Archive for solar system

Lynch: All planets in our solar system visible except Mars

There are five fellow planets in our solar system that we can see with the naked eye, and in May we can see all of them except Mars.

The red planet is just coming out from behind the sun in our sky and is still lost in the glow of morning twilight. Next spring, though, Mars will definitely be out of hiding and put on a great show, as it’ll will be as close to Earth as it’s been in a couple of years.

This month in our Wichita Falls skies, the first planet to check out is Saturn, for a couple of reasons. First, it’s still nearly at its closest approach to Earth for 2013, about 825 million miles away. That’s a long way off, but that’s OK because Saturn’s a giant planet, second only to Jupiter in girth. Not only that, it has a fabulous ring system that spans well over 130,000 miles in diameter, making it a very enticing telescope target even if you have just a small scope.

Get out that scope out and check out Saturn, because if you do it right, you’ll love, love, love what you see. Make sure before you use it to let your scope and all the eyepieces sit outside for a good half-hour to acclimate to outside temperature. When you’re gazing at Saturn with your cooled-off scope, make sure to take long continuous views so you can get use to the light level coming into your scope. It does make a difference. You should be able to see the ring system and the actual planet with gap between the two. You may also see a few tiny starlike objects huddle close to Saturn. Those are some of its brighter moons.

Saturn is so easy to find right in the evening southeastern sky. As soon as it’s dark enough, look southeast for the brightest star you can see. That’ll be Arcturus. About halfway from Arcturus to the horizon will be two stars almost as bright as Arcturus arranged diagonally. The star on the upper right is Spica, and the “star” on the lower left is Saturn. This week you can also use the nearly full moon to find Saturn. On Tuesday night the moon will be just to the upper right of Spica, and Wednesday night the moon will be parked just to the lower right of the ringed wonder of our solar system.

Like all planets, Saturn slowly migrates around the sun in its orbit, and as it does it also journeys among the backdrop of stars in what’s called the zodiac band. All the planets in our solar system orbit the sun in more or less the same plane. That’s really apparent in the spectacle of the great planetary traffic jam this week and next in the low west-northwest sky. All winter long the bright planet Jupiter has been regaling us among the great winter constellations, but it’s about to slip off the celestial stage, not to be seen in our evening skies again until late next fall. Our Earth in its orbit around the sun is turning away from that part of space. It’ll be quite a send-off for Jupiter, though, as it’s temporarily joined by two other planets, Venus and Mercury in a very tight conjunction, or what I call a very close celestial hug that you don’t want to miss!

All this is going to take place in the very low west-northwest sky just a little bit above the horizon. You’ll need to have a really clear view in that direction with a little or no tree line. There’s also a narrow window time to see it.

Start looking for the three planets in lowest west-northwest about 45 minutes after sunset in the later stages of evening twilight. Don’t look too much later, because this planet trio will slip below the horizon by around 10 p.m. All three should be visible to the naked eye even if where you’re looking from has a lot of light pollution.

Early this week the three planets will be lined up diagonally. Venus will be the brightest one and the first one to pop out in the pink glow of twilight. Jupiter will be second-brightest just to the upper left of Venus, and Mercury will least brilliant just the lower right of Venus barely above the horizon.

Through the rest of this week, because of the combined effect of their orbits around the sun and our Earth’s orbit, the planets will be dancing among each other.

It’ll be fun to watch the alignment change from night to night, and it’s great to do with kids. By the end of this week they’ll be arranged in a nearly perfect little triangle. If you hold out your thumb at arm’s length, you should be pretty much able to cover up all three planets. You can’t do that very often!

Next week the triangular pattern will break up, but all three planets will still be a tight little group.

When you’re taking in this show remember that while these planets are really close together in the sky, they are nowhere near each other physically. They just happen to be nearly in the same line of sight from our Earthly perch. Mercury is the closest at about 106 million miles away from Earth. Venus is more than 150 million miles distant, and Jupiter’s the farthest at well over 560 million miles.

Jupiter’s also by far the biggest of the gang, at 88,000 miles in diameter. Venus is a little over 7,500 miles in girth, and Mercury’s just a little over 3,000 miles. I wouldn’t bother spending much time looking at these three with your telescope, because all three will really appear fuzzy as they’re so close to the horizon where you have to look through the maximum amount of Earth’s blurring atmosphere. Just enjoy the best planet show of 2013 with the naked eye. Don’t miss it!

Mike Lynch is an amateur astronomer and professional broadcast meteorologist for WCCO Radio in Minneapolis/Paul and is author of the book “Stars, a Month by Month Tour of the Constellations,” published by Adventure Publications, available at bookstores at http://www.adventurepublica tions.net.

