Black holes want to absorb all matter and energy in the Universe. It’s just a matter of time. So what can we do to fight back? What superweapons have been devised to destroy black holes?
Black holes are the natural enemies of all spacefaring races. With their bottomless capacity to consume all light and matter, it’s just a few septillion years before all things in the Universe have found their way into the cavernous maw of a black hole, crushed into the infinitely dense singularity. If Star Trek has taught us anything, it’s that it’s mankind’s imperative to survive against all odds.
So will we take this lying down?
Heck no!
Will we strike first and destroy the black holes before they destroy us?
Heck yes!
A gas stream from galaxy ESO 137-001 shines brightly in X-rays captured by the Chandra X-Ray Observatory. The galaxy is captured in other wavelengths by the Hubble Space Telescope. Credit: NASA, ESA, CXC
Is that a tractor beam trying to latch on to galaxy ESO 137-001? While the bold blue stripe in the picture above looks like a Star Trek-like technology, this new picture combination captures a stream of gas shining brightly in X-rays.
The “galactic disrobing” is taking place as the galaxy moves through the center of a star cluster full of superheated gas, scientists said. You can see another shot of the chaos below the jump.
From Earth’s perspective, the galaxy (which looks a little like a jellyfish) is found in the Triangulum Australe (The Southern Triangle) , and is part of the Norma Cluster that is about 200 million light-years from the Milky Way (our own galaxy). ESO 137-001 is moving through a galaxy cluster called Abell 3627. All of the superheated gas in this region is making ESO 137-001 bleed gas from its own structure as it goes.
“These streaks are actually hot young stars, encased in wispy streams of gas that are being torn away from the galaxy by its surroundings as it moves through space,” stated the Hubble European Space Agency Information Centre. “This violent galactic disrobing is due to a process known as ram pressure stripping — a drag force felt by an object moving through a fluid. The fluid in question here is superheated gas, which lurks at the centres of galaxy clusters.”
“This image also shows other telltale signs of this process, such as the curved appearance of the disc of gas and dust — a result of the forces exerted by the heated gas,” the centre added. “The cluster’s drag may be strong enough to bend ESO 137-001, but in this cosmic tug-of-war the galaxy’s gravitational pull is strong enough to hold on to the majority of its dust — although some brown streaks of dust displaced by the stripping are visible.”
This stripping has been caught in other images, such as these 2007 and 2010 pictures from the Chandra X-Ray Observatory.
A Hubble Space Telescope image of spiral galaxy ESO 137-001 moving through galaxy cluster Abell 3627. The tendrils (visible in ultraviolet light) are gas flowing away from the galaxy as it moves through superheated gas in the area. Credit: NASA, ESA
Artist's impression of a planet orbiting a red dwarf star. Credit: University of Hertfordshire
Good news for planet-hunters: planets around red dwarf stars are more abundant than previously believed, according to new research. A new study — which detected eight new planets around these stars — says that “virtually” all red dwarfs have planets around them. Moreover, super-Earths (planets that are slightly larger than our own) are orbiting in the habitable zone of about 25% of red dwarfs nearby Earth.
“We are clearly probing a highly abundant population of low-mass planets, and can readily expect to find many more in the near future – even around the very closest stars to the Sun,” stated Mikko Tuomi, who is from the University of Hertfordshire’s centre for astrophysics research and lead author of the study.
The find is exciting for astronomers as red dwarf stars make up about 75% of the universe’s stars, the study authors stated.
The researchers looked at data from two planet-hunting surveys: HARPS (High Accuracy Radial Velocity Planet Searcher) and UVES (Ultraviolet and Visual Echelle Spectrograph), which are both at the European Southern Observatory in Chile. The two instruments measure the effect a planet has on its parent star, specifically by examining the gravitational “wobble” the planet’s orbit produces.
An artist’s concept of a rocky world orbiting a red dwarf star. (Credit: NASA/D. Aguilar/Harvard-Smithsonian center for Astrophysics).
Putting the information from both sets of data together, this amplified the planet “signals” and revealed eight planets around red dwarf stars, including three super-Earths in habitable zones. The researchers also applied a probability function to estimate how abundant planets are around this type of star.
The planets are between 15 and 80 light years away from Earth, and add to the 17 other planets found around low-mass dwarfs. Scientists also detected 10 weaker signals that could use more investigation, they said.
