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Mercury Surprises: Tiny Planet Has Odd Interior, Active Past | Messenger Spacecraft | S... - 0 views

  • interior unlike that of any other rocky planet in our solar system and a surprisingly dynamic history,
  • remained geologically active for a surprisingly large chunk of its evolutionary history, researchers said
  • planet's huge iron core is even larger than they had thought
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  • likely overlain with a solid shell of iron and sulfur
  • layered structure not known to exist on Earth, Venus or Mars
  • Messenger has taken nearly 100,000 images and made more than 4 million measurements of the planet's surface
  • probe is mapping Mercury's surface and gathering data on the planet's composition, magnetic environment and tenuous atmosphere, among other features
  • s original science campaign was designed to last one Earth year
  • NASA announced in November that it had granted the spacecraft a one-year mission extension
  • officially began its extended mission earlier this week.
  • In one study
  • They found that the range of elevations was smaller than that found on either Mars or the moon.
  • also observed that the floors of many Mercury craters have been tilted substantially
  • suggest that internal forces pushed the craters up after the impacts created them
  • not out of the question that Mercury is still active today
  • not very likely
  • have not observed an active eruption or extrusion
  • determined that Mercury has "mascons," large positive gravity anomalies associated with big impact basins
  • first discovered on the moon in 1968 and caused great problems in the Apollo program because they tugged low-orbiting spacecraft around and made navigation difficult
  • Subsequently mascons were discovered on Mars
  • find out that Mercury has
  • appear to be a common feature of terrestrial planetary bodies
  • gravity calculations also suggest that Mercury has an iron core that comprises roughly 85 percent of the planet's radius
  • Earth's iron core covers about half of its radius
  • new findings should help shed light on Mercury's past
  • formation and evolution of rocky planets in general
  • looks like a layer of solid iron sulfide overlies Mercury's core — a feature not known to exist on any other terrestrial planet
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Water Ice Found at Mercury's North Pole | Space.com - 0 views

  • Confirming decades of suspicion, a NASA spacecraft has spotted vast deposits of water ice on the planet closest to the sun
  • Temperatures on Mercury can reach 800 degrees Fahrenheit (427 degrees Celsius
  • around the north pole, in areas permanently shielded from the sun's heat
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  • Messenger spacecraft found a mix of frozen water and possible organic materials
  • Evidence of big pockets of ice is visible from a latitude of 85 degrees north up to the pole
  • smaller deposits scattered as far away as 65 degrees north.
  • NASA will direct Messenger's observation toward that area in the coming months — when the angle of the sun allows — to get a better look
  • Researchers also believe the south pole has ice, but Messenger's orbit has not allowed them to obtain extensive measurements of that region yet
  • Messenger will spiral closer to the planet in 2014 and 2015 as it runs out of fuel
  • Speculation about water ice on Mercury dates back more than 20 years
  • In 1991, Earth-bound astronomers fired radar signals to Mercury and received results showing there could be ice at both poles
  • reinforced by 1999 measurements using the more powerful Arecibo Observatorymicrowave beam in Puerto Rico
  • Radar pictures beamed back to New Mexico's Very Large Array showed white areas that researchers suspected was water ice.
  • The laser is weak — about the strength of a flashlight — but just powerful enough to distinguish bright icy areas from the darker, surrounding Mercury regolith
  • Messenger's neutron spectrometer spotted hydrogen, which is a large component of water ice. But the temperature profile unexpectedly showed that dark, volatile materials – consistent with climes in which organics survive – are mixing in with the ice
  • Organic materials are life's ingredients, though they do not necessarily lead to life itself
  • the presence of organics is also suspected on airless, distant worlds such as Pluto
  • suspect Mercury's water ice is coated with a 4-inch (10 centimeters) blanket of "thermally insulating material
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Mercury Passes in Front of the Sun, as Seen From Mars - Mars Science Laboratory - 0 views

