Rhea’s Impact Basins

Rhea’s two large impact basins are shown in this image. Image credit: NASA/JPL/SSI Click to enlarge
This close view of Rhea prominently shows two large impact basins on the ancient and battered moon. The great age of these basins is suggested by the large number of smaller craters that are overprinted within them.

Ejecta from the bright, relatively young crater seen in Crater Contrast spreads from the eastern limb.

Terrain visible in this view is on the side of Rhea (1,528 kilometers, or 949 miles across) that faces away from Saturn. North on Rhea is up and tilted 30 degrees to the left.

This enhanced color view was created by combining images taken using filters sensitive to ultraviolet, visible green and infrared light. The images were taken with the Cassini spacecraft narrow-angle camera on Dec. 23, 2005, at a distance of approximately 341,000 kilometers (212,000 miles) from Saturn and at a Sun-Saturn-spacecraft, or phase, angle of 42 degrees. The image scale is 2 kilometers (1 mile) per pixel.

The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA’s Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging operations center is based at the Space Science Institute in Boulder, Colo.

For more information about the Cassini-Huygens mission visit http://saturn.jpl.nasa.gov . The Cassini imaging team homepage is at http://ciclops.org .

Original Source: NASA/JPL/SSI News Release

Two Stars Kicked Out of the Milky Way

An artist’s conception of an exiled star speeding out of the milkyway. Image credit: Ruth Bazinet, CfA Click to enlarge
TV reality show contestants aren’t the only ones under threat of exile. Astronomers using the MMT Observatory in Arizona have discovered two stars exiled from the Milky Way galaxy. Those stars are racing out of the Galaxy at speeds of more than 1 million miles per hour – so fast that they will never return.

“These stars literally are castaways,” said Smithsonian astronomer Warren Brown (Harvard-Smithsonian Center for Astrophysics). “They have been thrown out of their home galaxy and set adrift in an ocean of intergalactic space.”

Brown and his colleagues spotted the first stellar exile in 2005. European groups identified two more, one of which may have originated in a neighboring galaxy known as the Large Magellanic Cloud. The latest discovery brings the total number of known exiles to five.

“These stars form a new class of astronomical objects – exiled stars leaving the Galaxy,” said Brown.

Astronomers suspect that about 1,000 exile stars exist within the Galaxy. By comparison, the Milky Way contains about 100,000,000,000 (100 billion) stars, making the search for exiles much more difficult than finding the proverbial “needle in a haystack.” The Smithsonian team improved their odds by preselecting stars with locations and characteristics typical of known exiles. They sifted through dozens of candidates spread over an area of sky almost 8000 times larger than the full moon to spot their quarry.

“Discovering these two new exiled stars was neither lucky nor random,” said astronomer Margaret Geller (Smithsonian Astrophysical Observatory), a co-author on the paper. “We made a targeted search for them. By understanding their origin, we knew where to find them.”

Theory predicts that the exiled stars were thrown from the galactic center millions of years ago. Each star once was part of a binary star system. When a binary swings too close to the black hole at the galaxy’s center, the intense gravity can yank the binary apart, capturing one star while violently flinging the other outward at tremendous speed (hence their technical designation of hypervelocity stars).

The two recently discovered exiles both are short-lived stars about four times more massive than the sun. Many similar stars exist within the galactic center, supporting the theory of how exiles are created. Moreover, detailed studies of the Milky Way’s center previously found stars orbiting the black hole on very elongated, elliptical orbits – the sort of orbits that would be expected for former companions of hypervelocity stars.

“Computer models show that hypervelocity stars are naturally made near the galactic center,” said theorist Avi Loeb of the Harvard-Smithsonian Center for Astrophysics. “We know that binaries exist. We know the galactic center holds a supermassive black hole. So, exiled stars inevitably will be produced when binaries pass too close to the black hole.”

Astronomers estimate that a star is thrown from the galactic center every 100,000 years on average. Chances of seeing one at the moment of ejection are slim. Therefore, the hunt must continue to find more examples of stellar exiles in order to understand the extreme environment of the galactic center and how those extremes lead to the formation of hypervelocity stars.

