it will do during the mission. Some robotic probes sent to explore space have had mission patches. From the wing of the space shuttle to the top of the NASA homepage, the agency's official insignia is probably its best-known symbol.
The round red, white and blue insignia, nicknamed the "meatball," was designed by employee James Modarelli in 1959, NASA's second year. The design incorporates references to different aspects of the mission of the National Aeronautics and Space Administration. The round shape of the insignia represents a planet. The stars represent space. The red v-shaped vector represents aeronautics. The circular orbit around the agency's name represents space travel.
After it was introduced, the "meatball" was the most common symbol of NASA for 16 years, but in 1975 NASA decided to create a more "modern" logo. That logo, which consisted of the word "NASA" in a unique type style, was nicknamed the "worm." That logo was retired in 1992, and the classic meatball insignia has been the most common agency symbol since.
In addition to the insignia, NASA has another official symbol. If the meatball is the everyday face of NASA, the NASA seal is the dressed-up version. The NASA administrator uses the seal for formal purposes such as award presentations and ceremonies. Like the meatball insignia, the seal also includes planet, stars, orbit and vector elements
NASA also uses symbols for specific projects within the agency. Each space shuttle crew designed a patch that represents what they were going to do during the mission. Some robotic probes sent to explore space have had mission patches.
Image Credits: NASA
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