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"content": "\u003cp>\u003cspan class=\"left\">\u003cimg src=\"http://ww2.kqed.org/quest/wp-content/uploads/sites/39/2011/04/f_304_211_171_1024s.jpg\">\u003cem>Extreme ultraviolet composite solar image from NASA's SDO. \u003cbr>Credit: NASA/SDO\u003c/em>\u003c/span>\u003c/p>\n\u003cp>\"If that was a scoop of ice cream, what kind would it be?\" I asked the 7-year-old girl visiting our 20-inch telescope's dome.\u003c/p>\n\u003cp>A pensive look crosses her face, as if she were standing at the counter of an ice cream parlor looking at the list of flavors. \"Mint chocolate chip,\" she decides. \u003c/p>\n\u003cp>The girl was looking at a new video display recently installed in the observatory at \u003ca href=\"http://www.chabotspace.org/index.htm\">Chabot Space & Science Center\u003c/a>, which shows up-to-the hour, time-compressed movies made from the spectacular solar imagery coming out of NASA's \u003ca href=\"http://sdo.gsfc.nasa.gov/\">Solar Dynamics Observatory \u003c/a>(SDO). \u003c/p>\n\u003cp>\u003c!--more-->\u003c/p>\n\u003cp>[ad fullwidth]\u003c/p>\n\u003cp>And it really does resemble a big, luminous, writhing ball of colorful ice cream (though what \"writhing ice cream\" is, I'm not certain; use your imagination).\u003c/p>\n\u003cp>Kept up-to-date by an Internet feed from Lockheed's \u003ca href=\"http://www.lmsal.com/\">Solar and Astrophysics Lab \u003c/a>in Palo Alto, the display at Chabot is showing visitors visions of our Sun unlike anything that has preceded it. \u003c/p>\n\u003cp>SDO was launched last year, and since then has been capturing high resolution, multi-wavelength visible and extreme-ultraviolet imagery at very frequent intervals. Its array of extreme-ultraviolet imaging telescopes (the \u003ca href=\"http://sdo.gsfc.nasa.gov/data/aiahmi/browse.php\">\"AIA\" instrument\u003c/a>) captures the energetic UV emissions from the Sun's hot atmosphere, revealing in extraordinary detail the Sun's busy and complicated magnetic activity: hot active regions, solar flares, coronal mass ejections, magnetic loops and arcs, and prominences. \u003c/p>\n\u003cp>The various images taken at the different wavelengths are \u003ca href=\"http://sdo.gsfc.nasa.gov/assets/img/latest/f_304_211_171_1024.jpg\">blended together \u003c/a>into an exquisitely colorful, nuanced, and delicious movie of a day of the life of the Sun (and with about 24 hours of images compressed into a few seconds, you really can see a day of its life!).\u003c/p>\n\u003cp>SDO was built to give us a much more detailed picture of what makes the Sun tick as we enter the 24th Solar Cycle, which started in the last few years. A \u003ca href=\"http://solarscience.msfc.nasa.gov/SunspotCycle.shtml\">Solar Cycle \u003c/a>is the period over which solar magnetic activity rises, climaxes, and falls again. Solar Cycle 1 started around the year 1755, and in the intervening centuries we've been through 23 cycles, which have averaged pretty reliably at about 11 years long each. (Solar Cycle 1, by the way, wasn't the first; that's just when they started numbering them, shortly after their discovery.)\u003c/p>\n\u003cp>Over the past few years, the Sun has been pretty quiet; our solar telescopes at Chabot have seen few sunspots (markers of regions of magnetic activity), and even the Sun's energetic atmosphere has been more or less quiescent, with only the occasional prominence or filament (\"clouds\" of cooler gases confined by solar magnetic fields) visible through special \"Hydrogen-Alpha\" filters. \u003c/p>\n\u003cp>But that's all changing now. Through our visible light telescopes, beautiful groups of sunspots have started making regular appearances, crossing the Sun's face as the Sun slowly rotates in space. Sunspots appear darker than the surrounding visible surface of the Sun, being a couple of thousand degrees cooler—but they are still quite bright; if we blocked off all of the Sun's light except that shining from an average sized sunspot (average meaning Earth-sized), it