The characteristics of exiled stars give clues to their origin. For example, if a large cluster of stars spiraled into the Milky Way’s central black hole, many stars might be thrown out at nearly the same time. Every known hypervelocity star left the galactic center at a different time, therefore there is no evidence for a “burst” of exiles.

Hypervelocity stars also offer a unique probe of galactic structure. “During their lifetime, these stars travel across most of the Galaxy,” said Geller. “If we could measure their motions across the sky, we could learn about the shape of the Milky Way and about the way the mysterious dark matter is distributed.”

The first newfound exile, in the direction of the constellation Ursa Major, is designated SDSS J091301.0+305120. It is traveling out of the galaxy at a speed of about 1.25 million miles per hour and currently is located at a distance of about 240,000 light-years from the earth. The second exile, in the direction of the constellation Cancer, is designated SDSS J091759.5+672238. It is moving outward at 1.43 million miles per hour and currently is located about 180,000 light-years from the earth.

Both stars, although traveling at tremendous speeds through space, are located so far from the earth that their motion cannot be detected except with sophisticated astronomical instruments.

This research has been submitted to The Astrophysical Journal Letters for publication and will be available online at http://arxiv.org/abs/astro-ph/0601580. Authors on the paper are Brown, Geller, Scott Kenyon and Michael Kurtz (Smithsonian Astrophysical Observatory).

Headquartered in Cambridge, Mass., the Harvard-Smithsonian Center for Astrophysics (CfA) is a joint collaboration between the Smithsonian Astrophysical Observatory and the Harvard College Observatory. CfA scientists, organized into six research divisions, study the origin, evolution and ultimate fate of the universe.

Original Source: CfA News Release

2005 Was the Hottest Year

2005 was the warmest year since the late 1800s. Image credit: NASA Click to enlarge
The year 2005 may have been the warmest year in a century, according to NASA scientists studying temperature data from around the world.

Climatologists at NASA’s Goddard Institute for Space Studies (GISS) in New York City noted that the highest global annual average surface temperature in more than a century was recorded in their analysis for the 2005 calendar year.

Some other research groups that study climate change rank 2005 as the second warmest year, based on comparisons through November. The primary difference among the analyses, according to the NASA scientists, is the inclusion of the Arctic in the NASA analysis. Although there are few weather stations in the Arctic, the available data indicate that 2005 was unusually warm in the Arctic.

In order to figure out whether the Earth is cooling or warming, the scientists use temperature data from weather stations on land, satellite measurements of sea surface temperature since 1982, and data from ships for earlier years.

Previously, the warmest year of the century was 1998, when a strong El Nino, a warm water event in the eastern Pacific Ocean, added warmth to global temperatures. However, what’s significant, regardless of whether 2005 is first or second warmest, is that global warmth has returned to about the level of 1998 without the help of an El Nino.

The result indicates that a strong underlying warming trend is continuing. Global warming since the middle 1970s is now about 0.6 degrees Celsius (C) or about 1 degree Fahrenheit (F). Total warming in the past century is about 0.8? C or about 1.4? F.

“The five warmest years over the last century occurred in the last eight years,” said James Hansen, director of NASA GISS. They stack up as follows: the warmest was 2005, then 1998, 2002, 2003 and 2004.

Over the past 30 years, the Earth has warmed by 0.6? C or 1.08? F. Over the past 100 years, it has warmed by 0.8? C or 1.44? F.

Current warmth seems to be occurring nearly everywhere at the same time and is largest at high latitudes in the Northern Hemisphere. Over the last 50 years, the largest annual and seasonal warmings have occurred in Alaska, Siberia and the Antarctic Peninsula. Most ocean areas have warmed. Because these areas are remote and far away from major cities, it is clear to climatologists that the warming is not due to the influence of pollution from urban areas.

