Signs posted outside launch Pad-OA at the NASA Wallops Flight Facility. Credit: NASA/Bill Ingalls.
These custom road signs at NASA’s Wallops Flight Facility are, well, out of this world with awesomeness. They refer to the recent launch of the LADEE spacecraft to the Moon and the upcoming launch this week of the Orbital Sciences Corporation Antares rocket, with its Cygnus cargo spacecraft heading to the International Space Station for a demonstration cargo resupply mission. Launch is currently scheduled for Wednesday, September 18 during a window of 10:50-11:05 am EDT (14:50-15:05 UTC).
A jet of energetic particles (shown in magenta) is shaping the environment around the star IRAS 15445-5449. Infrared light from dusty material which the jet has already shaped into a symmetric form is shown in green. The star itself is hidden by dust in its environment. Credit: E. Lagadec/ESO/A. Pérez Sánchez)
The incredible visual appearance of planetary nebulae are some of the most studied and observed of deep space objects. However, these enigmatic clouds of gas have defied explanation as to their shapes and astronomers are seeking answers. Thanks to a new discovery made by an international team of scientists from Sweden, Germany and Austria, we have now observed a jet of high-energy particles in the process of being ejected from an expiring star.
When a sun-like star reaches the end of its life, it begins to shed itself of its outer layers. These layers blossom into space at speeds of a few kilometers per second, forming a variety of shapes and sizes – yet we know little about what causes their ultimate appearance. Now astronomers are taking a close look at a rather normal star that has reached the end of its life and is beginning to form a planetary nebula. Cataloged as IRAS 15445-5449, this stellar study resides 230,000 light years away in the constellation of Triangulum Australe (the Southern Triangle). Through the use of the CSIRO Australia Telescope Compact Array, a compliment of six 22-meter radio telescopes in New South Wales, Australia, researchers have found what may be the answer to this mystery… high-speed magnetic jets.
“In our data we found the clear signature of a narrow and extremely energetic jet of a type which has never been seen before in an old, Sun-like star,” says Andrés Pérez Sánchez, graduate student in astronomy at Bonn University, who led the study.
How does a radio telescope aid researchers in an optical study? In this case the radio waves emitted by the dying star are compatible with the trademark high-energy particles they are expected to produce. These “spouts” of particles travel at nearly the speed of light and coincident jets are also known to emanate from other astronomical objects that range from newborn stars to supermassive black holes.
“What we’re seeing is a powerful jet of particles spiraling through a strong magnetic field,” says Wouter Vlemmings, astronomer at Onsala Space Observatory, Chalmers. “Its brightness indicates that it’s in the process of creating a symmetric nebula around the star.”
Will these high-energy particles contained within the jet eventually craft the planetary nebula into an ethereal beauty? According to the astronomers, the current state of IRAS 15445-5449 is probably a short-lived phenomenon and nothing more than an intense and dramatic phase in its life… One we’re lucky to have observed.
“The radio signal from the jet varies in a way that means that it may only last a few decades. Over the course of just a few hundred years the jet can determine how the nebula will look when it finally gets lit up by the star,” says team member Jessica Chapman, astronomer at CSIRO in Sydney, Australia.
Will our Sun also follow suit? Right now the answer is unclear. There may be more to this radio picture than meets the ear. However, rest assured that this new information is being heard and might well become the target of additional radio studies. Considering the life of a planetary nebula is generally expected to last few tens of thousands of years, this is a unique opportunity for astronomers to observe what might be a transient occurrence.
“The star may have an unseen companion – another star or large planet — that helps create the jet. With the help of other front-line radio telescopes, like ALMA, and future facilities like the Square Kilometre Array (SKA), we’ll be able to find out just which stars create jets like this one, and how they do it,” says Andrés Pérez Sánchez.
The zodiacal light in the Nevada dawn. The plane of the ecliptic can be traced by Jupiter in Gemini & Mars in the Beehive cluster just below center. (Credit: Cory Schmitz, used with permission).
This week leading up to the September equinox offers you a fine chance to catch an elusive phenomenon in the pre-dawn sky.
We’re talking about the zodiacal light, the ghostly pyramid-shaped luminescence that heralds the approach of dawn. Zodiacal light can also be seen in the post-dusk sky, extending from the western horizon along the ecliptic.
September is a great time for northern hemisphere observers to try and sight this glow in the early dawn. This is because the ecliptic is currently at a high and favorable angle, pitching the zodiacal band out of the atmospheric murk low to the horizon. For southern hemisphere observers, September provides the best time to hunt for the zodiacal light after dusk. In March, the situation is reversed, with dusk being the best for northern hemisphere observers and dawn providing the best opportunity to catch this elusive phenomenon for southern observers.