  • This is the first transit of the sun by a planet observed from any planet other than Earth, and also the first imaging of Mercury from Mars
  • Mercury fills only about one-sixth of one pixel as seen from such great distance, so the darkening does not have a distinct shape, but its position follows Mercury's expected path based on orbital calculations.
  • The observations were made on June 3, 2014,
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  • the same Mastcam frames show two sunspots approximately the size of Earth. The sunspots move only at the pace of the sun's rotation, much slower than the movement of Mercury.
  • The next Mercury transit visible from Earth will be May 9, 2016.
  • Mercury and Venus transits are visible more often from Mars than from Earth
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Curiosity Captures Mercury from Mars - 0 views

  • NASA’s Curiosity rover
  • does get a chance to skygaze on occasion. And while looking at the Sun on June 3, 2014
  • the rover’s Mastcam spotted
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  • Mercury
  • across the Sun’s face
  • Silhouetted against the bright disk of the Sun, Mercury barely appears as a hazy blur in the filtered Mastcam images
  • it was moving relatively quickly during the transit, passing the darker smudges of two Earth-sized sunspots over the course of several hours.
  • It’s the first time Mercury has ever been imaged from Mars
  • the first time we’ve observed a planet transiting our Sun from another world besides our own
  • this was
  • a carefully calculated observation using the Mastcam’s right 100mm telephoto lens and neutral density filter, which is used to routinely image the Sun in order to measure the dustiness of the Martian atmosphere
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Tiny exoplanet smaller than Mercury: Smallest planet yet found outside solar system (Up... - 0 views

  • The bigger the star, the lower the frequency, or 'pitch' of its song
  • The team determined Kepler-37's mass is about 80 percent the mass of our sun
  • That's the lowest mass star astronomers have been able to measure using oscillation data for an ordinary star
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  • Those measurements also allowed the main research team to more accurately measure the three planets orbiting Kepler-37, including the tiny Kepler-37b
  • Kepler-37b is about 80% the size of Mercury and is the first exoplanet to be found that is smaller than any planet in our own Solar System
  • Kepler-37b is very likely a rocky planet with no atmosphere or water, similar to Mercury
  • "The detection of such a small planet shows for the first time that stellar systems host planets much smaller as well as much larger than anything we see in our own Solar System."
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Smallest Exoplanet Yet Discovered by 'Listening' to a Sun-like Star - 0 views

  • Scientists have discovered a new planet orbiting a Sun-like star, and the exoplanet is the smallest yet found in data from the Kepler mission
  • Kepler-37b, is smaller than Mercury, but slightly larger than Earth’s Moon
  • discovery came from a collaboration between Kepler scientists and a consortium of international researchers who employ asteroseismology
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  • measuring oscillations in the star’s brightness caused by continuous star-quakes, and turning those tiny variations in the star’s light into sounds
  • The bigger the star, the lower the frequency, or ‘pitch’ of its song
  • The measurements made by the astroseismologists allowed the Kepler research team to more accurately measure the tiny Kepler-37b
  • revealing two other planets in the same planetary system: one slightly smaller than Earth and one twice as large
  • Kepler-37b is very likely a rocky planet with no atmosphere or water, similar to Mercury
  • “The detection of such a small planet shows for the first time that stellar systems host planets much smaller as well as much larger than anything we see in our own Solar System.”
  • host star, Kepler-37, is about 210 light-years from Earth
  • All three planets orbit the star at less than the distance Mercury is to the Sun
  • Kepler-37b orbits every 13 days at less than one-third Mercury’s distance from the Sun
  • estimated surface temperature of this smoldering planet, at more than 800 degrees Fahrenheit (700 degrees Kelvin
  • hot enough to melt the zinc in a penny
  • Kepler-37c and Kepler-37d, orbit every 21 days and 40 days, respectively
  • The size of the star must be known in order to measure the planet’s size accurately
  • scientists examined sound waves generated by the boiling motion beneath the surface of the star
  • The technique for stellar seismology is analogous to how geologists use seismic waves generated by earthquakes to probe the interior structure of Earth
  • sound waves travel into the star and bring information back up to the surface
  • waves cause oscillations that Kepler observes as a rapid flickering of the star’s brightness
  • barely discernible, high-frequency oscillations in the brightness of small stars are the most difficult to measure
  • why most objects previously subjected to asteroseismic analysis are larger than the Sun
  • Kepler-37 has a radius just three-quarters of the Sun
  • the radius of the star is known to 3 percent accuracy, which translates to exceptional accuracy in the planet’s size.
  • this discovery took a long time to verify, as the signature of this very small exoplanet was hard to confirm
  • Kepler is sending astronomers photometry data that’s “probably the best we’ll see in our lifetimes
  • uncovered a planet smaller than any in our solar system orbiting one of the few stars that is both bright and quiet, where signal detection was possible
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NASA - 2004 and 2012 Transits of Venus - 0 views