Original Source: NASA News Release

Tethys and Tiny Atlas

The two moons Tethys and tiny Atlas. Image credit: NASA/JPL/SSI Click to enlarge
This view from Cassini contains not one, but two moons. Tethys is slightly overexposed so that the real target of this image, tiny Atlas, can be seen. Atlas is at image center, just outside the A ring.

A couple of faint ringlets are visible in the Encke Gap, right of center. Tethys is 1,071 kilometers (665 miles) wide; Atlas is a mere 32 kilometers (20 miles) wide.

The image was taken in visible light with the Cassini spacecraft narrow-angle camera on Dec. 21, 2005, at a distance of approximately 2 million kilometers (1.2 million miles) from Tethys and 1.7 million kilometers (1.1 million miles) from Atlas. The image scale is 12 kilometers (7 miles) per pixel on Tethys.

The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA’s Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging operations center is based at the Space Science Institute in Boulder, Colo.

For more information about the Cassini-Huygens mission visit http://saturn.jpl.nasa.gov . The Cassini imaging team homepage is at http://ciclops.org .

Original Source: NASA/JPL/SSI News Release

Life Doesn’t Change Terrain Much

The more we explore Mars, the more it looks like Earth. Image credit: NASA Click to enlarge
One of the paradoxes of recent explorations of the Martian surface is that the more we see of the planet, the more it looks like Earth, despite a very big difference: Complex life forms have existed for billions of years on Earth, while Mars never saw life bigger than a microbe, if that.

“The rounded hills, meandering stream channels, deltas and alluvial fans are all shockingly familiar,” said William E. Dietrich, professor of earth and planetary science at the University of California, Berkeley. “This caused us to ask: Can we tell from topography alone, and in the absence of the obvious influence of humans, that life pervades the Earth? Does life matter?”

In a paper published in the Jan. 26 issue of the journal Nature, Dietrich and graduate student J. Taylor Perron reported, to their surprise, no distinct signature of life in the landforms of Earth.

“Despite the profound influence of biota on erosion processes and landscape evolution, surprisingly,?there are no landforms that can exist only in the presence of life and, thus, an abiotic Earth probably would present no unfamiliar landscapes,” said Dietrich.

Instead, Dietrich and Perron propose that life – everything from the lowest plants to large grazing animals – creates a subtle effect on the land not obvious to the casual eye: more of the “beautiful, rounded hills” typical of Earth’s vegetated areas, and fewer sharp, rocky ridges.

“Rounded hills are the purest expression of life’s influence on geomorphology,” Dietrich said. “If we could walk across an Earth on which life has been eliminated, we would still see rounded hills, steep bedrock mountains, meandering rivers, etc., but their relative frequency would be different.”

When a NASA scientist acknowledged to Dietrich a few years ago that he saw nothing in the Martian landscape that didn’t have a parallel on Earth, Dietrich began thinking about what effects life does have on landforms and whether there is anything distinctive about the topography of planets with life, versus those without life.

“One of the least known things about our planet is how the atmosphere, the lithosphere and the oceans interact with life to create landforms,” said Dietrich, a geomorphologist who for more than 33 years has studied the Earth’s erosional processes. “A review of recent research in Earth history leads us to suggest that life may have strongly contributed to the development of the great glacial cycles, and even influenced the evolution of plate tectonics.”

One of the main effects of life on the landscape is erosion, he noted. Vegetation tends to protect hills from erosion: Landslides often occur in the first rains following a fire. But vegetation also speeds erosion by breaking up the rock into smaller pieces.

“Everywhere you look, biotic activity is causing sediment to move down hill, and most of that sediment is created by life,” he said. “Tree roots, gophers and wombats all dig into the soil and raise it, tearing up the underlying bedrock and turning it into rubble that tumbles downhill.”

Because the shape of the land in many locations is a balance between river erosion, which tends to cut steeply into a slope’s bedrock, and the biotically-driven spreading of soil downslope, which tends to round off the sharp edges, Dietrich and Perron thought that rounded hills would be a signature of life. This proved to be untrue, however, as their colleague Ron Amundson and graduate student Justine Owen, both of the campus’s Department of Environmental Science, Policy and Management, discovered in the lifeless Atacama Desert in Chile, where rounded hills covered with soil are produced by salt weathering from the nearby ocean.