The clash of the zodiacal light and the plane of our galaxy. (Credit: Cory Schmitz, used with permission).
Cory Schmitz’s recent outstanding photos taken from the Nevada desert brought to mind just how ephemeral a glimpse of the zodiacal light can be. The glow was a frequent sight for us from dark sky sites just outside of Tucson, Arizona—but a rarity now that we reside on the light-polluted east coast of the U.S.
In order to see the zodiacal light, you’ll need to start watching before astronomical twilight—the start of which is defined as when the rising Sun reaches 18 degrees below the local horizon—and observe from as dark a site as possible under a moonless sky.
The Bortle dark sky scale lists the zodiacal light as glimpse-able under Class 4 suburban-to-rural transition skies. Under a Class 3 rural sky, the zodiacal light may extend up to 60 degrees above the horizon, and under truly dark—and these days, almost mythical—Class 1 and 2 skies, the true nature of the zodiacal band extending across the ecliptic can become apparent. The appearance and extent of the zodiacal light makes a great gauge of the sky conditions at that favorite secret dark sky site.
The source of the zodiacal light is tiny dust particles about 10 to 300 micrometres in size scattered across the plane of the solar system. The source of the material has long been debated, with the usual suspects cited as micrometeoroid collisions and cometary dust. A 2010 paper by Peter Jenniskens and David Nesvorny in the Astrophysical Journal cites the fragmentation of Jupiter-class comets. Their model satisfactorily explains the source of about 85% of the material. Dust in the zodiacal cloud must be periodically replenished, as the material is slowly spiraling inward via what is known as the Poynting-Robertson effect. None other than Brian May of the rock group Queen wrote his PhD thesis on Radial Velocities in the Zodiacal Dust Cloud.
But even if you can’t see the zodiacal light, you still just might be able to catch it. Photographing the zodiacal light is similar to catching the band of the Milky Way. In fact, you can see the two crossing paths in Cory’s images, as the bright winter lanes of the Orion Spur are visible piercing the constellation of the same name. Cory used a 14mm lens at f/3.2 for the darker image with a 20 second exposure at ISO 6400 and a 24mm lens at f/2.8 with a 15 second exposure at ISO 3200 for the brighter shot.
The orientation of the ecliptic & the zodiacal band as seen from latitude 30 deg north in September, about 1 hour before sunrise. (Created by the author in Stellarium).
Under a truly dark site, the zodiacal light can compete with the Milky Way in brightness. The early Arab astronomers referred to it as the false dawn. In recent times, we’ve heard tales of urbanites mistaking the Milky Way for the glow of a fire on the horizon during blackouts, and we wouldn’t be surprised if the zodiacal light could evoke the same. We’ve often heard our friends who’ve deployed to Afghanistan remark how truly dark the skies are there, as military bases must often operate with night vision goggles in total darkness to avoid drawing sniper fire.
Another even tougher but related phenomenon to spot is known as the gegenschein. This counter glow sits at the anti-sunward point where said particles are approaching 100% illumination. This time of year, this point lies off in the constellation Pisces, well away from the star-cluttered galactic plane. OK, we’ve never seen it, either. A quick search of the web reveals more blurry pics of guys in ape suits purporting to be Bigfoot than good pictures of the gegenschein. Spotting this elusive glow is the hallmark of truly dark skies. The anti-sunward point and the gegenschein rides highest near local midnight.
And speaking of which, the September equinox occurs this weekend on the 22nd at 4:44 PM EDT/20:44 Universal Time. This marks the beginning of Fall for the northern hemisphere and the start of summer for the southern.
The Full Harvest Moon also occurs later this week, being the closest Full Moon to the equinox occurring on September 19th at 7:13AM EDT/11:13 UT. Said Moon will rise only ~30 minutes apart on successive evenings for mid-northern latitude observers, owing to the shallow angle of the ecliptic. Unfortunately, the Moon will then move into the morning sky, drowning out those attempts to spy the zodiacal light until late September.
Be sure to get out there on these coming mornings and check out the zodiacal light, and send in those pics in to Universe Today!
This elevated rise on Mercury resembles a vaguely humanoid shape
You’ve all heard of the “face on Mars” and the “man in the Moon” — well I guess this would be the “man on Mercury!” And I feel like I’ve seen him somewhere before…
“Oh, they’ve encased him in carbonite. He should be quite well protected.”