would appear as bright as the Full Moon on a clear night. \u003c/p>\n\u003cp>Through our Hydrogen-Alpha telescopes, prominences and filaments are becoming far more numerous, and more amazingly huge than over the past few years of minimal solar activity. \u003c/p>\n\u003cp>And the SDO movie display is revealing to us a great deal of activity—hot spots of magnetic mayhem spouting from within the Sun and surging into the atmosphere. With the peak of solar activity of Solar Cycle 24 expected to occur sometime in 2013, we're in for at least a couple of years of ever-increasing fireworks on the Sun, with all the related space weather storms, auroral light shows, and cell phone interference that comes with it. \u003c/p>\n\u003cp>What flavors of Sun are we serving then? Well, we have vanilla of course, served up by our little Sunspotter visible light telescopes—vanilla is my favorite ice cream…. And the Hydrogen-Alpha scopes scoop burgundy cherry and bubblegum in nice spoon-sized portions (bubblegum not your taste? Try some of ours…). \u003c/p>\n\u003cp>Imagery from the old and reliable \u003ca href=\"http://sohowww.nascom.nasa.gov/\">SOHO \u003c/a>satellite solar observatory offer blueberry, key lime, butter brickle, and strawberry. And the new SDO movies provide our newest menu items: mint chocolate chip, pistachio and black cherry, rainbow sherbet, and blueberry walnut banana supreme…or whatever unusual and mindboggling combination that comes to your mind when you look at them!\u003c/p>\n\u003cp>Come on up to Chabot for a taste! Napkins not provided….\u003c/p>\n\u003cp>\u003c/p>\n\u003cp> 37.8148 -122.178\u003c/p>\n\n",
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"content": "\u003cdiv class=\"post-body\">\u003cp>\u003cp>\u003cspan class=\"left\">\u003cimg src=\"http://ww2.kqed.org/quest/wp-content/uploads/sites/39/2011/04/f_304_211_171_1024s.jpg\">\u003cem>Extreme ultraviolet composite solar image from NASA's SDO. \u003cbr>Credit: NASA/SDO\u003c/em>\u003c/span>\u003c/p>\n\u003cp>\"If that was a scoop of ice cream, what kind would it be?\" I asked the 7-year-old girl visiting our 20-inch telescope's dome.\u003c/p>\n\u003cp>A pensive look crosses her face, as if she were standing at the counter of an ice cream parlor looking at the list of flavors. \"Mint chocolate chip,\" she decides. \u003c/p>\n\u003cp>The girl was looking at a new video display recently installed in the observatory at \u003ca href=\"http://www.chabotspace.org/index.htm\">Chabot Space & Science Center\u003c/a>, which shows up-to-the hour, time-compressed movies made from the spectacular solar imagery coming out of NASA's \u003ca href=\"http://sdo.gsfc.nasa.gov/\">Solar Dynamics Observatory \u003c/a>(SDO). \u003c/p>\n\u003cp>\u003c!--more-->\u003c/p>\n\u003cp>\u003c/p>\u003c/div>",
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"content": "\u003cdiv class=\"post-body\">\u003cp>\u003c/p>\n\u003cp>And it really does resemble a big, luminous, writhing ball of colorful ice cream (though what \"writhing ice cream\" is, I'm not certain; use your imagination).\u003c/p>\n\u003cp>Kept up-to-date by an Internet feed from Lockheed's \u003ca href=\"http://www.lmsal.com/\">Solar and Astrophysics Lab \u003c/a>in Palo Alto, the display at Chabot is showing visitors visions of our Sun unlike anything that has preceded it. \u003c/p>\n\u003cp>SDO was launched last year, and since then has been capturing high resolution, multi-wavelength visible and extreme-ultraviolet imagery at very frequent intervals. Its array of extreme-ultraviolet imaging telescopes (the \u003ca href=\"http://sdo.gsfc.nasa.gov/data/aiahmi/browse.php\">\"AIA\" instrument\u003c/a>) captures the energetic UV emissions from the Sun's hot atmosphere, revealing in extraordinary detail the Sun's busy and complicated magnetic activity: hot active regions, solar flares, coronal mass ejections, magnetic loops and arcs, and prominences. \u003c/p>\n\u003cp>The various images taken at the different wavelengths are \u003ca href=\"http://sdo.gsfc.nasa.gov/assets/img/latest/f_304_211_171_1024.jpg\">blended together \u003c/a>into an exquisitely colorful, nuanced, and delicious movie of a day of the life of the Sun (and with about 24 hours of images compressed into a few seconds, you really can see a day of its life!).