“There are other things on Mars, such as freeze-thaw activity, that can break rock” to create the rounded hills seen in photos taken by NASA’s rovers, Perron said.

They also looked at river meanders, which on Earth are influenced by streamside vegetation. But Mars shows meanders, too, and studies on Earth have shown that rivers cut into bedrock or frozen ground can create meanders identical to those created by vegetation.

The steepness of river courses might be a signature, too, they thought: Coarser, less weathered sediment would erode into the streams, causing the river to steepen and the ridges to become higher. But this also is seen in Earth’s mountains.

“It’s not hard to argue that vegetation affects the pattern of rainfall and, recently, it has been shown that rainfall patterns affect the height, width and symmetry of mountains, but this would not produce a unique landform,” Dietrich said. “Without life, there would still be asymmetric mountains.”

Their conclusion, that the relative frequency of rounded versus angular landforms would change depending on the presence of life, won’t be testable until elevation maps of the surfaces of other planets are available at resolutions of a few meters or less. “Some of the most salient differences between landscapes with and without life are caused by processes that operate at small scales,” Perron said.

Dietrich noted that limited areas of Mars’ surface have been mapped at two-meter resolution, which is better than most maps of the Earth. He is one of the leaders of a National Science Foundation (NSF)-supported project to map in high resolution the surface of the Earth using LIDAR (LIght Detection And Ranging) technology. Dietrich co-founded the National Center of Airborne Laser Mapping (NCALM), a joint project between UC Berkeley and the University of Florida to conduct LIDAR mapping showing not only the tops of vegetation, but also the bare ground as if denuded of vegetation. The research by Dietrich and Perron was funded by NSF’s National Center for Earth-surface Dynamics, the NSF Graduate Research Fellowship Program and NASA’s Astrobiology Institute.

Original Source: UC Berkeley News Release

Icy Extrasolar Planet Discovered

An artist’s illustration shows the extrasolar planet orbiting a dim star. Image credit: NASA Click to enlarge
Using a relatively new planet-hunting technique that can spot worlds one-tenth the mass of our own, researchers have discovered a potentially rocky, icy body that may be the smallest planet yet found orbiting a star outside our solar system.

The discovery suggests the technique, gravitational microlensing, may be an exceptional technology for finding distant planets with traits that could support life.

“This is an important breakthrough in the quest to answer the question ‘Are we alone?'” said Michael Turner, assistant director for the National Science Foundation (NSF) mathematical and physical sciences directorate. “The team has discovered the most Earth-like planet yet, and more importantly, has demonstrated the power of a new technique that is sensitive to detecting habitable planets. It can probe a much greater portion of our galaxy and is complementary to other techniques.”

Located more than 20,000 light years away in the constellation Sagittarius, close to the center of our Milky Way galaxy, planet OGLE-2005-BLG-390Lb is approximately five-and-a-half times the mass of Earth.

Orbiting a star one-fifth the mass of the sun at a distance almost three times that of Earth’s orbit, the newly discovered planet is frigid: the estimated surface temperature is -364 degrees Fahrenheit (-220 degrees Celsius).

Although astronomers doubt this cold body could sustain organisms, researchers believe gravitational microlensing will bring opportunities for observing other rocky planets in the “habitable zones” of stars – regions where temperatures are perfect for maintaining liquid water and spawning life.

The discovery, authored by 73 collaborators from 32 institutions, appears in the Jan. 26 issue of the journal Nature.

OGLE (Optical Gravitational Lensing Experiment) project telescopes first observed the lensing event on July 11, 2005. In an attempt to catch microlensing events as they occur, OGLE scans most of the central Milky Way each night, discovering more than 500 microlensing events per year. But to detect the signature of low-mass planets, astronomers must observe these events much more frequently than OGLE’s one survey per night.