  • Transits of Venus across the disk of the Sun are among the rarest of planetary alignments
  • only six such events have occurred since the invention of the telescope (1631, 1639, 1761, 1769, 1874 and 1882
  • event begins with contact I which is the instant when the planet's disk is externally tangent with the Sun. The entire disk of the Venus is first seen at contact II when the planet is internally tangent with the Sun. During the next several hours, Venus gradually traverses the solar disk at a relative angular rate of approximately 4 arc-min/hr. At contact III, the planet reaches the opposite limb and is once again internally tangent with the Sun. The transit ends at contact IV when the planet's limb is externally tangent to the Sun
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  • Geographic Visibility of 2012 June 06
  • The entire transit (all four contacts) is visible from northwestern North America, Hawaii, the western Pacific, northern Asia, Japan, Korea, eastern China, Philippines, eastern Australia, and New Zealand.
  • Sun sets while the transit is still in progress from most of North America, the Caribbean, and northwest South America
  • transit is already in progress at sunrise for observers in central Asia, the Middle East, Europe, and eastern Africa
  • No portion of the transit will be visible from Portugal or southern Spain, western Africa, and the southeastern 2/3 of South America.
  • due to the International Date Line the Western Hemisphere will see the transit on June 5.
  • Transits of Venus are only possible during early December and early June when Venus's orbital nodes pass across the Sun
  • Transits show a clear pattern of recurrence at intervals of 8, 121.5, 8 and 105.5 years
  • next pair of Venus transits occur over a century from now on 2117 Dec 11 and 2125 Dec 08.
  • Edmund Halley first realized that transits of Venus could be used to measure the Sun's distance
  • establishing the absolute scale of the solar system from Kepler's third law
  • his method proved impractical since contact timings of the desired accuracy are impossible due to the effects of atmospheric seeing and diffraction
  • the 1761 and 1769 expeditions to observe the transits of Venus gave astronomers their first good value for the Sun's distance.
  • Mercury can also transit the Sun
  • undergoes transits much more frequently. There are about 13 or 14 transits of Mercury each century
  • Mercury transits fall within several days of 8 May and 10 November
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April 9 - Today in Science History - Scientists born on April 9th, died, and events - 0 views

  • First astronauts selected
  • In 1959, NASA announced the selection of America's first seven astronauts for project Mercury. Scott Carpenter, Gordon Cooper, John Glenn, Gus Grissom, Wally Schirra, Alan Shepard and Donald Slayton were chosen from 110 applicants. Their training program at Langley, which ranged from a graduate-level course in introductory space science to simulator training and scuba-diving. Project Mercury, NASA's first high profile program, was an effort to learn if humans could survive in space. NASA required astronaut candidates to be male, not over 40 years old, not more than 5' 11" height and in excellent physical condition. On 5 May 1961, Shepard became the first American in space
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Odd Alien Planets So Close Together They See 'Planetrise' | Kepler Mission | Space.com - 0 views

