Love observing the Moon? There’s a new iPhone, iPod and iPad app that will provide everything you need to know. LunarCalc shows moon phases from any date between the years 1900 and 2200. It also provides ecliptic latitude and longitude, zodiacal position, distance from Earth, and apogee and perigee dates. The iPad version also provides moonrise, moonset and culmination, percent illuminated and lunation period.
LunarCalc is available in eight languages: English, Spanish, French, Italian, German Portuguese, Russian and Japanese.
Courtesy of the app’s creator, Fabio Rendelucci, Universe Today has 3 LunarCalc apps to giveaway. The first three correct answers to the following question will win. Post your answer in the comment section.
Question: When will the next total lunar eclipse take place?
To find out more or to buy the app, search “LunarCalc” in iTunes to download it.
Opportunity rover at the SW rim of Santa Maria Crater on New Year's Eve 2010 - Sol 2466. The rover sits at the edge of the crater rim and was photographed from Mars orbit by the HiRISE camera aboard NASA’s Mars Reconnaissance Orbiter. Look closely to see the rover tracks on the left as Opportunity approached the westerm rim of Santa Maria crater. Credit: NASA/JPL/University of Arizona
[/caption]
“I enjoy seeing our rover again,“ says Steve Squyres in an exclusive for Universe Today. Squyres is the top scientist for the Opportunity and Spirit Mars rovers.
NASA’s Opportunity rover was just been photographed from Mars Orbit while perched at the precipice of Santa Maria crater – just meters away from the edge of the Southwest rim. The photo was taken on New Year’s Eve, Dec. 31, 2010 on Sol 2466 of the mission which has lasted nearly 7 years ! Opportunity landed on Mars on Jan. 24, 2004.
“Well, it’s always great to see images like that,” Steve Squyres just informed me after seeing the new photos of Opportunity. Squyres, of Cornell University, is the Principal Scientific Investigator for NASA’s Spirit and Opportunity Mars rovers.
“This one reminds me a lot of the first time we ever saw a rover from orbit, just after Opportunity had arrived at the rim of Victoria crater. It’s a very evocative scene, and it’s hard not to project certain things onto the rover (“valiant”, “lonely”) when you see it. Mostly, though, I just enjoy seeing our rover again.”
“The last time I laid eyes on Opportunity was about seven and a half years ago, and it’s nice getting another glimpse of her,” said Squyres.
Oblique view of Opportunity on New Years Eve 2010 from Mars Orbit. HiRISE also took an an oblique view of the same area of Mars. This image shows the view looking West, as MRO pointed off nadir 18 degrees to the West to acquire this oblique image, similar to the view out an airplane window. Credit: NASA/JPL/University of Arizona
Opportunity arrived at the western rim of Santa Maria on Dec. 16 (Sol 2451) after a long and arduous trek of some 19 km since departing from Victoria Crater over 2 years ago in September 2008.
The rover has been exploring around the western portion of Santa Maria crater since arriving and is now heading to the southeast rim which possesses deposits of hydrated minerals.
Opportunity drove some 40 meters south along the steep rim from the initial location at “Palos” Promontory and then bumped incrementally further up to the edge on Sol 2464 at a place dubbed “Wanahani”.
The rover was photographed from Mars orbit while perched at “Wanahani” on New Years Eve, Dec 31, 2010 on Sol 2466.
“We are driving the vehicle in a counterclockwise direction around Santa Maria to reach the very interesting hydrated sulfates on the other side,” according to Ray Arvidson, the deputy principal investigator for the rovers, in an interview from Washington University in St. Louis. “We’ll make 3 stops or more depending on what we see”
Simultaneously to being photographed from orbit, the rover itself was of course merrily snapping a ground level view of Santa Maria. To experience the surface eye view from Opportunity, see our photo mosaic – stitched from the raw images – to display the rovers panoramic perspective whilst gazing outwards from “Wanahani” to the cliffs of Santa Maria on Sols 2464 and 2466.
Opportunity’s surface view of Santa Maria on New Years Eve Dec 31 while being photographed overhead from Mars Orbit.