This time-lapse color panorama from China’s Chang’e-3 lander shows the Yutu rover at two different positions during its trek over the Moon’s surface at its landing site from Dec. 15-18, 2013. This view was taken from the 360-degree panorama. Credit: CNSA/Chinanews/Ken Kremer/Marco Di Lorenzo. See our complete Yutu timelapse pano at NASA APOD Feb. 3, 2014: http://apod.nasa.gov/apod/ap140203.htm
This time-lapse color panorama from China’s Chang’e-3 lander shows the Yutu rover at two different positions during its trek over the Moon’s surface at its landing site from Dec. 15-18, 2013. This view was taken from the 360-degree panorama.
Credit: CNSA/Chinanews/Ken Kremer/Marco Di Lorenzo.
See our complete 5 position Yutu timelapse pano herein and 3 position pano at NASA APOD Feb. 3, 2014: http://apod.nasa.gov/apod/ap140203.htm
Story updated[/caption]
The serious technical malfunction afflicting the life and continued operations of China’s Yutu moon rover since the start of its second Lunar Night time hibernation in late January 2014 has been identified as an inability to properly maneuver the life giving solar panels, according to a top Chinese space official.
“Yutu suffered a control circuit malfunction in its driving unit,” according to a newly published report on March 1 by the state owned Xinhua news agency.
“The control circuit problem prevented Yutu from entering the second dormancy as planned,” said Ye Peijian, chief scientist of the Chang’e-3 program, in an exclusive interview with Xinhua.
At the time that Yutu’s 2nd Lunar sleep period began on Jan. 25, 2014, Chinese space officials had announced that the robot’s future was in jeopardy after it suffered an unidentified “ mechanical control anomaly” due to the “complicated lunar surface.”
A functioning control circuit is required to lower the rovers mast and protect the delicate components and instruments mounted on the mast from directly suffering from the extremely harsh cold of the Moon’s recurring night time periods.
“Normal dormancy needs Yutu to fold its mast and solar panels,” said Ye.
The high gain communications antenna and the imaging cameras are attached to the mast.
They must be folded down into a warmed electronics box to shield them from the damaging effects of the Moon’s nightfall when temperatures plunge dramatically to below minus 180 Celsius, or minus 292 degrees Fahrenheit.
Chang’e-3/Yutu Timelapse Color Panorama
This newly expanded timelapse composite view shows China’s Yutu moon rover at two positions passing by crater and heading south and away from the Chang’e-3 lunar landing site forever about a week after the Dec. 14, 2013 touchdown at Mare Imbrium. This cropped view was taken from the 360-degree timelapse panorama. See complete 360 degree landing site timelapse panorama herein and APOD Feb. 3, 2014. Chang’e-3 landers extreme ultraviolet (EUV) camera is at right, antenna at left. Credit: CNSA/Chinanews/Ken Kremer/Marco Di Lorenzo – kenkremer.com. See our complete Yutu timelapse pano at NASA APOD Feb. 3, 2014: http://apod.nasa.gov/apod/ap140203.htm
The solar panels also generate power during each Lunar day to keep the robot alive and conduct its mission of scientific exploration roving across the lunar terrain.
The rover and Chang’e-3 stationary lander must power down and sleep during each lunar night since there is no sunlight available to generate power and no communications are possible with Earth.
The panel driving unit also helps maneuver the panels into position to efficiently point to the sun to maximize the electrical output.
“The driving unit malfunction prevented Yutu to do those actions” said Ye.
Each lunar day and night lasts for alternating periods of 14 Earth days.
“This means Yutu had to go through the lunar night in extremely low temperatures.”
Apparently the mast was not retracted and remained vertical during the lunar nights 2 and 3.
And the camera somehow survived the harsh temperature decline and managed to continue operating since it snapped two images of the Chan’ge-3 lander during Lunar Day 3. See our two image mosaic – below.
360-degree time-lapse color panorama from China’s Chang’e-3 lander. This new 360-degree time-lapse color panorama from China’s Chang’e-3 lander shows the Yutu rover at five different positions, including passing by crater and heading south and away from the Chang’e-3 lunar landing site forever during its trek over the Moon’s surface at its landing site from Dec. 15-22, 2013 during the 1st Lunar Day. Credit: CNSA/Chinanews/Ken Kremer/Marco Di Lorenzo – kenkremer.com. See our Yutu timelapse pano at NASA APOD Feb. 3, 2014: http://apod.nasa.gov/apod/ap140203.htm
In addition to being chief scientist of the Chang’e-3 program Ye is also a member of the National Committee of the Chinese People’s Political Consultative Conference, the country’s top political advisory body.
Yutu is China’s first ever Moon rover and successfully accomplished a soft landing on the Moon on Dec. 14, 2013, piggybacked atop the Chang’e-3 mothership lander.