So, when OGLE detected the July 11 lensing, its early warning system alerted fellow astronomers across the globe to microlensing event OGLE-2005-BLG-390 (for the 390th galactic bulge OGLE discovered in 2005). At that point, though, no one knew a planet would emerge.

“The only way to realize the full scientific benefit of our observations is to share the data with our competition,” said co-author Bohdan Paczynski of Princeton University, who along with Andrzej Udalski of Warsaw University Observatory and their colleagues co-founded OGLE in 1997.

The telescopes of PLANET (Probing Lensing Anomalies NETwork) and RoboNet tracked the July 11 episode to completion, providing the data that confirmed the presence of a previously unknown planet. These telescopes collect observations more frequently in an attempt to detect the microlensing signature of planets.

“This discovery was possible because the sun never rises on the PLANET collaboration,” said lead author and PLANET researcher Jean-Philippe Beaulieu of the Institut d’Astrophysique de Paris, France. “The global nature of the PLANET collaboration was crucial for obtaining data throughout the 24-hour planetary signal,” he added.

Ironically, when preparing the final report, the researchers discovered that during its test runs, the new MOA (Microlensing Observations in Astrophysics) telescope, MOA-2, had taken additional measurements of the lensing event. The 6-foot (1.8-meter) aperture telescope has a wider field-of-view than the OGLE telescope, enabling it to observe 100 million stars many times per night. MOA-2 is one of several recent and future advancements that gravitational microlensing proponents hope will greatly increase the number of Earth-like planet discoveries.

OGLE also has plans to increase the field-of-view of its own telescope, and other microlensing groups are proposing to build a new telescope in South Africa. They have also proposed a space mission to see planets as small as Mars as well as free-floating planets that no longer orbit a host star.

“The new discovery provides a strong hint that low-mass planets may be much more common than Jupiters,” said co-author and PLANET researcher David Bennett of the University of Notre Dame. Most extrasolar planets found so far have been Jupiter-sized.

“Microlensing should have discovered dozens of Jupiters by now if they were as common as these five-Earth-mass planets. This illustrates the primary strength of the gravitational microlensing method: its ability to find planets of low-mass,” Bennett said.

Low-mass planets can yield signals that are too weak to detect with other methods. With microlensing, the signals of low-mass planets are rare but not weak. Thus, the rate of low-mass planet discoveries should increase dramatically if more microlensing events can be searched for planetary signals.

Original Source: NSF News Release

Prometheus and Dione

The Saturnian moons Prometheus and Dione. Image credit: NASA/JPL/SSI Click to enlarge
The ring moon Prometheus continues its work shaping the delicate F ring as Dione looks on. It is easy to see how Prometheus has an irregular, oblong shape, while Dione is quite round.

The rings are partly cut off by Saturn’s shadow at right. Prometheus is 102 kilometers (63 miles) wide; Dione is 1,123 kilometers (700 miles) wide.

The image was taken in visible light with the Cassini spacecraft narrow-angle camera on Dec. 20, 2005, at a distance of approximately 2.5 million kilometers (1.6 million miles) from Dione and 2.2 million kilometers (1.4 million miles) from Prometheus. The image scale is 15 kilometers (9 miles) per pixel on Dione and 13 kilometers (8 miles) per pixel on Prometheus.

The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA’s Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging operations center is based at the Space Science Institute in Boulder, Colo.

For more information about the Cassini-Huygens mission visit http://saturn.jpl.nasa.gov . The Cassini imaging team homepage is at http://ciclops.org .

NASA/JPL/SSI News Release

Opportunity Begins Its Third Year on Mars

Opportunity rover’s panorama of “Erebus Rim”. Image credit: NASA/JPL Click to enlarge
NASA’s Mars rovers, Spirit and Opportunity, have been working overtime to help scientists better understand ancient environmental conditions on the red planet. The rovers are also generating excitement about the exploration of Mars outlined in NASA’s Vision for Space Exploration.

