It’s a reasonable assumption that most Universe Today website visitors are, at the very least, intrigued by the night sky. This Universe Today reader, someone who always enjoys learning something new, was surprised to discover yet another cultural association with the wonders of the world around us. Vexillology is the scientific study of flags and apparently has a connection with Astronomy. If you’re looking for a highly informational book mashing up Astronomy and Vexillogy, Flags of the Night Sky, When Astronomy Meets National Pride, by Andre G. Bordeleau is a great resource.
In the United States of America we’re familiar with our country’s flag. We may also know our state’s flag. But, do we know what the colors and patterns stand for? Think about the gathering of the world at the Olympics. There’s something magical about the opening ceremonies of the Games. Talented athletes with a lifetime of hard work and dedication to their sport proudly march behind the honored flag bearer of their nation. As the flags and their teams walk through the arena, the world tunes in to watch centuries of national pride. All of these flags are not pure decoration, they have profound thought and meaning behind them. Flags of the world are displayed on an international Olympic stage; many portraying interesting connections to the night sky.
Bordeleau begins his book with a look at an internationally recognized flag – Brazil’s. Although its history dates back to 1889, its most recent incarnation is the most well known. According to Bordeleau, “The current flag of Brazil is akin to a star atlas featuring 9 different constellations and 27 stars.” The stars are not purely decorative; they correlate to specific states and to the capital. The Astronomy connection is fantastic.
With chapters ranging from sun-bearing flags, moon-bearing flags, and one titled “Starry Flags: Here’s Stars in Your Eyes”, Flags of the Night Sky covers it all. If you’re looking for in depth insight into national cultures displayed through their flags and their connections tied to the heavens above, this is a well organized, great resource.
Flags of the Night Sky is available for purchase or download at Amazon.com
Universe Today and Springer are pleased to be able to offer three free copies of Flags of the Night Sky to our readers. In order to be entered into the giveaway drawing, just put your email address into the box at the bottom of this post (where it says “Enter the Giveaway”) before Monday, March 10. If this is the first time you’re registering for a giveaway, you’ll receive a confirmation email immediately where you’ll need to click a link to be entered into the drawing. For those who have registered previously, you’ll receive an email later where you can enter this drawing.
How heavy is a kilogram, how long is a second? How warm is a degree? We measure our Universe is so many different ways, using different units of measurement. But how do scientists come up with measurement tools which are purely objective? Continue reading “Astronomy Cast Ep. 336: Units of Measure”
This Image of M82 including a supernova at near-infrared wavelengths J, H, and K (1.2, 1.65, and 2.2 microns), made Feb. 20 by the FLITECAM instrument on SOFIA. (NASA/SOFIA/FLITECAM team/S. Shenoy)
Astronomers wanting a closer look at the recent Type Ia supernova that erupted in M82 back in January are in luck. Thanks to NASA’s Stratospheric Observatory for Infrared Astronomy (SOFIA) near-infrared observations have been made from 43,000 feet — 29,000 feet higher than some of the world’s loftiest ground-based telescopes.
(And, technically, that is closer to M82. If only just a little.)
All sarcasm aside, there really is a benefit from that extra 29,000 feet. Earth’s atmosphere absorbs a lot of wavelengths of the electromagnetic spectrum, especially in the infrared and sub-millimeter ranges. So in order to best see what’s going on in the Universe in these very active wavelengths, observational instruments have to be placed in very high, dry (and thus also very remote) locations, sent entirely out into space, or, in the case of SOFIA, mounted inside a modified 747 where they can simply be flown above 99% of the atmosphere’s absorptive water vapor.
NASA’s airborne SOFIA observatory (SOFIA/USRA)
During a recent 10-hour flight over the Pacific, researchers aboard SOFIA turned their attention to SN2014J, one of the closest Type Ia “standard candle” supernovas that have ever been seen. It appeared suddenly in the relatively nearby Cigar Galaxy (M82) in mid-January and has since been an exciting target of observation for scientists and amateur skywatchers alike.