  • Astronomers have discovered two alien planets around the same star whose orbits come so close together that each rises in the night sky of its sister world
  • ,200 light-years from Earth
  • differ greatly in size and composition but come within just 1.2 million miles (1.9 million kilometers) of each other, closer than any other pair of planets known,
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  • Kepler-36b, appears to be a rocky "super-Earth" 4.5 times as massive as our planet
  • Kepler-36c, is a gaseous, Neptune-size world about eight times as massive as Earth
  • planets meet up every 97 days in a conjunction that would make each dramatically visible in the other's sky.
  • At their closest approach, the two planets are separated by five times the distance between the Earth and the moon
  • as different in density as Earth and Saturn
  • Kepler-36b and c are actually more like 20 times closer together than any two planets in our neck of the woods
  • Kepler-36c, which is about 3.7 times wider than Earth, likely has a rocky core surrounded by a substantial atmosphere filled with lots of hydrogen and helium
  • Kepler-36b, on the other hand, is a super-Earth just 1.5 times wider than our planet. Iron likely constitutes about 30 percent of its mass, water around 15 percent and atmospheric hydrogen and helium less than 1 percent
  • Kepler-36c orbits once every 16 days, at an average distance of 12 million miles (19 million km). Kepler-36b orbits each 14 days and sits about 11 million miles (18 million km) from the star.
  • Kepler-36b probably formed relatively close to the star
  • Kepler-36c likely took shape farther out
  • large-scale migrations that can bring initially far-flung planets much closer together
  • Kepler-36b probably sporting lava flows on its surface
  • orbit roughly three times closer to their host star, known as Kepler-36a, than the hellishly hot planet Mercury does to our sun
  • Kepler-36a is likely a bit hotter than our star
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Battered Asteroid Lutetia a Rare Relic of Earth's Birth | Asteroids & Comets | Earth Fo... - 0 views

  • The oddball asteroid Lutetia is a rocky remnant of the material that formed Earth, Venus and Mercury about 4.5 billion years ago, a new study suggests
  • Its composition suggests it likely formed close to the sun in the same cloud of material that eventually coalesced into the inner solar system's rocky planets.
  • then it was booted out to its current location in the main asteroid belt between Mars and Jupiter, most likely after a run-in with a young planet
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  • Lutetia, which is about 62 miles (100 kilometers) across
  • Lutetia's spectrum matched that of one particular class of meteorite called enstatite chondrites, which are known to date from the early solar system
  • Enstatite chondrites are thought to have formed close to the sun and to have served as building blocks for the rocky planets, especially Earth, Venus and Mercury, researchers said.
  • The implication is that Lutetia also originated close to the sun, not out in the main asteroid belt where it currently sits
  • Lutetia's birthplace makes the space rock pretty special. Astronomers have estimated that just 2 percent of the bodies that formed where it likely did ended up in the main asteroid belt.
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Two Powerful Coronal Mass Ejections (Hey Mercury, down in front!) [hd video] | Flickr -... - 0 views

  • Nov. 12-14, 2011
  • The first event is a halo CME event in that the leading edge of the particle cloud expanded in an arc around the Sun
  • In the second, larger event the bright cloud is heading out into space and away from Earth
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  • The bright object moving into the field of view in the lower right is Mercury
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MESSENGER: MErcury Surface, Space ENvironment, GEochemistry, and Ranging - 0 views

  • , a portion of the terrain surrounding the northern margin of the Caloris basin
  • an elevated block in the shape of a certain carbonite-encased smuggler who can make the Kessel Run in less than twelve parsecs
  • This block may be part of the original surface that pre-dates the formation of Caloris, which was shaped by material ejected during the basin-forming event
Mars Base

May 5 - Today in Science History - Scientists born on May 5th, died, and events - 0 views