Wanahani outlook at Santa Maria Crater. Opportunity took this panaromic mosaic from “Wanhani” just meters from the crater rim on Dec 29, 2010 (Sol 2464). Note rover tracks near rim at left, relatively clean solar panel at right and numerous ejecta rocks. The rim is inclined roughly 5 degrees here. CRISM mapper results suggest water bearing materials are located at the southeastern edge of the crater rim, nicknamed “Yuma”. Portions of distant Endeavour Crater are faintly visible as bumps on the horizon in the background. Mosaic Credit: NASA/JPL/Cornell, Ken Kremer, Marco Di Lorenzo
“Opportunity is imaging the crater interior to better understand the geometry of rock layers as a means of defining the stratigraphy and the impact process, says Matt Golembek, Mars Exploration Program Landing Site Scientist at the Jet Propulsion Laboratory (JPL), Pasadena, Calif.
Santa Maria is a relatively young, 90 meter-diameter impact crater (note blocks of ejecta around the crater), but old enough to collect sand dunes in its interior.
Santa Maria Crater, located in Meridiani Planum, is about 6 kilometers from the rim of Endeavour Crater, which contains spectral indications of phyllosilicates, or clay bearing minerals that are believed to have formed in wet conditions that could have been more habitable than the later acidic conditions in which the sulfates Opportunity has been exploring formed.
Data from the CRISM mineral mapper aboard MRO data show indications of hydrated sulfates on the Southeast edge of the Santa Maria Crater at which Opportunity is planning on spending the upcoming solar conjunction. After that, Opportunity will traverse to the Northwest rim of Endeavour Crater, aided tremendously by HiRISE images like the one here for navigation and targeting interesting smaller craters along the way.
Opportunity rover at the SW rim of Santa Maria Crater on New Year's Eve 2010 - Sol 2466. The rover sits at the edge of the crater rim and was photographed from Mars orbit by the HiRISE camera aboard NASA’s Mars Reconnaissance Orbiter. Look closely to see the rover tracks on the left as Opportunity approached the westerm rim of Santa Maria crater. Credit: NASA/JPL/University of Arizona
Colors are important in astronomy. They can be used to get a quick feel for the temperature of stars, map out hydrogen alpha, or even find oxygen when it gives off a distinctive green glow from the forbidden transistion. Yet thus far, all images of exoplanets have only been taken in a single color filter leaving astronomers with a flat picture and no understanding of the color of a planet. A new paper corrects this oversight while analyzing the polarization of reflected starlight to develop an understanding of the characteristics of the planet’s atmosphere.
One of the properties of light is that it often becomes polarized upon reflection. This allows for polarized sunglasses to effectively reduce glare from road surfaces because the reflection tends to polarize the light in a preferred direction. Similarly, light striking a planet’s atmosphere will have a preferred axis of polarization. The degree of polarization will depend on many factors including, the angle of incidence (corresponding to the planetary phase), the types of molecules in the atmosphere, and the color, or wavelength, of light through which the planet is observed.
The object of interest was HD189733b and observations were taken in using the UBV filters system which uses filters in the ultra-violet, blue, and green (or “visible”) portions of the spectra. They were conduced at the Nordic Optical Telescope in Spain.
To control for the variations, astronomers would need to observe the planet at several wavelengths to understand how the color was affecting the results, as well as to watch the planet for several orbits to trace how the phase impacted the observations. Presently, the authors have not gone so far as to compare various composition models against these observations as this study was largely intended to be a feasibility study at multi-wavelength polarization detection.
Results have shown that the planet is brightest in the blue portion of the spectra, a result that confirms earlier, theoretical predictions for hot Jupiters as well as tentative observational findings based on single color studies done last year. This supports the notion that the dominant mechanism of polarization is Rayleigh scattering in the atmosphere. The result of this is that the planet would likely appear to be a deep blue to the naked eye, much the same way our sky appears blue, but a much more vivid color due to the increased depth to which we would look. The observations also confirmed that polarization was greatest when the planet was near greatest elongation (as far to either side of the star as possible instead of near in front or behind when viewed from Earth) which supports that the polarization is due to scattering in the atmosphere as opposed to the starlight being initially polarized from large starspots.