In addition to getting a bird’s-eye-view of a supernova, they used the opportunity to calibrate and test the FLITECAM (First Light Infrared Test Experiment CAMera) instrument, a near infrared camera with spectrographic capabilities mounted onto SOFIA’s 2.5-meter German-built main telescope.
What they’ve found are the light signatures of heavy metals being ejected by the exploding star. (Rock on, SN2014J.)
“When a Type Ia supernova explodes, the densest, hottest region within the core produces nickel 56,” said Howie Marion from the University of Texas at Austin, a co-investigator aboard the flight. “The radioactive decay of nickel-56 through cobalt-56 to iron-56 produces the light we are observing tonight. At this life phase of the supernova, about one month after we first saw the explosion, the H- and K-band spectra are dominated by lines of ionized cobalt. We plan to study the spectral features produced by these lines over a period of time and see how they change relative to each other. That will help us define the mass of the radioactive core of the supernova.”
Three images of M82 and the supernova SN2014J, including one from the FLITECAM instrument on SOFIA (right). Credit: NASA/SOFIA/FLITECAM team/S. Shenoy
Further observations from SOFIA will help researchers learn more about the evolution of Type Ia supernovas, which in addition to being part of the life cycles of certain binary-pair stars are also valuable tools used by astronomers to determine distances to far-off galaxies.
Researchers work at the FLITECAM instrument station on board SOFIA on Feb. 20 (NASA/SOFIA/N. Veronico)
“To be able to observe the supernova without having to make assumptions about the absorption of the Earth’s atmosphere is great,” said Ian McLean, professor at UCLA and developer of FLITECAM. “You could make these observations from space as well, if there was a suitable infrared spectrograph to make those measurements, but right now there isn’t one. So this observation is something SOFIA can do that is absolutely unique and extremely valuable to the astronomical community.”
UPDATE 4 March 2014: The FY 2015 budget request proposed by the White House will effectively shelf the SOFIA mission, redirecting its funding toward planetary missions like Cassini and an upcoming Europa mission. Unfortunately, SOFIA’s flying days are now numbered, unless German partner DLR increases its contribution. Read more here.
Apollo 9's lunar module, "Spider", during a test in 1969. Credit: NASA
Hard to believe the decades fly by so fast. It was 45 years ago today that the crew of Apollo 9 took off from the Kennedy Space Center en route to a big test of the lunar module. Being March 1969, history shows that it was only about four months later when men touched the moon for the first time ever.
Getting to the moon, however, required making sure that the lunar landing craft was in tip-top shape. This was the first test of the lunar module in space. Apollo 9 astronauts Jim McDivitt, Rusty Schweickart and Dave Scott spent several days shaking out the spacecraft in the relative safety of Earth orbit.
The mission is perhaps best remembered for the first docking of “Spider” (the lunar module) and “Gumdrop” (the command module), but plenty happened during their March 3-13, 1969 mission. You can relive some of the most memorable moments of training and the mission in the gallery below. More information on the mission is available at NASA.