The rovers continue to find new variations of bedrock in areas they are exploring on opposite sides of Mars. The geological information they have collected adds evidence about ancient Martian environments that included periods of wet, possibly habitable conditions.

“The extended journeys taken by the two rovers across the surface of Mars has allowed the science community to continue to uncover discoveries that will enable new investigations of the red planet far into the future.” said Mary Cleave, associate administrator for the Science Mission Directorate, NASA Headquarters.

NASA’s third mission extension for the rovers lasts through September 2006, if they remain usable that long. During their three-month primary missions, the rovers drove farther and examined more rocks than the prescribed criteria for success.

Opportunity begins its third year on Mars today. It is examining bedrock exposures along a route between “Endurance” and “Victoria” craters. Opportunity found evidence of a long-ago habitat of standing water on Mars.

On Jan. 3, Spirit passed its second anniversary inside the Connecticut-sized Gusev Crater. Initially, Spirit did not find evidence of much water, and hills that might reveal more about Gusev’s past were still mere bumps on the horizon. By operating eight times as long as planned, Spirit was able to climb up those hills, examine a wide assortment of rocks and find mineral fingerprints of ancient water.

While showing signs of wear, Spirit and Opportunity are still being used to their maximum remaining capabilities. On Spirit, the teeth of the rover’s rock abrasion tool are too worn to grind the surface off any more rocks, but its wire-bristle brush can still remove loose coatings. The tool was designed to uncover three rocks, but it exposed interiors of 15 rocks.

On Opportunity, the steering motor for the front right wheel stopped working eight months ago. A motor at the shoulder joint of the rover’s robotic arm shows symptoms of a broken wire in the motor winding. Opportunity can still maneuver with its three other steerable wheels. Its shoulder motor still works when given extra current, and the arm is still useable without that motor.

The rovers are two of five active robotic missions at Mars, which include NASA’s Mars Odyssey and Mars Global Surveyor and the European Space Agency’s Mars Express orbiters. The orbiters and surface missions complement each other in many ways. Observations by the rovers provide ground-level understanding for interpreting global observations by the orbiters. In addition to their own science missions, the orbiters relay data from Mars.

NASA’s Jet Propulsion Laboratory, Pasadena, Calif., a division of the California Institute of Technology, manages the Mars Exploration Rover, Odyssey and Global Surveyor projects for NASA’s Science Mission Directorate.

For images and information about the rovers and their discoveries on the Web, visit: http://www.nasa.gov/mars

Original Source: NASA/JPL News Release

What’s Up This Week – January 23 – January 29, 2006

What's Up 2006

Download our free “What’s Up 2006” ebook, with entries like this for every day of the year.

M1: “The Crab Nebula”. Image credit: R. Jay GaBany. Click to enlarge.
Monday, January 23 – Thanks to dark skies, tonight will be the perfect opportunity to “go crabbing” in Taurus. Although M1 was discovered by John Bevis in 1731, it became the first object on Charles Messier’s astronomical list. He rediscovered M1 while searching for the expected return of Halley’s Comet in late August 1758 and these “comet confusions” prompted Messier to start cataloging. It wasn’t until Lord Rosse gathered enough light from M1 in the mid-1840’s that the faint filamentary structure was noted (although he may not have given the Crab Nebula its name). To have a look for yourself, locate Zeta Tauri and look about a finger-width northwest. You won’t see the “Crab legs” in small scopes – but there’s much more to learn about this famous “supernova remnant” in the future.

Tuesday, January 24 – Today is the birthday of American solar astronomer Harold Babcock. Born in 1882, Babcock proposed that the sunspot cycle was a result of the Sun’s differential rotation and magnetic field in 1961. Would you like to have a look at the Sun? Although solar observing is best done with a proper filter, it is perfectly safe to use the “solar projection method.”