Certainly, this study has demonstrated the potential for astronomers to begin exploring planetary characteristics with polarization. However, it may be some time before it becomes accepted in general use. While the findings were certainly above the background noise, there existed a significant degree of uncertainty in the measurements resulting from the faint nature of planets. Being a large, hot Jupiter, HD189733b is a strong candidate since it is close to its parent star and thus, receives a large amount of light. Using such methods for other exoplanets, more distant from their parent stars will likely prove an even more daunting task, requiring careful preparation and observations.
This flag flew to the Moon and back with the Apollo 11 crew. It's one of the many items from the history of spaceflight up for sale at an upcoming auction. Image Credit: RR Auction
[/caption]
If you’re interested in owning an artifact or two from the history of spaceflight, now could be your chance to snag some up. From January 13-20, over 400 artifacts relating to the history of spaceflight will be up on the auction block at RR Auction. There’s a diverse number of different pieces, ranging from an Atlas I and II crow’s foot wrench to numerous items that flew aboard many of the Apollo missions and on Projects Mercury and Gemini.
There are even a few spare parts for the Shuttle, though it’s probably not a good idea to follow along in Johnny Cash’s footsteps; if you build a space shuttle one piece at a time, it’ll cost you more than a dime and I doubt you’ll want to fly it into space.
This auction is filled with loads of memorabilia – much of it signed by astronauts or other NASA personnel – from the Apollo missions. There is a US flag that flew with the Apollo 11 crew to the Moon and back, attached to a certificate signed by Armstrong, Aldrin and Collins. As you can imagine, this one is going to go for a lot – the bidding starts at $2500. If you drill it out so it'll fit, and with a little help from an A-daptor kit, you could have a shuttle running just like a song. Image Credit: RR Auction. Mangled lyrics credit: The Man in Black
One piece that has been getting a lot of attention – and will probably also sell for quite a lot, given that it starts out at $1000 – is the original page from the November 1969 Playboy magazine featuring topless Playmate DeDe Lind. The page was stuck to a piece of cardboard aboard Apollo 12, and traveled all the way to the Moon and back aboard the Yankee Clipper.
It’s accompanied by a certificate of authenticity from Richard Gordon, the Apollo 12 Command Module pilot, which reads in part: “This cue card, which flew with me to the moon, has been in my sole possession and part of my personal space collection since my return from the moon in 1969 aboard America’s second lunar landing mission, and it remains one of the all-time greatest Apollo era astronaut ‘Gotcha’s!’” Historic, indeed.
This photograph of the Sun, taken by the Atmospheric Imaging Assembly (AIA) instrument on NASA's Solar Dynamics Observatory reveals the faint, inner corona. At the Sun's limb, prominences larger than the Earth arc into space. Bright active regions like the one on the Sun's face at lower center are often the source of huge eruptions known as coronal mass ejections. Credit: NASA/LMSAL/SAO
[/caption]
Usually the only time we can see the innermost part of the Sun’s corona is when there is a total eclipse. But now, with the Atmospheric Imaging Assembly (AIA) instrument on NASA’s Solar Dynamics Observatory and a new image processing program, scientists are getting unprecedented views of the innermost corona 24 hours a day, 7 days a week.
“The AIA solar images, with better-than-HD quality views, show magnetic structures and dynamics that we’ve never seen before on the Sun,” said astronomer Steven Cranmer from the Harvard-Smithsonian Center for Astrophysics (CfA). “This is a whole new area of study that’s just beginning.”
The Sun’s outer layer, or corona is composed of light, gaseous matter, and has two parts. The outer corona is white, with streamers extending out millions of miles from the edge of the sun. The inner corona, lying next to the red chromosphere, is a band of pale yellow.