Apollo 9 astronauts Jim McDivitt (front) and Rusty Schweickart inside the lunar module mission simulator at the Kennedy Space Center. Apollo 9 flew in March 1969. Credit: NASASpotlights shine on the Saturn V rocket carrying Apollo 9 prior to its launch from the Kennedy Space Center on March 3, 1969. Credit: NASAThe Apollo 9 astronauts walk out to the vehicle that will take them out to the launch pad, hours before launch on March 3, 1969. From left: Jim McDivitt (commander), Dave Scott (command module pilot) and Rusty Schweickart (lunar module pilot). Credit: NASAThe launch of Apollo 9 on March 3, 1969. Credit: NASAApollo 9’s “Spider” lunar module lies nestled in the third stage of the Saturn V rocket that carried it to space in March 1969. Credit: NASAApollo 9 lunar module pilot Rusty Schweickart during a spacewalk in March 1969. Here, he was standing on the porch of the lunar module “Spider.” Credit: NASAApollo 9 lunar module pilot Rusty Schweickart during a spacewalk in March 1969. Credit: NASAApollo 9 commander Jim McDivitt (right) drinks from a hand water dispenser while lunar module pilot Rusty Schweickart looks on. Photo is a still from a March 1969 television broadcast. Credit: NASAApollo 9 commander Jim McDivitt shows off several days’ beard growth during March 1969. The photo was taken in lunar module “Spider”. Credit: NASAApollo 9’s lunar module “Spider” during a test in March 1969. Credit: NASAApollo 9 astronaut Dave Scott during a spacewalk from the command module in March 1969. The Mississippi River is visible in the background. Credit: NASAA recovery helicopter picks up Apollo 9 command module “Gumdrop” and brings it to recovery ship USS Guadalcanal on March 13, 1969. Click for larger version. Credit: NASA / Elizabeth Howell (photo combination)The Apollo 9 astronauts await recovery from a helicopter from USS Guadalcanal on March 13, 1969. The crew included Jim McDivitt (in hatch), Rusty Schweickart (far right, in foreground) and Dave Scott (behind Schweickart). The other people are frogmen from the recovery team. Credit: NASAThe Apollo 9 aboard the recovery ship USS Guadalcanal on March 13, 1969. From left: Rusty Schweickart (lunar module pilot), Dave Scott (command module pilot) and Jim McDivitt (commander). Credit: NASA
Neil Armstrong in the LM after his historic moonwalk (NASA)
Neil Armstrong — the first man on the moon, who died in 2012 — will now be the namesake of one of NASA’s research centers. A new law designated the Armstrong Flight Research Center took effect March 1, replacing the old name since 1976, the Dryden Flight Research Center.
Former NASA deputy administrator Hugh L. Dryden will still see his name in the area, however, as the center’s 12,000-square-mile (31,000-square-kilometer) Western Aeronautical Test Range is now called Dryden Aeronautical Test Range.
“I cannot think of a more appropriate way to honor these two leaders who broadened our understanding of aeronautics and space exploration,” stated NASA administrator Charles Bolden.
“Both Dryden and Armstrong are pioneers whose contributions to NASA and our nation still resonate today. Armstrong was the first person to walk on the moon. Dryden’s expertise at the National Advisory Committee for Aeronautics and then at NASA established America’s leadership in aerospace, and his vision paved the way for Armstrong to take those first steps.”
NASA astronaut Neil Armstrong earlier in his career, when he flew X-15s at the NACA High-Speed Flight Station (now called the NASA Armstrong Flight Research Center). Credit: NASA
At the center, Armstrong is probably best remembered for his flights in the X-15, a rocket-powered aircraft that set several altitude and speed records in the 1960s. At what was then the NACA High-Speed Flight Station, he flew seven times in that particular experimental aircraft, along with 41 other kinds of aircraft, between 1955 and 1962. Armstrong was also involved with development of a predecessor to a lunar landing training vehicle used in the Apollo missions (which almost killed Armstrong in a practice run for Apollo 11).
Neil Armstrong at the Kennedy Space Center (KSC) Saturn V Exhibit (Control Room) for the 30th Anniversary of Apollo 11 on July 16, 1999. Credit: John Salsbury
Armstrong’s connection with the research center continued after he left the astronaut corps, when he was NASA’s deputy associate administrator for aeronautics. In this capacity, NASA wrote, he was “overseeing aeronautical research programs being conducted at the center, particularly its pioneering work on developing digital electronic flight control systems.”
The center is located on California’s Edwards Air Force Base. Renaming was directed in legislation authored by Rep. Kevin McCarthy (R) of California’s 22nd district (and also the house majority whip), NASA stated. After the bill passed the U.S. House of Representatives in 2013 and the Senate in January, President Barack Obama signed the name into law Jan. 16. A renaming ceremony is expected in the spring.