Article source: http://www.timesrecordnews.com/news/2013/may/20/all-planets-in-our-solar-system-visible-except/

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Astronomy Nights: Cassini: Mission to Saturn, the Jewel of the Solar System

Friday, May 17, 7:30 pm — Astronomy Nights: Cassini: Mission to Saturn, the Jewel of the Solar System — Head to the Observatory to explore the night sky, planets, stars, and more. Start by enjoying a presentation on Cassini and its mission to Saturn, followed by a visit to view the night sky through the Observatory’s 22-inch research telescope. The presentation portion of the program will be held rain or shine. Please note viewing hours are weather permitting. This program is suitable for ages 5 and over. Members: Free | Non-Members: Adults $3, Children (5–17) $2.

Location: Behind the Heckscher Farm, enter from Scofieldtown Road. GPS users enter – 151 Scofieldtown Road.

cost

Article source: http://www.thehour.com/calendar/astronomy-nights-cassini-mission-to-saturn-the-jewel-of-the/event_f00de8bc-b757-11e2-a33f-0019bb30f31a.html

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Spacecraft will visit asteroid with new name

OSIRIS-REx spacecraft and asteroid BennuAn asteroid that will be explored by a NASA spacecraft has a new name, thanks to a third-grade student in North Carolina.

NASA’s Origins-Spectral Interpretation-Resource Identification-Security-Regolith Explorer (OSIRIS-REx) spacecraft will visit the asteroid now called Bennu, named after an important ancient Egyptian avian deity. OSIRIS-REx is scheduled to launch in 2016, rendezvous with Bennu in 2018, and return a sample of the asteroid to Earth in 2023.

The name for the carbon-rich asteroid, designated in the scientific community as (101955) 1999 RQ36, is the winning entry in an international student contest. Nine-year-old Michael Puzio suggested the name because he imagined the Touch-and-Go Sample Mechanism (TAGSAM) arm and solar panels on OSIRIS-REx look like the neck and wings in drawings of Bennu, which Egyptians usually depicted as a gray heron. Puzio wrote that the name suits the asteroid because it means “the ascending one,” or “to shine.”

TAGSAM will collect a sample from Bennu and store it for return to Earth. The sample could hold clues to the origin of the solar system and the source of water and organic molecules that may have contributed to the development of life on Earth. The mission will be a vital part of NASA’s plans to find, study, capture, and relocate an asteroid for exploration by astronauts. NASA recently announced an asteroid initiative proposing a strategy to leverage human and robotic activities for the first human mission to an asteroid while also accelerating efforts to improve detection and characterization of asteroids.

“There were many excellent entries that would be fitting names and provide us an opportunity to educate the world about the exciting nature of our mission,” said Dante Lauretta of the University of Arizona in Tucson. “The information about the composition of Bennu and the nature of its orbit will enable us to explore our past and better understand our future.”

More than 8,000 students, all younger than 18, from more than 25 countries entered the “Name that Asteroid!” contest last year. Each contestant submitted one name with a maximum of 16 characters and a short explanation for the name.

The contest was a partnership with The Planetary Society in Pasadena, California; the Massachusetts Institute of Technology Lincoln Laboratory in Lexington, Massachusetts; and the University of Arizona. The partners assembled a panel to review the submissions and submit a top choice to the International Astronomical Union (IAU) Committee for Small Body Nomenclature. The IAU is the governing body that officially names a celestial object.

“Bennu struck a chord with many of us right away,” said Bruce Betts from The Planetary Society. “While there were many great entries, the similarity between the image of the heron and the TAGSAM arm of OSIRIS-REx was a clever choice. The parallel with asteroids as both bringers of life and as destructive forces in the solar system also created a great opportunity to teach.”

The Lincoln Near Earth Asteroid Research Program survey team discovered the asteroid in 1999, early in NASA’s Near-Earth Objects Observation Program, which detects and catalogs near-Earth asteroids and comets.

“The samples of Bennu returned by OSIRIS-REx will allow scientists to peer into the origin of the solar system and gain insights into the origin of life,” said Jason Dworkin, from NASA’s Goddard Space Flight Center in Greenbelt, Maryland.

Article source: http://www.astronomy.com/~/link.aspx?_id=d63cb200-2a61-4090-8671-fe768a9030ec

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Astronomy for the family Sunday at Eptek

SUMMERSIDE – Is life in the solar system more common than generally thought? Join members of the Athena Community Astronomy Club to learn about new discoveries.