In yet another instance of the phenomenon known as pareidolia, it’s hard not to see the vaguely human shape in this image of Mercury’s surface, acquired by the MESSENGER spacecraft in July 2011. But what looks like a person with upraised arms (resembling, the team suggests, a certain carbonite-encased space smuggler) is really an ancient block of surface crust that juts from the floor of Mercury’s vast Caloris basin — likely the remnants of harder material predating the basin-forming impact 3.9 billion years ago. The low angle of sunlight from the west helps to highlight the surface shapes.
The image above shows an area 96 km (59.7 mi.) across.
If Jabba really wanted to keep his favorite wall decoration safe, perhaps he should have put it on Mercury…
Titan peeks from behind two of Saturn's rings. Another small moon Epimetheus, appears just above the rings. Credit: NASA/JPL/Space Science Institute
Icy volcanoes are likely responsible for changes in brightness on the surface of Titan, the largest moon of Saturn, according to a new study.
Images with the Cassini spacecraft’s visual and infrared mapping spectrometer revealed the brightness, or albedo, of two equatorial areas changing during the study period. Tui Regio (which got darker from 2005 to 2009) and Sotra Patera (which got brighter from 2005 to 2006).
The researchers also pointed to “volcanic-like features” in these areas as evidence that the potential cryovolcanoes, as these icy volcanoes are known, might be connected to an ocean on Titan.
Top: Sotra Patera, a cryovolcanic candidate on Titan that has a one-kilometer crater. (Credit: NASA/JPL Caltech/USGS/University of Arizona). Bottom: The Kirishima volcano in Japan, a terrestrial analogue (Credit: USGS).
“All of these features, plus a need for a methane reservoir and volcanic activity to replenish the methane in the atmosphere, is compatible with the theory of active cryovolcanism on Titan,” stated Anezina Solomonidou , a planetary geologist with the Paris Observatory as well as the National and Kapodistrian University of Athens.
“These results have important implications for Titan’s potential to support life, as these cryovolcanic areas might contain environments that could harbor conditions favorable for life,” Solomonidou added.
Of note, Titan also has a fresh-looking surface with few craters on it, indicating that something might be altering the surface. “Its landscape is remarkably Earth-like with dunes and lakes, erosion due to weathering and tectonic-like features,” a statement on the research added.
There’s been chatter about cryovolcanoes on Titan before. In 2010, researchers said a chain of peaks found on the moon could be evidence of this type of feature. However, a 2012 preliminary California Institute of Technology weather model of the moon explained many of its features without necessarily needing to rely on cryovolcanoes.
Curiosity’s views a rock outcrop after arriving for a short stay at ‘Waypoint 1’- dramatically back dropped by her primary destination, Mount Sharp. Front hazcam camera image from Sol 393 (Sept 13, 2013). Credit: NASA/JPL-Caltech
Curiosity’s views a rock outcrop at ‘Darwin’ after arriving for a short stay at ‘Waypoint 1’ on Sept 12 (Sol 392) – dramatically back dropped by her primary destination, Mount Sharp. Front hazcam camera image from Sol 393 (Sept 13, 2013). Credit: NASA/JPL-Caltech
Story updated – see close up mosaic views of Darwin outcrop below[/caption]
NASA’s Curiosity Mars rover has just rolled into an intriguing site called ‘Darwin’ at ‘Waypoint 1’- having quickly picked up the driving pace since embarking at last on her epic trek to mysterious Mount Sharp more than two months ago. Did life giving water once flow here on the Red Planet?
Because the long journey to Mount Sharp – the robots primary destination – was certain to last nearly a year, the science team carefully choose a few stopping points for study along the way to help characterize the local terrain. And Curiosity has just pulled into the first of these so called ‘Waypoints’ on Sept 12 (Sol 392), the lead scientist confirmed to Universe Today.
“Curiosity has arrived at Waypoint 1,” project scientist John Grotzinger, of the California Institute of Technology in Pasadena, told Universe Today.
“Darwin is named after a geologic formation of rocks from Antarctica.”
She has now driven nearly 20% of the way towards the base of the giant layered Martian mountain she will eventually scale in search of life’s ingredients.
Altogether, the team selected five ‘Waypoints’ to investigate for a few days each as Curiosity travels in a southwestward direction on the road from the first major science destination in the ‘Glenelg’ area to the foothills of Mount Sharp, says Grotzinger.
“We’ll stay just a couple of sols at Waypoint 1 and then we hit the road again,” Grotzinger told me.