Armstrong is the second astronaut to have a center named after him. The Lewis Research Center in Cleveland was renamed Glenn Research Center after Sen. John Glenn (D) in 1999. Glenn flew twice in space. In 1962, Glenn became the first American to orbit the Earth. He then returned to space in 1998 at the age of 77, becoming the oldest person to fly in space to date.
The movie ‘Gravity’ ended up being a force to reckon with at the 86th Academy Awards on Sunday, with the space thriller pulling in seven Oscars — including Best Director.
Starring Sandra Bullock and George Clooney, the movie followed the aftermath of an orbital disaster. Despite criticism from some about the movie’s accuracy, the film picked up 10 nominations and numerous good vibes from critics. (The movie has a 97% “Fresh” rating on Rotten Tomatoes). You can see congratulations from NASA astronauts Mike Massimino and Cady Coleman below the jump.
“Like any other human endeavor, a film is a transformative experience, and I want to thank Gravity because for many of us involved in this film, it was definitely a transformative experience,” said director Alfonso Cuarón in his acceptance speech last night (March 2).
“And it’s good because it took so long, if not, it would be a waste of time. It really sucks,” he joked, “because for a lot of people, the transformative experience was wisdom. For me, it was just the colour of my hair.”
Among the people Cuarón paid tribute to was Sandra Bullock, who was nominated for ‘Best Lead Actress’ but lost out to Cate Blanchett, who won for her performance in Blue Jasmine.
Sandra Bullock in a still from the movie ‘Gravity.’ Credit: Regency Enterprises/Warner Bros. Entertainment
“You’re Gravity,’ Cuarón said to Bullock from the stage. “You’re the soul, heart of the film. You’re a most amazing collaborator and one of the best people I’ve ever met.”
The movie attracted 7 wins of its 10 Oscar nominations, failing to earn ‘Best Picture’ (which went to 12 Years A Slave), ‘Achievement in Production Design’ (given to American Hustle). and ‘Best Lead Actress’ Its wins were:
Best director (Alfonso Cuarón);
Achievement in cinematography (Emmanuel Lubezki);
Achievement in film editing (Alfonso Cuarón and Mark Sanger);
Achievement in music written for motion pictures (Original score) (Steven Price);
Achievement in sound editing (Glenn Freemantle);
Achievement in sound mixing (Skip Lievsay, Niv Adiri, Christopher Benstead and Chris Munro);
Achivement in visual effects (Tim Webber, Chris Lawrence, Dave Shirk and Neil Corbould).
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.
Mars rock rows and Mount Sharp. Martian landscape scene with rows of striated rocks in the foreground and Mount Sharp on the horizon. NASA's Curiosity Mars rover paused mid drive at the Junda outcrop to snap the component images for this navcam camera photomosaic on Sol 548 (Feb. 19, 2014) and then continued traveling southwards towards mountain base. UHF Antenna at right. Credit: NASA/JPL-Caltech/Marco Di Lorenzo/Ken Kremer-kenkremer.com
Mars rock rows and Spectacular Mount Sharp
Martian landscape scene with rows of striated rocks in the foreground and spectacular Mount Sharp on the horizon. NASA’s Curiosity Mars rover paused mid drive at the Junda outcrop to snap the component images for this colorized navcam camera photomosaic on Sol 548 (Feb. 19, 2014) and then continued traveling southwards towards mountain base. UHF Antenna at right.
Credit: NASA/JPL-Caltech/Marco Di Lorenzo/Ken Kremer-kenkremer.com
See stereo 3-D and look back views below[/caption]
Like any good tourist, NASA’s rover Curiosity apparently couldn’t resist the photobug urge from a gorgeous Martian mountain scene she happened by recently and decided to pull over and enjoy the view.