  • In 2000, a conjunction of the five bright planets - Mercury, Venus, Mars, Jupiter and Saturn - formed a rough line across the sky with the Sun and Moon. Unfortunately, nothing was visible from the earth, because the the line of planets was behind the Sun and hidden in its brilliance. Such a conjunction last happened in Feb 1962 and will not happen again until Apr 2438. Throughout former history, a conjuction event was regarded with foreboding. However, now science can be dismissive. Donald Olson, an expert on tides at Southwest Texas State University, working with the assistance of a graduate student, Thomas Lytle, calculated the stress on the Earth caused by the Moon and eight planets has often been routinely greater, most recently on 6 Jan 1990
  • Conjunction of the planets
  • First U.S. space flight
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  • In 1961, America's first astronaut in space, Alan Bartlett Shepherd, Jr., made a 15 minute sub-orbital flight that reached an altitude of 115 miles, during which he experienced about five minutes of "weightlessness." He was launched in the 2,000-lb. capsule Freedom 7 from Cape Canaveral, Florida, by a Mercury-Redstone 3 rocket. The flight travelled 302 miles at a speed relative to the ground of of 4,500 mph. Although Shepard thus became the first American in space, the world's first human in space flight was Yuri Gagarin, a Russian cosmonaut, launched into orbit less than one month earlier, on 12 Apr 1961.
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This Week's Sky at a Glance, May 23 - 31 | Sky & Telescope - 0 views

  • Wednesday, May 28
  • New Moon
  • (exact at 2:40 p.m. EDT)
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  • Friday, May 30
  • very low in the west-northwest in twilight for the hairline crescent Moon with Mercury to its right. They're far to the lower right of bright Jupiter
  • Saturday, May 31
  • The Moon, Jupiter, and Pollux above them form a nearly straight line in twilight as seen from North America
  • Mercury
  • highest evening apparition of 2014 for skywatchers at mid-northern latitudes,
  • fades this week
  • twilight deepens, look for it in the west-northwest to the lower right of bright Jupiter
  • Venus
  • "Morning Star" low due east during dawn
  • Mars (
  • ighest in the south in late twilight
  • Mars sets in the west around 3 or 4 a.m. daylight saving time
  • Jupiter
  • in the west in twilight
  • sinks during the evening and sets around 11 or midnight.
  • Jupiter is on the far side of the Sun from us
  • nearly its minimum apparent size.
  • Saturn
  • is two weeks past 10th opposition.
  • in the southeast during evening and stands highest in the south around 11 or midnight.
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NASA Moon Probes' Impact Craters Spotted from Space | Grail Mission | Space.com - 0 views

  • NASA's Lunar Reconnaissance Orbiter (LRO) snapped a series of photographs of the two 16.5-foot-wide (5 meters) craters, which mark where the space agency's twin Grail probes ended their gravity-mapping mission, and their operational lives, on Dec. 17.
  • It's a bit of a surprise that the LROC team was able to find the craters at all
  • the craters are small, nondescript features on a body riddled with impact scars
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  • The two Grail spacecraft — known as Ebb and Flow — slammed into a mountain near the lunar north pole at 3,771 mph (6,070 km/h), striking the surface about 20 seconds apart.
  • The Grail craters first showed up in LROC photos from January, but images taken on Feb. 28 show them in much greater detail
  • used these later photos to produce a topographic map of the impact zone
  • This map revealed that the two craters are separated by about 7,250 feet (2,210 m) in straight-line distance and 985 feet (300 m) in altitude
  • the crashes ejected material that appears darker than the surrounding lunar dirt.
  • these may be dark due to spacecraft material being mixed with the ejecta
  • may be residual fuel left in the probes' lines, or bits of their carbon-fiber bodies
  • LRO didn't get any images of the actual crashes, which occurred in the dark.
  • ultraviolet imaging spectrograph did see emissions from mercury and atomic hydrogen in the ejected plumes when they rose high enough to reach sunlight
  • The analysis of the Grail impact plumes is ongoing
  • The probes' measurements have allowed scientists to create the best-ever gravity map of any celestial body
  • And that map is getting better all the time, as researchers continue to analyze the data
  • The twin probes, which were each about the size of a washing machine, zipped around the moon at an average altitude of just 7 miles (11 km) in their final days
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