\u003c/p>\n\u003cp>SDO was built to give us a much more detailed picture of what makes the Sun tick as we enter the 24th Solar Cycle, which started in the last few years. A \u003ca href=\"http://solarscience.msfc.nasa.gov/SunspotCycle.shtml\">Solar Cycle \u003c/a>is the period over which solar magnetic activity rises, climaxes, and falls again. Solar Cycle 1 started around the year 1755, and in the intervening centuries we've been through 23 cycles, which have averaged pretty reliably at about 11 years long each. (Solar Cycle 1, by the way, wasn't the first; that's just when they started numbering them, shortly after their discovery.)\u003c/p>\n\u003cp>Over the past few years, the Sun has been pretty quiet; our solar telescopes at Chabot have seen few sunspots (markers of regions of magnetic activity), and even the Sun's energetic atmosphere has been more or less quiescent, with only the occasional prominence or filament (\"clouds\" of cooler gases confined by solar magnetic fields) visible through special \"Hydrogen-Alpha\" filters. \u003c/p>\n\u003cp>But that's all changing now. Through our visible light telescopes, beautiful groups of sunspots have started making regular appearances, crossing the Sun's face as the Sun slowly rotates in space. Sunspots appear darker than the surrounding visible surface of the Sun, being a couple of thousand degrees cooler—but they are still quite bright; if we blocked off all of the Sun's light except that shining from an average sized sunspot (average meaning Earth-sized), it would appear as bright as the Full Moon on a clear night. \u003c/p>\n\u003cp>Through our Hydrogen-Alpha telescopes, prominences and filaments are becoming far more numerous, and more amazingly huge than over the past few years of minimal solar activity. \u003c/p>\n\u003cp>And the SDO movie display is revealing to us a great deal of activity—hot spots of magnetic mayhem spouting from within the Sun and surging into the atmosphere. With the peak of solar activity of Solar Cycle 24 expected to occur sometime in 2013, we're in for at least a couple of years of ever-increasing fireworks on the Sun, with all the related space weather storms, auroral light shows, and cell phone interference that comes with it. \u003c/p>\n\u003cp>What flavors of Sun are we serving then? Well, we have vanilla of course, served up by our little Sunspotter visible light telescopes—vanilla is my favorite ice cream…. And the Hydrogen-Alpha scopes scoop burgundy cherry and bubblegum in nice spoon-sized portions (bubblegum not your taste? Try some of ours…). \u003c/p>\n\u003cp>Imagery from the old and reliable \u003ca href=\"http://sohowww.nascom.nasa.gov/\">SOHO \u003c/a>satellite solar observatory offer blueberry, key lime, butter brickle, and strawberry. And the new SDO movies provide our newest menu items: mint chocolate chip, pistachio and black cherry, rainbow sherbet, and blueberry walnut banana supreme…or whatever unusual and mindboggling combination that comes to your mind when you look at them!\u003c/p>\n\u003cp>Come on up to Chabot for a taste! Napkins not provided….\u003c/p>\n\u003cp>\u003c/p>\n\u003cp> 37.8148 -122.178\u003c/p>\n\n\u003c/div>\u003c/p>",