Barely seven hours after touchdown, the six wheeled moon buggy drove down a pair of ramps onto the desolate gray plains of the lunar surface at Mare Imbrium (Sea of Rains) covered by volcanic material.
For a time in mid-February, mission scientists feared that Yutu would no longer function when because no signals were received until two days later than the planned “awakening” from Lunar Night 2 on Feb. 10.
Mosaic of the Chang’e-3 moon lander and the lunar surface taken by the camera on China’s Yutu moon rover from a position south of the lander during Lunar Day 3. Note the landing ramp and rover tracks at left. Credit: CNSA/SASTIND/Xinhua/Marco Di Lorenzo/Ken Kremer
Fortunately, Yutu did finally wake up some 48 hours late on Feb. 12 and function on Lunar Day 3.
And the team engaged in troubleshooting to try and identify and rectify the technical problems.
Since then, Chinese space engineers engaged in troubleshooting to try and identify and rectify the technical problems in a race against time to find a solution before the start of Lunar Night 3.
“Yutu only carried out fixed point observations during its third lunar day.” according to China’s State Administration of Science, Technology and Industry for National Defence (SASTIND), responsible for the mission.
However it did complete some limited scientific observations. And fortunately the ground penetrating radar, panoramic and infrared imaging equipment all functioned normally.
Yutu and the companion Chang’e-3 lander have again gone into sleep mode during Lunar Night 3 on Feb. 22 and Feb 23 respectively, local Beijing time.
But the issue with the control circuit malfunction in its driving unit remains unresolved and still threatens the outlook for Yutu’s future exploration.
See our new Chang’e-3/Yutu lunar panoramas by Ken Kremer and Marco Di Lorenzo herein and at NASA APOD on Feb. 3, 2014.
Chang’e-3 lander and Yutu rover – from Above And Below Composite view shows China’s Chang’e-3 lander and Yutu rover from Above And Below (orbit and surface) – lander color panorama (top) and orbital view from NASA’s LRO orbiter (bottom). Chang’e-3 lander color panorama shows Yutu rover after it drove down the ramp to the moon’s surface and began driving around the landers right side to the south. Yellow lines connect craters seen in the lander panorama and the LROC image from LRO (taken at a later date after the rover had moved), red lines indicate approximate field of view of the lander panorama. Credit: CNSA/NASA/Ken Kremer/Marco Di Lorenzo/Mark Robinson
Yutu is now nearing its planned 3 month long life expectancy on a moon roving expedition to investigate the moon’s surface composition and natural resources.
The 1200 kg stationary lander is functioning normally. It is as expected to return science data about the Moon and conduct telescopic observations of the Earth and celestial objects for at least one year.
Yutu, which translates as ‘Jade Rabbit’ is named after the rabbit in Chinese mythology that lives on the Moon as a pet of the Moon goddess Chang’e.
“We all wish it would be able to wake up again,” said Ye according to CCTV, China’s state run broadcaster.
Ye will be reporting about Yutu and the Chang’e-3 mission at the annual session of the top advisory body, which opened today, Monday, March 3.
China is only the 3rd country in the world to successfully soft land a spacecraft on Earth’s nearest neighbor after the United States and the Soviet Union.
Stay tuned here for Ken’s continuing Chang’e-3, Orion, Orbital Sciences, SpaceX, commercial space, Curiosity, GPM, LADEE, Mars and more planetary and human spaceflight news. Learn more at Ken’s upcoming presentations at the NEAF convention on April 12/13.
A solar halo was visible neara the Chilidog Observatory in Monterrey, Mexico. Credit and copyright: César Cantú.
Here’s a few great astrophotos for today! Astrophotographer César Cantú from the Chilidog Observatory in Monterrey, Mexico captured this stunning halo around the Sun on March 2, 2014. A solar halo is an optical phenomenon produced by ice crystals creating colored or white arcs and spots in the sky. Conditions in the atmosphere have to be just right, with moisture or ice crystals creating a “rainbow” effect around the Sun. Sometimes the halos surround the Sun completely, other times, they appear as arcs around the Sun creating what is known as sundogs. Basically, sunlight is reflecting off moisture in the atmosphere.
Ice crystals in Earth’s atmosphere can also cause rings around the Moon, and moondogs and even Venus “pillars.”
But make sure you look at the crescent Moon tonight — if you’ve missed seeing the thin crescent the past two evenings, tonight it will still be only 11% illuminated (according to Universe Today’s Phases of the Moon app!). Tonight you still might have the chance to see a little Earthshine — reflected Earthlight visible on the Moon’s night side.
See some great crescent Moon and Earthshine images below!