Curiosity’s Progress on Rapid Transit Route from ‘Glenelg’ (start at top) to Mount Sharp entry point (bottom). Triangles indicate geologic ‘Waypoint’ stopping points along the way. Curiosity arrived at Waypoint 1 on Sol 392 (Sept 12, 2013). Credit: NASA
‘Waypoint 1’ is an area of intriguing outcrops that was chosen based on high resolution orbital imagery taken by NASA’s Mars Reconnaissance Orbiter (MRO) circling some 200 miles overhead. See route map herein.
In fact the team is rather excited about ‘Waypoint 1’ that’s dominated by the tantalizing rocky outcrop discovered there nicknamed ‘Darwin’.
Although Curiosity will only stay a short time at each of the stops, the measurements collected at each ‘Waypoint’ will provide essential clues to the overall geologic and environmental history of the six wheeled rover’s touchdown zone.
“Waypoint 1 was chosen to help break up the drive,” Grotzinger explained to Universe Today.
“It’s a chance to study outcrops along the way.”
The images from MRO are invaluable in aiding the rover handlers planning activities, selecting Curiosity’s driving route and targeting of the most fruitful science forays during the long trek to Mount Sharp – besides being absolutely crucial for the selection of Gale Crater as the robots landing site in August 2012.
The ‘Darwin’ outcrop may provide more data on the flow of liquid water across the crater floor.
Evolving Excitement Over ‘Darwin’ Rock Outcrop at ‘Waypoint 1’. For at least a couple of days, the science team of NASA’s Mars rover Curiosity is focused on a full-bore science campaign at a tantalizing, rocky site informally called “Darwin.” This view of Darwin was taken with the Mast Camera (Mastcam) on Sol 390 (Sept. 10, 2013). Credit: NASA/JPL-Caltech/Malin Space Science Systems
The scientists goal is to compare the floor of Gale Crater to the sedimentary layers of 3 mile high (5 kilometer high) Mount Sharp.
Waypoint 1 is just over 1 mile along the approximately 5.3-mile (8.6-kilometer) route from ‘Glenelg’ to the entry point at the base of Mount Sharp.
Curiosity spent over six months investigating the ‘Yellowknife Bay’ area inside Glenelg before departing on July 4, 2013.
What’s the origin of Darwin’s name?
“Darwin comes from a list of 100 names the team put together to designate rocks in the Mawson Quadrangle – Mawson is the name of a geologist who studied Antarctic geology,” Grotzinger told me.
“Recently we left the Yellowknife Quadrangle, so instead of naming rocks after geological formations in Canada’s north, we now turn to formation names of rocks from Antarctica, and Darwin is one of them.
“That will be the theme until we cross into the next quad,” Grotzinger explained.
Curiosity investigates the ‘Darwin’ rock outcrop up close after arriving for a short stay at ‘Waypoint 1’ on Sept 12 (Sol 392). This photo mosaic was assembled from navcam images taken on Sept 12, 2013. Credit: NASA/JPL-Caltech/Ken Kremer/Marco Di Lorenzo
Inside Yellowknife Bay, Curiosity conducted the historic first interplanetary drilling into Red Planet rocks and subsequent sample analysis with her duo of state of the art chemistry labs – SAM and CheMin.
At Yellowknife Bay, the 1 ton robot discovered a habitable environment containing the chemical ingredients that could sustain Martian microbes- thereby already accomplishing the primary goal of NASA’s flagship mission to Mars.
“We want to know how the rocks at Yellowknife Bay are related to what we’ll see at Mount Sharp,” Grotzinger elaborated in a NASA statement. “That’s what we intend to get from the waypoints between them. We’ll use them to stitch together a timeline — which layers are older, which are younger.”
On Sept. 5, Curiosity set a new one-day distance driving record for the longest drive yet by advancing 464 feet (141.5 meters) on her 13th month on the Red Planet.
As Curiosity neared Waypoint 1 she stopped at a rise called ‘Panorama Point’ on Sept. 7, spotted an outcrop of light toned streaks informally dubbed ‘Darwin and used her MastCam telephoto camera to collect high resolution imagery.
Curiosity will use her cameras, spectrometers and robotic arm for contact science and a “full bore science campaign” involving in-depth mineral and chemical composition analysis of Darwin and Waypoint 1 for the next few Sols, or Martian days, before resuming the trek to Mount Sharp that dominates the center of Gale Crater.