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"content": "\u003cp>\u003cspan class=\"left\">\u003cimg src=\"http://ww2.kqed.org/quest/wp-content/uploads/sites/39/2011/04/0.jpg\" alt=\"\">\u003cem>Courtesy of yurisnight.net.\u003c/em>\u003c/span>\u003c/p>\n\u003cp>Yuri’s Night 2011 stats: 557 events in 75 countries on 6 continents on 2 worlds (Earth and the Space Station!)\u003c/p>\n\u003cp>50 years ago the launch of a bell-shaped capsule called “Vostok 1” on April 12th, 1961 by Soviet Cosmonaut Yuri Gagarin made history as the first human to enter outer space. Exactly 20 years later, the United States innovated the space age by launching the Space Shuttle (April 12th, 1981). Twenty years later Yuri’s Night was created to connect and inspire the globe about human spaceflight –– honoring the past while looking forward to the next generation of spaceflight (think \u003ca href=\"http://www.spacex.com/\">Space X\u003c/a>, the Google Lunar X Prize and \u003ca href=\"http://www.virgingalactic.com/\">Virgin Galactic\u003c/a>!) This year commemorates the 10th anniversary of Yuri’s Night, the 30th Anniversary of the US space shuttle and the 50th anniversary of human spaceflight! \u003c/p>\n\u003cp>\u003c!--more-->\u003c/p>\n\u003cp>This also marks the 3rd anniversary of California Academy of Sciences involvement with \u003ca href=\"http://yurisnight.net/\">Yuri’s Night\u003c/a>. The NightLife team first began working with NASA and the Yuri’s Night collective back in 2009. NASA decided to cancel their Saturday night party at NASA Ames and asked us to host it at NightLife instead. We had 3922 guests come out to celebrate spaceflight. One of the guests was even Buzz Aldrin! In 2010, we expanded our reach. We had another very successful Yuri’s NightLife at the Academy and then participated at NASA Ames on Yuri’s Night School day on Friday and on their Festival Day on Saturday. \u003c/p>\n\u003cp>[ad fullwidth]\u003c/p>\n\u003cp>This year, NightLife celebrated Yuri by focusing on space as the great frontier on Thursday, April 7th. The Planetarium showed Dawn of the Space Age, the Geodome was set up in the Piazza to show star talks and Hofeld Hall was set up to give tours of Alien Worlds. Fred Bourgeouis, III, the CEO of \u003ca href=\"http://www.frednet.com/\">Team Frednet\u003c/a> came into speak about how his team of over 700 volunteers is prototyping a rocket to fly to the moon to win the \u003ca href=\"http://www.googlelunarxprize.org/\">Google Lunar X Prize \u003c/a>and Mary Roach wowed and amused guests about fodder in her new book \u003cem>\u003ca href=\"http://www.maryroach.net/packing-for-mars.html\">Packing for Mars\u003c/a>\u003c/em>. \u003c/p>\n\u003cp>Around dawn on Friday April 8th, the Portable Planetarium along with some very sleep colleagues set out to NASA Ames in Mountain View to give star talks about the night sky. I was told by a friend at NASA, that there were 6432 kids in attendance that day. The planetarium was scheduled for 15 minutes talks each half hour but it was so popular the presenters found a way to give back-to-back shows every fifteen minutes from 9am to 3pm. The rest of us were on sticker duty, keeping the kids amused while they waited, giving information and answering the survey question – Which is visible now in the night sky? The answer being Saturn, we even had the appropriate sticker to give out. All in all, it was a great third year for the Academy’s Yuri’s Night festivities and two among 557 events that celebrated human spaceflight this year.\u003c/p>\n\u003cp>\u003c/p>\n\u003cp> 37.7699 -122.467174\u003c/p>\n\n",
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"disqusTitle": "The Word From Mercury: MESSENGER Has Been Delivered",
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"content": "\u003cp>\u003cspan class=\"left\">\u003cimg src=\"http://ww2.kqed.org/quest/wp-content/uploads/sites/39/2011/04/messenger-orbits-mercury.gif\">\u003cem>Artist concept of MESSENGER arriving at Mercury. \u003cbr>Credit: NASA\u003cbr>\u003c/em>\u003c/span>\u003c/p>\n\u003cp>History has been made yet again: NASA's MESSENGER spacecraft is now in orbit around the solar system's innermost planet! \u003c/p>\n\u003cp>This is exciting to me. When I was a child, Mercury was a contender in my mind for \"favorite planet\"—right up there with Pluto, being so far away and mysterious, and Uranus, being such a pretty shade of blue. Mind you, that was back before spacecraft had visited any of them…. \u003c/p>\n\u003cp>Being closest to the Sun gave Mercury a claim to fame—just as Venus being the hottest planet or Earth being the home planet or Mars being the red planet or Saturn having rings…okay, they're all special.