This zoomed-in image shows how the Sun's magnetic field shapes hot coronal plasma. Photos like this highlight the ever-changing connections between gas captured by the Sun's magnetic field and gas escaping into interplanetary space. Credit: NASA/LMSAL/SAO
This outer layer of the Sun’s atmosphere is, paradoxically, hotter than the Sun’s surface, but so tenuous that its light is overwhelmed by the much brighter solar disk. The corona becomes visible only when the Sun is blocked, which happens for just a few minutes during an eclipse.
Now, with AIA, “we can follow the corona all the way down to the Sun’s surface,” said Leon Golub of the CfA.
Previously, solar astronomers could observe the corona by physically blocking the solar disk with a coronagraph, much like holding your hand in front of your face while driving into the setting Sun. However, a coronagraph also blocks the area immediately surrounding the Sun, leaving only the outer corona visible.
The AIA instrument on SDO allows astronomers to study the corona all the way down to the Sun’s surface.
Cranmer and CfA colleague Alec Engell developed a computer program for processing the AIA images above the Sun’s edge. These processed images imitate the blocking-out of the Sun that occurs during a total solar eclipse, revealing the highly dynamic nature of the inner corona. They will be used to study the initial eruption phase of coronal mass ejections (CMEs) as they leave the Sun and to test theories of solar wind acceleration based on magnetic reconnection.
The resulting images highlight the ever-changing connections between gas captured by the Sun’s magnetic field and gas escaping into interplanetary space.
This time-lapse movie shows two days of solar activity observed by the AIA instrument. Both the solar surface and dynamic inner corona are clearly visible in X-rays. Hot solar plasma streams outward in vast loops larger than Earth before plunging back onto the Sun’s surface. Some of the loops expand and stretch bigger and bigger until they break, belching plasma outward.
SDO launched in February 2010.
This video provides more information about the AIA instrument:
A new look at the Eagle Nebula by Hubble. Credit: ESA/Hubble & NASA
[/caption]
There are some stellar powerhouses inside the Eagle Nebula, and Hubble has captured a collection of these hot, blue stars. These dazzling stars are an open star cluster called NGC 6611, whose fierce ultraviolet glow make the surrounding Eagle Nebula glow brightly. But there are also areas in this image that look dark and empty. Are those areas just empty? No, they are actually very dense regions of gas and dust, which obstruct light from passing through.
Hubble astronomers say that many of these dark areas may be hiding the sites of the early stages of star formation, before the fledgling stars clear away their surroundings and burst into view. Dark nebulae, large and small, are dotted throughout the Universe. If you look up to the Milky Way with the naked eye from a dark, remote site, you can easily spot some huge dark nebulae blocking the background starlight.
This region in the Eagle Nebula formed about 5.5 million years ago and is found approximately 6,500 light-years from the Earth. The cluster and the associated nebula together are also known as Messier 16.
Astronomers refer to areas like the Eagle Nebula as HII regions. This is the scientific notation for ionised hydrogen from which the region is largely made. Extrapolating far into the future, this HII region will eventually disperse, helped along by shockwaves from supernova explosions as the more massive young stars end their brief but brilliant lives.
This picture was created from images from Hubble’s Wide Field Channel of the Advanced Camera for Surveys through the unusual combination of two near-infrared filters (F775W, colored blue, and F850LP, colored red). The image has also been subtly colorized using a ground-based image taken through more conventional filters. The Hubble exposure times were 2000 s in both cases and the field of view is about 3.2 arcminutes across.
A before and after animation of Supernova 2010lt. Credit: Dave Lane
A ten-year old girl from Canada has discovered a supernova, making her the youngest person ever to find a stellar explosion. The Royal Astronomical Society of Canada announced the discovery by Kathryn Aurora Gray of Fredericton, New Brunswick, (wonderful middle name!) who was assisted by astronomers Paul Gray and David Lane. Supernova 2010lt is a magnitude 17 supernova in galaxy UGC 3378 in the constellation of Camelopardalis, as reported on IAU Electronic Telegram 2618. The galaxy was imaged on New Year’s Eve 2010, and the supernova was discovered on January 2, 2011 by Kathryn and her father Paul.
7 years on Mars for Spirit and Opportunity. Poster by Glen Nagle. Click for access to downloadable versions.