This image comes from one of our “regulars,” John Chumack, who says, “If you have clear skies, go out again tonight (03-03-2014) and look West between 7:00pm and 8:00pm EST, you will see the crescent Moon with Earthshine!”
Also, just another note from John: between 7:00 pm and 8:00 pm the Planet Uranus is 7.5 degrees below the Crescent Moon just after Sunset, but you will not see Uranus until it gets dark enough. You will need a telescope or binoculars to easily view Uranus at Magnitude 5.9, shortly after 8:15pm Uranus will set in the west and then the Moon follows shortly after that.
The young thin Crescent Moon with Earthshine was hanging low in the west near Tampa, Florida on March 2, 2014. Credit and copyright: John Chumack.The Crescent Moon at 2.45 days old on March 3, 2014. Credit and copyright: James Lennie.Crescent Moon with Earthshine on March 3, 2014. Credit and copyright: Raymond Gilchrist.
Want to get your astrophoto featured on Universe Today? Join our Flickr group or send us your images by email (this means you’re giving us permission to post them). Please explain what’s in the picture, when you took it, the equipment you used, etc.
Electricity is a form of energy and it occurs in nature, so it was not “invented.” As to who discovered it, many misconceptions abound. Some give credit to Benjamin Franklin for discovering electricity, but his experiments only helped establish the connection between lightning and electricity, nothing more.
The truth about the discovery of electricity is a bit more complex than a man flying his kite. It actually goes back more than two thousand years.
In about 600 BC, the Ancient Greeks discovered that rubbing fur on amber (fossilized tree resin) caused an attraction between the two – and so what the Greeks discovered was actually static electricity. Additionally, researchers and archeologists in the 1930’s discovered pots with sheets of copper inside that they believe may have been ancient batteries meant to produce light at ancient Roman sites. Similar devices were found in archeological digs near Baghdad meaning ancient Persians may have also used an early form of batteries.
A replica and diagram of one of the ancient electric cells (batteries) found near Bagdad.
But by the 17th century, many electricity-related discoveries had been made, such as the invention of an early electrostatic generator, the differentiation between positive and negative currents, and the classification of materials as conductors or insulators.
In the year 1600, English physician William Gilbert used the Latin word “electricus” to describe the force that certain substances exert when rubbed against each other. A few years later another English scientist, Thomas Browne, wrote several books and he used the word “electricity” to describe his investigations based on Gilbert’s work.
Benjamin Franklin. Image Source: Wikipedia
In 1752, Ben Franklin conducted his experiment with a kite, a key, and a storm. This simply proved that lightning and tiny electric sparks were the same thing.
Italian physicist Alessandro Volta discovered that particular chemical reactions could produce electricity, and in 1800 he constructed the voltaic pile (an early electric battery) that produced a steady electric current, and so he was the first person to create a steady flow of electrical charge. Volta also created the first transmission of electricity by linking positively-charged and negatively-charged connectors and driving an electrical charge, or voltage, through them.
In 1831 electricity became viable for use in technology when Michael Faraday created the electric dynamo (a crude power generator), which solved the problem of generating electric current in an ongoing and practical way. Faraday’s rather crude invention used a magnet that was moved inside a coil of copper wire, creating a tiny electric current that flowed through the wire. This opened the door to American Thomas Edison and British scientist Joseph Swan who each invented the incandescent filament light bulb in their respective countries in about 1878. Previously, light bulbs had been invented by others, but the incandescent bulb was the first practical bulb that would light for hours on end.
Replica of Thomas Edison’s first lightbulb. Credit: National Park Service.
Swan and Edison later set up a joint company to produce the first practical filament lamp, and Edison used his direct-current system (DC) to provide power to illuminate the first New York electric street lamps in September 1882.
Later in the 1800’s and early 1900’s Serbian American engineer, inventor, and all around electrical wizard Nikola Tesla became an important contributor to the birth of commercial electricity. He worked with Edison and later had many revolutionary developments in electromagnetism, and had competing patents with Marconi for the invention of radio. He is well known for his work with alternating current (AC), AC motors, and the polyphase distribution system.
Later, American inventor and industrialist George Westinghouse purchased and developed Tesla’s patented motor for generating alternating current, and the work of Westinghouse, Tesla and others gradually convinced American society that the future of electricity lay with AC rather than DC.
Others who worked to bring the use of electricity to where it is today include Scottish inventor James Watt, Andre Ampere, a French mathematician, and German mathematician and physicist George Ohm.
And so, it was not just one person who discovered electricity. While the concept of electricity was known for thousands of years, when it came time to develop it commercially and scientifically, there were several great minds working on the problem at the same time.
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