\u003c/p>\n\u003cp>\u003c!--more-->\u003c/p>\n\u003cp>[ad fullwidth]\u003c/p>\n\u003cp>At first glance, \u003ca href=\"http://solarsystem.nasa.gov/planets/profile.cfm?Object=Mercury\">Mercury\u003c/a> presents the appearance of Earth's Moon, but doing just a little math tells you there's more to it. Just divide its mass by its volume and you get 5.43 grams per cubic centimeter—Mercury's average density. That's only a shade less than Earth's average density of 5.51 g/cc, which indicates that Mercury contains more heavy elements than the Moon—elements like iron, for example. (Personally, I suspect there's gold on that thar planet, too….) In fact, after Earth, Mercury is the densest known planet in the solar system. What does it hide under that cratered and radiation-baked surface?\u003c/p>\n\u003cp>An interesting tidbit about Mercury: because of its high density—because of the amount of material packed within its smallish confines—the surface gravity on Mercury is about the same as on Mars, even though Mars is larger. (Mercury has a diameter of just over 3000 miles, while Mars is about 4200 miles across.) On both worlds, you'd weight about 38% what you weigh on Earth. \u003c/p>\n\u003cp>And now, Mercury has joined a new club: planets that have been orbited by spacecraft—in this case, \u003ca href=\"http://www.nasa.gov/mission_pages/messenger/main/index.html\">NASA's MESSENGER\u003c/a>. MESSENGER has been en route to its final orbit around Mercury for over six and a half years. Since its launch on August 3, 2004, MESSENGER has been winding its way through the inner solar system, swinging back past Earth about a year after launch, making a couple of close passes by Venus, then three fly-bys of Mercury itself, before settling into orbit on March 17th. \u003c/p>\n\u003cp>This long and meandering path was a great fuel saver: by making flybys of planets, MESSENGER's trajectory and speed were altered to make the transition from Earth orbital velocity to a stable orbit around Mercury without burning a lot of fuel to do so. Other spacecraft have used gravitational \"slingshot\" maneuvers to change direction or gain speed for free, including the Voyagers and New Horizons (on its way to Pluto). \u003c/p>\n\u003cp>At Mercury, sunlight is up to ten times more intense than at Earth—and since Mercury has no atmosphere to filter out ultraviolet and X-rays, let's just say the sunburn you'd get standing on its surface would be nothing short of lethal. Never mind the lack of air….\u003c/p>\n\u003cp>To keep cool in the intense solar radiation environment around Mercury, MESSENGER takes advantage of the same physical principle that keeps the dark side of Mercury itself cool (as cold as negative 185 degrees F): insulation. Down on Mercury, the night-time surface is protected from the Sun's intense rays by an entire planet of material. With no atmosphere to trap heat, at night the temperature plummets as heat radiates from rocks and soil directly into space. \u003c/p>\n\u003cp>MESSENGER possesses a shield: a \"sun screen\" made of heat-resistant ceramic cloth, situated between the Sun and spacecraft much like someone holding a parasol to stay in the shade. \u003c/p>\n\u003cp>Poking out from behind its shield, MESSENGER wields two solar panels that provide the spacecraft all of its power—one distinct advantage of the otherwise troublesome intensity of Mercurial sunlight. \u003c/p>\n\u003cp>Now that MESSENGER is in orbit, what do we hope to discover in the days and months ahead? \u003c/p>\n\u003cp>Is there ice at the bottom of polar crater floors? How is Mercury's magnetic field generated? Does Mercury have, or did it have, plate tectonics? What's it made of? How does Mercury interact with plasma flowing from the Sun—the solar wind? Are there any strange obelisks on its surface? …to make just a partial list…. Answers to follow (for most of them, anyway). \u003c/p>\n\u003cp>\u003c/p>\n\u003cp> 37.8148 -122.178\u003c/p>\n\n",