On Sunday evening, May 5, at 7:30, local astronomy club members will offer a presentation called “Following the Water.”

Ron Perry, one of the presenters, says, “Scientists are looking for water on other planets and finding some surprising results.”

The one-hour presentation will share some of the amazing findings that new technology has turned up when investigating planets around other stars.

Maybe guests could be in for a view of the comet of the century. This illustrated talk will be held in the main gallery at Eptek Centre.

Following the presentation, members of the Athena club will have telescopes set up outside so everyone can have a look at the stars and planets.

Perry confirmed, “Both the ringed planet, Saturn, and the largest planet, Jupiter, are visible in the evening sky. If skies are clear, we’ll look at these marvelous objects through a telescope.”

Families and the general public are invited to attend. Call 888-8373 for more details.

 

Article source: http://www.journalpioneer.com/News/Local/2013-05-02/article-3232487/Astronomy-for-the-family-Sunday-at-Eptek/1

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How Mars and Jupiter Formed from Space Rock Crashes




Interior of Mars Artist Rendition


An artist rendition of the interior of Mars. A new study suggests Mars formed from the collision of smaller space rocks than those that created the rocky core of Jupiter. Image added April 30, 2013.
CREDIT: NASA/JPL-Caltech


The violent space rock collisions that gave birth to Mars appear to be surprisingly different from those thought to form the rocky core of Jupiter, scientists say.

The difference comes from variations in the disc of dust, ice and other particles that swirled around the sun in the early years of the solar system.

Researchers said there was a “gradient” in the size of planetesimals — an early stage of planet formation — that orbited the young sun. Planets that were further away from the sun were more likely to grow larger than worlds closer in, they added. [Take a Photo Tour of the Planets]

“This difference can be explained by the snow line,” said Hiroshi Kobayashi, a researcher at Nagoya University in Japan, referring to the zone in the solar system where it was cold enough for icy compounds to condense 4.5 billion years ago.

“If we consider terrestrial planets, this is close to the sun, this means the temperature was very high, and the main component of the solid was rock, or something like that,” Kobayashi added. “But if we consider the outer disc — in this case, the main component is ice — it probably was ice planetesimals [that formed Jupiter].”

Growing up through crashing together

The solar system came into existence about 4.5 billion years ago, according to today’s theories. The sun formed in the center of a swirling disc of debris. As particles and heat streamed out from the young sun, most of the ice and gas in the inner solar system dissipated, leaving small rocky bodies behind.

Kobayashi and his co-author Nicolas Dauphas, a researcher at the Origins Lab at the University of Chicago, ran computer simulations to see how Mars formed under these conditions.

Mars orbits roughly 1.5 astronomical units (AU), or Earth-sun distances, from the sun today. The model divided the planetesimals that formed Mars into four rings, or annuli, that were 1.5, 1.8, 2.2 and 2.7 AUs from the sun, treating the millions of bodies as larger “mass batches” to simplify the calculation.

Next, the researchers followed the evolution of Mars by watching how the planetesimals crashed into one another over time. The collisions varied depending on a few factors: how much gas surrounded Mars, the variability of the bodies’ orbits, and the orbits’ inclination to the rest of the relatively flat plane of the solar system.

The process is somewhat chaotic, according to the model. The smaller planetesimals can easily lose a significant chunk of their mass when crashing into one another, thus creating even smaller bodies after colliding, the researchers noted.

Some of these pieces stick on to the larger body, while others move away, depending on how they interact with gas in the area.

This means that unlike Mars, which has a core just one-tenth the size of the Earth’s, the timescale for creating Jupiter’s massive core — which is nearly 10 times the size of Earth’s — would be quite lengthy, especially when small planetesimal collisions are considered, Kobayashi said.

“For large planetesimals, fragment accretion is less important,” he added. “The growth timescale is too long to produce Jupiter’s core within the gas lifetime.”

‘Tens of Mars-size embryos’

The scientists determined that the planetesimals that formed Mars likely collectively formed in annuli of a hundredth of the mass of the sun. Each of the individual planetesimals had a radius of less than 6.21 miles (10 kilometers).

The smashing and growing process likely produced “tens of Mars-size embryos” swarming between 0.4 AU and 1.5 AU from the sun.

Mars itself, which was orbiting 1 AU from the sun, was probably “scattered” to a distance of about 1.5 AU, Kobayashi said, possibly because Jupiter’s gravity altered the orbit of Mars. The planet shifted orbits due to a resonance with Saturn after the giants formed, according to some theories.

Kobayashi cautioned, however, that the theory of Jupiter moving is still very new and requires further study.