Before we start, NEVER look at the Sun directly with the eye or with any unfiltered optical device, such as binoculars or a telescope. We’re not joking when we say this will blind you. Exposed film, mylar, and smoked glass are also UNSAFE. But don’t be afraid, because we’re here to tell you how you can enjoy solar viewing. A safe way to observe sunspots is to “project” an image of the Sun through a telescope or binoculars onto a screen. This can be as simple as cardboard, a paper plate, a wall or whatever you have handy. If you’re using a telescope be sure the finderscope is securely capped. If you use binoculars, cover one of the two tubes. By using the shadow method to aim, you will see a bright circle of light on your makeshift screen. This is the solar disc. Adjust the focus by moving the distance of the screen from your optics until it’s about the size of a small plate. If the image is blurry, use manual focus until the edges of the disc become sharp. Even though it might take a little practice, you’ll soon become proficient at this method and be able to see a surprising amount of detail in and around sunspot areas. Happy and SAFE viewing to you!

Today in 1986, the United States Voyager 2 became the first spacecraft to fly by Uranus, providing us with the most outstanding photographs and information on the planet to date. After 10,382 days of successful operation, Voyager 2 still continues on towards the stars carrying “The Sounds of Earth.”

Speaking of stars, turn your scope on brilliant Rigel – Orion’s south-westernmost bright star. Enjoy its cool radiance and look for an 8th magnitude companion just outside the spikes of light caused by the Earth’s atmosphere.

Wednesday, January 25 – This morning before dawn, look for the Moon very near Antares. Many observers in the southern portions of Mexico, Peru and Ecudor will have the opportunity to see it occulted, so please check with the International Occultation Timing Association (IOTA) for details.

Today is the birthday of Joseph Louis Lagrange. Born in 1736, the famed French mathematician made important contributions to the field of celestial mechanics. We’re not talking “wrenches in space,” but how masses interact gravitationally to keep things orderly in the solar system and beyond. If you’re up early this morning, have a look at the lunar crater named for him. You’ll find LaGrange on the southern limb about one-quarter the distance up from the cusp. But, you won’t find the SOHO satellite there. NASA’s “eye on Sol” is parked at Lagrange point one (L1) between the Earth and Sun.

Tonight let’s journey to Orion and have a look at a pair of neighboring open clusters. Found a little less than a hand span northwest of Betelguese, NGC 1807 and NGC 1817 aren’t exactly twins. Both clusters are of similar magnitude and can be seen as faint patches in binoculars. Through a telescope, NGC 1817 appears far more populated with stars than its neighbor. Studies based on stellar motion reveal that NGC 1817 has far more stars than the brighter NGC 1807. Although the two are quite distant from one another in space, we get to see them both as close friends…

Thursday, January 26 – In keeping with our dark sky studies, tonight we’ll explore planetary nebula NGC 1514 in Taurus. Locate it by moving about two finger-width’s south-east of Zeta Perseii. Planetary nebulae were first described as “planetary” by William Herschel in 1785. Before then, all were simply considered “nebulae.” It was once thought they were made of stars, but today we know planetaries are created from material given off by a single star. Many show well-defined rings of one type or another. Others – like M1 – are irregularly shaped supernova remnants. NGC 1514’s material is slowly boiled off over time, rather than caused by a violent explosion.

It would be very hard to find the neutron central star in M1, but almost any scope can make out NGC 1514’s 10th magnitude fueling star as it quietly cooks away gases to feed its nebulous shroud. Because it is so bright, it can easily overwhelm the eye. This makes NGC 1514 similar to the famous “Blinking Planetary” – NGC 6826 – in Cygnus.

Friday, January 27 – The planet Saturn is at opposition tonight, meaning it rises as the Sun sets. Look for it late in the evening moving past M44 – “the Beehive” – cluster in Cancer. The 2006 apparition will continue to feature Saturn’s rings and the planet’s southern hemisphere.

Are you ready for more deep sky? Then let’s head off towards the galaxy NGC 1023 in Perseus. It’s a beautiful example of a slightly tilted “SB0” spiral galaxy. You won’t see any spiral arms on this one – but not because your telescope isn’t large enough. Unlike our own Milky Way, NGC 1023 really doesn’t have any. But, it does have a bright galactic hub bending like a thick lens going outward. At the center of the hub is one of the most massive black holes within a hundred million light-years. Don’t worry about being pulled in, because this galaxy is located 33 million light-years away! You’ll find it a bit closer to home about a fist-width southwest of Algol – Beta Persei.