Curiosity Spies Mount Sharp – her primary destination. Curiosity will ascend mysterious Mount Sharp and investigate the sedimentary layers searching for clues to the history and habitability o the Red Planet of billions of years. This mosaic was assembled from Mastcam camera images taken on Sol 352 (Aug 2, 2013). Credit: NASA/JPL-Caltech/MSSS/ Marco Di Lorenzo/Ken Kremer
She will not conduct any drilling here or at the other waypoints, several team members have told me, unless there is some truly remarkable ‘Mars-shattering’ discovery.
Why is Curiosity now able to drive longer than ever before?
“We have put some new software – called autonav, or autonomous navigation – on the vehicle right after the conjunction period back in March 2013,” Jim Erickson, Curiosity Project Manager of NASA’s Jet Propulsion Laboratory (JPL), told Universe Today.
“This will increase our ability to drive. But how much it helps really depends on the terrain.”
And so far the terrain has cooperated.
“We are on a general heading of southwest to Mount Sharp,” said Erickson. See the NASA JPL route map.
“We have been going through various options of different planned routes.”
As of today (Sol 394), Curiosity remains healthy, has traveled 2.9 kilometers and snapped over 82,000 images.
If all goes well Curiosity could reach the entry point to Mount Sharp sometime during Spring 2014, at her current driving pace.
Learn more about Curiosity, Mars rovers,LADEE, Cygnus, Antares, MAVEN, Orion and more at Ken’s upcoming presentations
Sep 17/18: LADEE Lunar & Antares/Cygnus ISS Rocket Launches from Virginia”; Rodeway Inn, Chincoteague, VA
Oct 3: “Curiosity, MAVEN and the Search for Life on Mars – (3-D)”, STAR Astronomy Club, Brookdale Community College & Monmouth Museum, Lincroft, NJ, 8 PM
Oct 8: LADEE Lunar & Antares/Cygnus ISS Rocket Launches from Virginia”; Princeton University, Amateur Astronomers Assoc of Princeton (AAAP), Princeton, NJ, 8 PM
Once a week or so, we try to organize a giveaway for Universe Today readers with various sponsors. Sometimes it’s books, clothing, DVDs, apps or tickets to space-related stuff.
Entering the giveaways is easy. All you have to do is enter your email address into the box at the bottom of the giveaway and you’re entered. This also adds you to our giveaway email mailing list. Whenever we’ve got a new giveaway, you can click a single link and be entered into the new giveaway (and you can unsubscribe any time).
Don’t worry if you live outside of the US, almost all our giveaways are world wide.
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Are you a skeptical person, overwhelmed with SPAM, and looking for the catch?
I can respect that.
Companies looking to promote their latest books, movies, etc, send me free stuff all the time. It fills my bookshelves and I never have time to use it all. Instead of hoarding it myself, I’d rather just reward Universe Today readers with free stuff.
Companies are able to promote their new space-related products to you; you have a chance to win free stuff; I get to clean out my bookshelves. Win-win-win. Continue reading “Universe Today Giveaways”
Stars swirl over the Batsto Mansion in New Jersey. Credit and copyright: Jack Fusco.
Need a little inspiration to go out and do some stargazing this weekend? Look no further than this gorgeous timelapse by Jack Fusco. There are awesome views of both sea and sky, the Milky Way, star trails, awesome cloud scenes and funky, directionally-challenged moving lights in the sky.
I’ve been working on a timelapse of the night sky over the New Jersey coastline,” Jack told us via email. “New Jersey definitely isn’t the best location for stargazing, but I think given the circumstances, many people will be surprised. I hope it inspires people to set some time aside to stargaze where they live even if they previously thought it wasn’t worth trying.”
Jack said he’s been working on this one for 10 months, and it’s definitely worth the hard work he’s put in.
Jack also gives a shout out to those affected by Hurricane Sandy last year. “A special thank you to all of those who have worked so hard to restore the homes of those lost during Sandy,” he writes on Vimeo. “Thank you to every volunteer that has spent time bringing the beauty back to our boardwalks and our beaches. The last year has been filled with heartbreak and devastation with much work still being done.”
Once again, we have gathered together the forces of space journalism to report on the big news stories of the week. And there were lots of big stories indeed, with the launch of NASA’s LADEE mission to the Moon, and the awesome fact that Voyager 1 has totally left the Solar System.
Host: Fraser Cain
Journalists: Amy Shira Teitel, Nicole Gugliucci, Matthew Francis, David Dickinson, Nancy Atkinson
We record the Weekly Space Hangout every Friday at 12 pm Pacific / 3 pm Eastern as a live Google+ Hangout on Air. You can watch the show from right here on Universe Today, or on our YouTube channel.