So she stopped the dune buggy mid-drive on the sandy road to her daily destination one Sol last week on Feb. 19, powered up the camera suite and excitedly snapped a spectacular landscape view of a striated rock field dramatically back dropped by towering Mount Sharp on the horizon.
See our Mars rocks and Mount Sharp photomosaic above and a 3-D stereoscopic view from NASA below.
The sedimentary foothills of Mount Sharp, which reaches 3.4 miles (5.5 km) into the Martian sky, is the 1 ton robots ultimate destination inside Gale Crater because it holds caches of water altered minerals.
Martian Landscape With Rock Rows and Mount Sharp (Stereo) This stereo landscape scene from NASA’s Curiosity Mars rover on Feb. 19, 2014 shows rows of rocks in the foreground and Mount Sharp on the horizon. It appears three dimensional when viewed through red-blue glasses with the red lens on the left. Credit: NASA/JPL-Caltech
And just for good measure, Curiosity also snapped a series of breathtaking look back photos showing her tracks in the dune filled terrain from whence she came since straddling through the Dingo Gap gateway. See our mosaics below.
The panoramic mountain view taken on Sol 548 shows rows of striated rocks all oriented in a similar direction in the foreground with Mount Sharp in the background.
Curiosity looks back across dune field to her wheel tracks and a small crater she just missed. Flattened rear hazcam image, colorized from Sol 555 (Feb 27, 2014). Credit: NASA/JPL-Caltech/Marco Di Lorenzo/Ken Kremer-kenkremer.com
Scientists directed Curiosity to drive by the rock rows nicknamed “Junda” after their interest was piqued by orbital images taken by the powerful telescopic camera on NASA’s Mars Reconnaissance Orbiter (MRO) circling overhead.
The six wheeled rover paused during the planned Feb. 19 drive of 328 feet (100 meters) to capture the imagery.
She then pushed forward to finish the day’s drive and snapped another fabulous look back view – see our mosaic below.
And the next day on Feb. 20 (Sol 549), she also completed her second 100 meter drive in reverse.
Her handlers are occasionally commanding Curiosity to drive backwards in a newly tested bid to minimize serious damage to the six 20 inch diameter wheels in the form of rips and tears caused by rough edged Red Planet rocks – see our wheel mosaic below.
Curiosity looks back at Martian sand dunes and rover tracks after passing by Junda outcrop (right) on Sol 548 (Feb. 19, 2014) with Gale Crater rim and Mount Sharp on the distant horizon. Navcam colorized photomosaic. Credit: NASA/JPL-Caltech/Ken Kremer- kenkremer.com/Marco Di Lorenzo
Curiosity is well on the way to her next near term goal, which is a science waypoint, named Kimberly (formerly called KMS-9), which lies about half a mile ahead.
Kimberly is of interest to the science team because it sits at an the intersection of different rock layers and also features ground with striations like those at “Junda”.
Curiosity looks back eastward to ‘Dingo Gap’ sand dune inside Gale Crater. After crossing over the 3 foot (1 meter) tall dune on Sol 539, Feb. 9, 2014 the rover drove westward into the ‘Moonlight Valley’. The parallel rover wheel tracks are 9 feet (2.7 meters) apart. Assembled from Sol 539 colorized navcam raw images. Credit: NASA/JPL/ Ken Kremer- kenkremer.com/Marco Di Lorenzo
So, after the rover reaches Kimberly, researchers plan to temporarily halt driving for awhile to investigate the location and direct the robot to drill into another rock to collect samples for analysis by the two state- of-the -art chemistry labs.
If drilling is warranted, Kimberly would be the site of Curiosity’s first drilling operation since the Cumberland outcrop target was bored into during the spring of 2013 at Yellowknife Bay.
Curiosity departed the Yellowknife Bay region in July 2013 where she discovered a habitable zone and thereby accomplished the primary goal of the mission.