The remaining planetesimals would have had highly eccentric orbits, so they planetesimals could have crashed into other solar-system fragments. Kobayashi’s model said it was likely these were blown apart over time.

The research will appear in the July issue of Icarus.

Follow Elizabeth Howell @howellspace, or SPACE.com @Spacedotcom. We’re also on Facebook and Google+. Original article on SPACE.com.

Article source: http://www.space.com/20900-mars-jupiter-space-rocks-formation.html

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NASA’s Cassini spacecraft observes meteoroids colliding with Saturn’s rings

Meteoroid impacts on Saturn's ringsNASA’s Cassini spacecraft has provided the first direct evidence of small meteoroids breaking into streams of rubble and crashing into Saturn’s rings.

These observations make Saturn’s rings the only location besides Earth, the Moon, and Jupiter where scientists and amateur astronomers have been able to observe impacts as they occur. Studying the impact rate of meteoroids from outside the saturnian system helps scientists understand how different planet systems in our solar system formed.

The solar system is full of small, speeding objects. These objects frequently pummel planetary bodies. The meteoroids at Saturn are estimated to range from about a half inch to several yards (1 centimeter to several meters) in size. It took scientists years to distinguish tracks left by nine meteoroids in 2005, 2009, and 2012.

Results from Cassini already have shown Saturn’s rings act as very effective detectors of many kinds of surrounding phenomena, including the interior structure of the planet and the orbits of its moons. For example, a subtle but extensive corrugation that ripples 12,000 miles (19,000 kilometers) across the innermost rings tells of a very large meteoroid impact in 1983.

“These new results imply the current-day impact rates for small particles at Saturn are about the same as those at Earth — two very different neighborhoods in our solar system — and this is exciting to see,” said Linda Spilker, Cassini project scientist at NASA’s Jet Propulsion Laboratory in Pasadena, California. “It took Saturn’s rings acting like a giant meteoroid detector — 100 times the surface area of the Earth — and Cassini’s long-term tour of the Saturn system to address this question.”

The saturnian equinox in summer 2009 was an especially good time to see the debris left by meteoroid impacts. The very shallow sun angle on the rings caused the clouds of debris to look bright against the darkened rings in pictures from Cassini’s imaging science subsystem.

“We knew these little impacts were constantly occurring, but we didn’t know how big or how frequent they might be, and we didn’t necessarily expect them to take the form of spectacular shearing clouds,” said Matt Tiscareno, a Cassini participating scientist at Cornell University in Ithaca, New York. “The sunlight shining edge-on to the rings at the saturnian equinox acted like an anti-cloaking device, so these usually invisible features became plain to see.”

Tiscareno and his colleagues now think meteoroids of this size probably break up on a first encounter with the rings, creating smaller, slower pieces that then enter into orbit around Saturn. The impact into the rings of these secondary meteoroid bits kicks up the clouds. The tiny particles forming these clouds have a range of orbital speeds around Saturn. The clouds they form soon are pulled into diagonal, extended bright streaks.

“Saturn’s rings are unusually bright and clean, leading some to suggest that the rings are actually much younger than Saturn,” said Jeff Cuzzi, a Cassini interdisciplinary scientist specializing in planetary rings and dust at NASA’s Ames Research Center in Moffett Field, California. “To assess this dramatic claim, we must know more about the rate at which outside material is bombarding the rings. This latest analysis helps fill in that story with detection of impactors of a size that we weren’t previously able to detect directly.”

Article source: http://www.astronomy.com/~/link.aspx?_id=2fc2587b-9463-4056-bc61-5bee76b6b157

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NASA Probe Observes Meteors Colliding With Saturn’s Rings

RELEASE
:
13-120

NASA Probe Observes Meteors Colliding With Saturn’s Rings

WASHINGTON — NASA’s Cassini spacecraft has provided the first direct evidence of small meteoroids breaking into streams of rubble and crashing into Saturn’s rings.

These observations make Saturn’s rings the only location besides Earth, the moon, and Jupiter where scientists and amateur astronomers have been able to observe impacts as they occur. Studying the impact rate of meteoroids from outside the Saturn system helps scientists understand how different planet systems in the solar system formed.

Our solar system is full of small, speeding objects. Planetary bodies frequently are pummeled by them. The meteoroids at Saturn range from about one-half inch to several yards (1 centimeter to several meters) in size. It took scientists years to distinguish tracks left by nine meteoroids in 2005, 2009 and 2012.

Details of the observations appear in a paper in the Thursday edition of Science.