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"content": "\u003cdiv class=\"post-body\">\u003cp>\u003c/p>\n\u003cp>At first glance, \u003ca href=\"http://solarsystem.nasa.gov/planets/profile.cfm?Object=Mercury\">Mercury\u003c/a> presents the appearance of Earth's Moon, but doing just a little math tells you there's more to it. Just divide its mass by its volume and you get 5.43 grams per cubic centimeter—Mercury's average density. That's only a shade less than Earth's average density of 5.51 g/cc, which indicates that Mercury contains more heavy elements than the Moon—elements like iron, for example. (Personally, I suspect there's gold on that thar planet, too….) In fact, after Earth, Mercury is the densest known planet in the solar system. What does it hide under that cratered and radiation-baked surface?\u003c/p>\n\u003cp>An interesting tidbit about Mercury: because of its high density—because of the amount of material packed within its smallish confines—the surface gravity on Mercury is about the same as on Mars, even though Mars is larger. (Mercury has a diameter of just over 3000 miles, while Mars is about 4200 miles across.) On both worlds, you'd weight about 38% what you weigh on Earth. \u003c/p>\n\u003cp>And now, Mercury has joined a new club: planets that have been orbited by spacecraft—in this case, \u003ca href=\"http://www.nasa.gov/mission_pages/messenger/main/index.html\">NASA's MESSENGER\u003c/a>. MESSENGER has been en route to its final orbit around Mercury for over six and a half years. Since its launch on August 3, 2004, MESSENGER has been winding its way through the inner solar system, swinging back past Earth about a year after launch, making a couple of close passes by Venus, then three fly-bys of Mercury itself, before settling into orbit on March 17th. \u003c/p>\n\u003cp>This long and meandering path was a great fuel saver: by making flybys of planets, MESSENGER's trajectory and speed were altered to make the transition from Earth orbital velocity to a stable orbit around Mercury without burning a lot of fuel to do so. Other spacecraft have used gravitational \"slingshot\" maneuvers to change direction or gain speed for free, including the Voyagers and New Horizons (on its way to Pluto). \u003c/p>\n\u003cp>At Mercury, sunlight is up to ten times more intense than at Earth—and since Mercury has no atmosphere to filter out ultraviolet and X-rays, let's just say the sunburn you'd get standing on its surface would be nothing short of lethal. Never mind the lack of air….\u003c/p>\n\u003cp>To keep cool in the intense solar radiation environment around Mercury, MESSENGER takes advantage of the same physical principle that keeps the dark side of Mercury itself cool (as cold as negative 185 degrees F): insulation. Down on Mercury, the night-time surface is protected from the Sun's intense rays by an entire planet of material. With no atmosphere to trap heat, at night the temperature plummets as heat radiates from rocks and soil directly into space. \u003c/p>\n\u003cp>MESSENGER possesses a shield: a \"sun screen\" made of heat-resistant ceramic cloth, situated between the Sun and spacecraft much like someone holding a parasol to stay in the shade. \u003c/p>\n\u003cp>Poking out from behind its shield, MESSENGER wields two solar panels that provide the spacecraft all of its power—one distinct advantage of the otherwise troublesome intensity of Mercurial sunlight. \u003c/p>\n\u003cp>Now that MESSENGER is in orbit, what do we hope to discover in the days and months ahead? \u003c/p>\n\u003cp>Is there ice at the bottom of polar crater floors? How is Mercury's magnetic field generated? Does Mercury have, or did it have, plate tectonics? What's it made of? How does Mercury interact with plasma flowing from the Sun—the solar wind? Are there any strange obelisks on its surface? …to make just a partial list…. Answers to follow (for most of them, anyway). \u003c/p>\n\u003cp>\u003c/p>\n\u003cp> 37.8148 -122.178\u003c/p>\n\n\u003c/div>\u003c/p>",
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