To date Curiosity’s odometer stands at 5.3 kilometers and she has taken over 125,000 images.
The robot has somewhat less than another 5 km to go to reach the base of Mount Sharp.
She perhaps may arrive sometime in mid 2014.
Arrival time at Mount Sharp depends on driving speed and whether the upcoming terrain is smoother or strewn with sharp edged rocks that have hindered progress due to accumulating wear and tear on the aluminum wheels.
Up close photomosaic view shows lengthy tear in rover Curiosity’s left front wheel caused by recent driving over sharp edged Martian rocks on the months long trek to Mount Sharp. Raw images taken by the MAHLI camera on Curiosity’s arm on Jan. 31, 2014 (Sol 529) were assembled to show some recent damage to several of its six wheels Credit: NASA / JPL / MSSS / Marco Di Lorenzo / Ken Kremer- kenkremer.com See below complete 6 wheel mosaic and further wheel mosaics for comparison
Stay tuned here for Ken’s continuing Curiosity, Opportunity, Chang’e-3, GPM, SpaceX, Orbital Sciences, LADEE, MAVEN, MOM, Mars and more planetary and human spaceflight news. Learn more at Ken’s upcoming presentations at the NEAF convention on April 12/13.
Curiosity’s View Past Tall Dune at edge of ‘Dingo Gap’
This photomosaic from Curiosity’s Navigation Camera (Navcam) taken at the edge of the entrance to the Dingo Gap shows a 3 foot (1 meter) tall dune and valley terrain beyond to the west, all dramatically back dropped by eroded rim of Gale Crater. View from the rover’s current position on Sol 528 (Jan. 30, 2014). The rover team may decide soon whether Curiosity will bridge the dune gap as a smoother path to next science destination. Credit: NASA/JPL-Caltech/Marco Di Lorenzo/Ken Kremer- kenkremer.com
Infrared image of comet NEOWISE (C/2014 C3). Credit: NASA/JPL-Caltech
NASA’s NEOWISE mission — formerly known as just WISE — has identified the first comet of its new near-Earth object hunting career… and, according to mission scientists, it’s a “weirdo.”
In its former life NASA’s WISE (Wide-field Infrared Survey Explorer) spacecraft scanned the entire sky in infrared wavelengths. It helped discover the galaxy’s coldest stars, the Universe’s brightest galaxies, and some of the darkest asteroids lurking in the main asteroid belt between Mars and Jupiter… as well as closer in to Earth’s neck of the woods.
After exhausting its supply of liquid coolant needed to shield itself from its own radiating heat, in 2011 WISE was put into a state of hibernation. It was awoken last year and rebranded NEOWISE, and set upon the task of locating unknown objects with orbits in the proximity of Earth’s.
Artist’s impression of the WISE satellite
To date several new asteroids have already been found by NEOWISE, and on February 14, 2014, it spotted its first comet.
“We are so pleased to have discovered this frozen visitor from the outermost reaches of our solar system,” said Amy Mainzer, NEOWISE principal investigator at JPL. “This comet is a weirdo — it is in a retrograde orbit, meaning that it orbits the sun in the opposite sense from Earth and the other planets.”
Designated “C/2014 C3 (NEOWISE),” the comet was 143 million miles (230 million km) away in the image above — a composite made from six infrared exposures. That’s 585 times the distance to the Moon, or about the average distance between the Earth and Mars.
The tail of the comet NEOWISE extends about 25,000 miles (40,000 km) to the right in the image.
Overall, C/2014 C3 (NEOWISE) was spotted six times before it moved out of range of the spacecraft’s view. The comet has a highly-eccentric 20-year orbit that takes it high above the plane of the Solar System and out past the orbit of Jupiter. Technically, with a perihelion distance greater than 1.3 AU, comet C/2014 C3 does not classify as a near-Earth object (and its orbit does not intersect Earth’s.) But it’s still good to know that NEOWISE is looking out for us.