Results from Cassini already have shown Saturn’s rings act as very effective detectors of many kinds of surrounding phenomena, including the interior structure of the planet and the orbits of its moons. For example, a subtle but extensive corrugation that ripples 12,000 miles (19,000 kilometers) across the innermost rings tells of a very large meteoroid impact in 1983.

“These new results imply the current-day impact rates for small particles at Saturn are about the same as those at Earth– two very different neighborhoods in our solar system, and this is exciting to see,” said Linda Spilker, Cassini project scientist at NASA’s Jet Propulsion Laboratory (JPL) in Pasadena, Calif. “It took Saturn’s rings acting like a giant meteoroid detector — 100 times the surface area of the Earth — and Cassini’s long-term tour of the Saturn system to address this question.”

The Saturnian equinox in summer 2009 was an especially good time to see the debris left by meteoroid impacts. The very shallow sun angle on the rings caused the clouds of debris to look bright against the darkened rings in pictures from Cassini’s imaging science subsystem.

“We knew these little impacts were constantly occurring, but we didn’t know how big or how frequent they might be, and we didn’t necessarily expect them to take the form of spectacular shearing clouds,” said Matt Tiscareno, lead author of the paper and a Cassini participating scientist at Cornell University in Ithaca, N.Y. “The sunlight shining edge-on to the rings at the Saturnian equinox acted like an anti-cloaking device, so these usually invisible features became plain to see.”

Tiscareno and his colleagues now think meteoroids of this size probably break up on a first encounter with the rings, creating smaller, slower pieces that then enter into orbit around Saturn. The impact into the rings of these secondary meteoroid bits kicks up the clouds. The tiny particles forming these clouds have a range of orbital speeds around Saturn. The clouds they form soon are pulled into diagonal, extended bright streaks.

“Saturn’s rings are unusually bright and clean, leading some to suggest that the rings are actually much younger than Saturn,” said Jeff Cuzzi, a co-author of the paper and a Cassini interdisciplinary scientist specializing in planetary rings and dust at NASA’s Ames Research Center in Moffett Field, Calif. “To assess this dramatic claim, we must know more about the rate at which outside material is bombarding the rings. This latest analysis helps fill in that story with detection of impactors of a size that we weren’t previously able to detect directly.”

The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. JPL manages the Cassini-Huygens mission for NASA’s Science Mission Directorate in Washington. JPL designed, developed and assembled the Cassini orbiter and its two onboard cameras. The imaging team consists of scientists from the United States, England, France and Germany. The imaging operations center is based at the Space Science Institute in Boulder, Colo.

For images of the impacts and information about Cassini, visit:

http://www.nasa.gov/cassini

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Article source: http://www.nasa.gov/home/hqnews/2013/apr/HQ_13-120_Saturn_Meteors.html

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A Trip Around Mars with Kevin Fong – Part One

The planet Mars boasts the most dramatic landscapes in our solar system. Kevin Fong embarks on a grand tour around the planet with scientists, artists and writers who know its special places intimately- through their probes, roving robots and imaginations. This first part of the journey includes Mars’ gargantuan volcanoes, an extreme version of Earth’s Grand Canyon and the cratered Southern Highlands where future explorers might find safety from the Red Planet’s deadly radiation environment.

Producer: Andrew Luck-Baker

Article source: http://www.bbc.co.uk/programmes/p0175w4h

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Discovery – A Trip Around Mars with Kevin Fong – Part One

The planet Mars boasts the most dramatic landscapes in our solar system. Kevin Fong embarks on a grand tour around the planet with scientists, artists and writers who know its special places intimately- through their probes, roving robots and imaginations. This first part of the journey includes Mars’ gargantuan volcanoes, an extreme version of Earth’s Grand Canyon and the cratered Southern Highlands where future explorers might find safety from the Red Planet’s deadly radiation environment.

Producer: Andrew Luck-Baker

Article source: http://www.bbc.co.uk/iplayer/episode/p0175w4h/Discovery_A_Trip_Around_Mars_with_Kevin_Fong_Part_One/

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Discovery – A Trip Around Mars with Kevin Fong 1/2

The planet Mars boasts the most dramatic landscapes in our solar system. Kevin Fong embarks on a grand tour around the planet with scientists, artists and writers who know its special places intimately- through their probes, roving robots and imaginations. This first part of the journey includes Mars’ gargantuan volcanoes, an extreme version of Earth’s Grand Canyon and the cratered Southern Highlands where future explorers might find safety from the Red Planet’s deadly radiation environment.

Article source: http://www.bbc.co.uk/iplayer/episode/p0175w4h/Discovery_A_Trip_Around_Mars_with_Kevin_Fong_1_2/

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