[/caption]
Today, January 3, 2011, is the 7th anniversary of the Spirit rover landing on Mars. In their tradition, Glen Nagle and Stu Atkinson from Unmanned Spaceflight have teamed up to create a poster and poem combo to celebrate. The poster includes scenes from both Spirit’s and Opportunity’s adventures – Glen and Stu challenge you to see how many places you can name. Click on the images or visit Glen’s Astro0 website for higher resolution versions that you can download to print a poster or use for wallpaper.
And happy anniversary to the Mars Exploration Rovers and their science and engineering teams!
MER poster with poem by Stu Atkinson. Image by Glen Nagle. Click for access to higher resolution versions.
In just a few hours the peak of the first meteor shower of 2011 will begin – the Quadrantids. Where did these mysterious meteors begin their life and how can you observe one yourself? Then step inside…
Beginning each New Year and lasting for nearly a week, the Quadrantid Meteor Shower sparkles across the night sky for nearly all viewers around the world. Its radiant belongs to an extinct constellation once known as Quadran Muralis, but any meteors will seem to come from the general direction of bright Arcturus and Bootes. This is a very narrow stream, which may have once belonged to a portion of the Aquarids, but recent scientific data points to a what may have been a cosmic collision. According the most recent data, the Quandrantid meteors may have been formed about five centuries ago when a near-Earth asteroid named 2003 EH1 and a comet smashed into one another. Historic records from ancient China put comet C/1490 Y1 in the path of probability.
As Jupiter‘s gravity continues to perturb the stream, another 400 years may mean this shower will become as extinct as the constellation for which it was once known, but we aren’t out of the running just yet. “Peaking in the wee morning hours of Tuesday, Jan. 4, the Quads have a maximum rate of about 100 per hour (varies between 60 and 200),” says Bill Cooke of NASA’s Meteoroid Environment Office. “What makes this year so special is that the Moon is New on the night of the peak, so there will be no interference from moonlight.”
As exciting as it may seem, there are a few problems associated with observing the Quadrantid meteor shower. The first is the weather, because this northern hemisphere show occurs during a notoriously cold season making observations uncomfortable at best. The second is the brevity of the activity itself. Because Earth intersects the debris orbit of 2003 EH1 at a perpendicular angle, we zip right through the trail. That’s why the shower activity is so fast and slightly unpredictable. A third consideration is the high probability of cloud cover – but take heart… NASA has you covered!
“Got clouds? No problem.” says SpaceWeather. “You can stay inside and listen to the Quadrantids. Tune into SpaceWeather Radio for a live audio stream from the Air Force Space Surveillance Radar. When a Quadrantid passes over the facility, you will hear a “ping” caused by the radar’s powerful transmitter echoing from the meteor’s ion trail. During the shower’s peak, the soundtrack is guaranteed to entertain.
So where and when to look? “You can start watching after 2:30am in the North to North East look between the handle of the Big Dipper -Ursa Major and the Constellation of Bootes or the Kite shaped constellation, this is the radiant location as the Meteors will appear to radiate from this general area.” says professional astrophotographer, John Chumack. “Or after 2:30am simply look between the North Star and bright star Arcturus in the East. The Quadrantid Meteors will appear to be coming from this general area of the sky. There is no moon present during this year’s shower, so you can watch all night if you like without moonlight interfering, but the best time will be after 2:30am. As the night goes on the Big Dipper, Bootes and Arcturus climb higher into the sky, so keep watching because the number of meteors usually picks up after 2:30am and gets better through 6:00am. as Earth rotates into the stream. Meteors can appear anywhere in the sky, so look in all directions of the sky as the Quadrantid radiant reaches straight over head. The Quadrantid Meteors are rather fast movers. They enter the atmosphere at about 90,000 to 120,000mph, and can have some impressive long trails.”
Will the Quadrantid Meteor Shower live up to its expectations? No one knows for sure… But we’ll be watching!
Many thanks to John Chumack of Galactic Images for his inspiring photo and to NASA for the locator chart. We thank you so much!