There is a much closer supermassive black hole at the center of our own galaxy. It’s a profound gravitational anomaly causing stars to take on strange, highly elliptical orbits at very high speeds – some which have orbits taking far less time than Jupiter does to revolve around the Sun. The stars involved (“S-stars”) appear mysteriously young to astronomers. This might occur because their outer atmospheres are being stripped away by gravitational tidal forces. It’s happening in NGC 1023 as well, but that galaxy is ten times more massive than our own!

Saturday, January 28 – It’s Saturday and New Moon! Many amateurs will be out tonight “partying” beneath the darkest night sky of the month. All that’s needed is a wide-open field well away from glow from artificial lights and a variety of optical instruments – eyes, binoculars, and telescopes. The joy of observing can be multiplied many times over when shared with others!

What should you bring to a “star party?” Start with your favorite scope and a short list of things to observe including both “everybody’s favorites” and at least one “special study” that others may not have observed before! Tonight, the two “Greats” – M31 and M42 – will be on everyone’s list, but what about those “great” unknowns?

Consider NGC 1535 – a fine planetary nebula with central star in Eridanus. At magnitude 10, this 1600 light-year distant beauty has an easy 12th magnitude star providing illumination at its core. Use high power to give “image scale” to this small, subtle study. You’ll find it just about a fist’s width east-northeast of Gamma Eridani. If you find it difficult, you’d be right – but that’s why this aqua blue planetary is not more widely appreciated!

Sunday, January 29 – Today is the birthday of Johannes Hevelius. Born in 1611, Hevelius was the first to publish detailed maps of the Moon. His book, Selenographia, debuted in 1647. That’s 359 years ago – and it’s still accurate! Too bad there’s no Moon to celebrate with… Or is it?

Let’s have a look instead at the Pleiades – M45. We aren’t finished observing the Pleiades yet, because the “Seven Sisters” may not be finished either. On a moonless night, you can see the afterbirth of stellar creation – the faint sheen of nebulosity illuminated by hot stars doing their best to “light up the night.” Most easily spotted is NGC 1435 associated with Merope and NGC 1432 near Maia. To be sure you are seeing the nebulosity, look well away from both stars. From Merope (the southernmost bright star) look due south – away from the brightest stars of the cluster. Compare that to the nebulosity which surrounds all seven major stars – but especially Maia – north of Merope. Be sure not to stare directly. They will appear like a pale smear or a “fog” on your optics. Move your eyes around to activate the sensitive light-receptors in the eye – that’s using your eyes to advantage!

Until next week? May all of your journeys be at… Light Speed! ~Tammy Plotner

Contributing Writer: Jeff Barbour @ astro.geekjoy.com

Icy Epimetheus

Icy Epimetheus behind Saturn’s rings. Image credit: NASA/JPL/SSI Click to enlarge
The Cassini spacecraft captured this glimpse of icy Epimetheus just before the small moon disappeared behind the bulk of Saturn’s atmosphere.

See Looking Down on Epimetheus for a closer view of Epimetheus (116 kilometers, or 72 miles across).

The image was taken in visible light with the Cassini spacecraft narrow-angle camera on Dec. 20, 2005, at a distance of approximately 2.3 million kilometers (1.4 million miles) from Epimetheus and 2.2 million kilometers (1.4 million miles) from Saturn. The image scale is 14 kilometers (9 miles) per pixel on Epimetheus and 13 kilometers (8 miles) per pixel on Saturn.

The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA’s Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging operations center is based at the Space Science Institute in Boulder, Colo.

For more information about the Cassini-Huygens mission visit http://saturn.jpl.nasa.gov . The Cassini imaging team homepage is at http://ciclops.org .

Original Source: NASA/JPL/SSI News Release