2007-2012 Double-sided Mission Events Calendar, part of the Dawn Mission Art series.  http://photojournal.jpl.nasa.gov/catalog/PIA19378
Dawn 2007-2012 Double-sided Mission Events Calendar
NASA Spitzer Space Telescope celebrated its 12th anniversary with a new digital calendar showcasing some of the mission most notable discoveries and popular cosmic eye candy.  The digital calendar is online at http://www.jpl.nasa.gov/images/spitzer/20150820/Spitzer12thAnniversaryCalendar.pdf  The calendar follows the life of the mission, with each month highlighting top infrared images and discoveries from successive years -- everything from a dying star resembling the eye of a monster to a star-studded, swirling galaxy. The final month includes a brand new image of the glittery star-making factory known as the Monkey Head nebula.  Spitzer, which launched into space on August 25, 2003, from Cape Canaveral, Florida, is still going strong. It continues to use its ultra-sensitive infrared vision to probe asteroids, comets, exoplanets (planets outside our solar system) and some of the farthest known galaxies. Recently, Spitzer helped discover the closest known rocky exoplanet to us, named HD219134b, at 21 light-years away.  In fact, Spitzer's exoplanet studies continue to surprise the astronomy community. The telescope wasn't originally designed to study exoplanets, but as luck -- and some creative engineering -- would have it, Spitzer has turned out to be a critical tool in the field, probing the climates and compositions of these exotic worlds. This pioneering work began in 2005, when Spitzer became the first telescope to detect light from an exoplanet.  http://photojournal.jpl.nasa.gov/catalog/PIA19872
NASA Spitzer 12th Anniversary Space Calendar
The mosaic of Visible and Infrared Spectrometer (VIR) data shows the location of the data acquired by VIR during the HAMO (high-altitude mapping orbit) phase of NASA's Dawn mission. VIR can image Vesta in a number of different wavelengths of light, ranging from the visible to the infrared part of the electromagnetic spectrum. This mosaic shows the images taken at a wavelength of 550 nanometers, which is in the visible part of the electromagnetic spectrum. During HAMO VIR obtained more than 4.6 million spectra of Vesta. It is clear from this image that the VIR observations are widely distributed across Vesta, which results in a global view of the spectral properties of Vesta's surface.  http://photojournal.jpl.nasa.gov/catalog/PIA19368
Dawn 2013-2015 Double-sided Mission Events Calendar
Snow covered the northeastern United States on last day of meteorological winter, 2014. Climatologists and meteorologists break seasons down into three-month groups, based on annual temperature and our calendar. This method is helpful for weather observing and forecasting, and for planning consistent agricultural dates, such as expected first frosts or best planting date. Meteorological winter – the season where temperatures are, on average, coldest and when snow is most likely to fall – runs from December 1 to February 28 in the United States and Canada.  Winter can also be defined by the astronomical calendar, which is based on the rotation of the Earth around the sun. In this method, the seasons are defined by two solstices (times when the sun’s path is furthest from the Earth’s equator) and two equinoxes (the times when the sun passes directly above the equator). In the Northern Hemisphere, winter begins on the winter solstice, which falls on or around December 22 and ends on or around March 21, at the vernal (spring) equinox.  On February 28, 2014, the Moderate Resolution Imaging Spectroradiometer aboard NASA’s Aqua satellite captured this true-color image of a sunny winter day in the northeastern United States. Snow stretches from Maine west to Indiana and south along the ridges of the Appalachian Mountains well into West Virginia. In Canada, the landscape appears greener, primarily because snow lies on conifers (evergreen) trees in the boreal forest regions. The Great Lakes, with the exception of Lake Ontario, are almost completely covered with ice.  Credit: NASA/GSFC/Jeff Schmaltz/MODIS Land Rapid Response Team   <b><a href="http://www.nasa.gov/audience/formedia/features/MP_Photo_Guidelines.html" rel="nofollow">NASA image use policy.</a></b>  <b><a href="http://www.nasa.gov/centers/goddard/home/index.html" rel="nofollow">NASA Goddard Space Flight Center</a></b> enables NASA’s mission through four scientific endeavors: Earth Science, Heliophysics, Solar System Exploration, and Astrophysics. Goddard plays a leading role in NASA’s accomplishments by contributing compelling scientific knowledge to advance the Agency’s mission.  <b>Follow us on <a href="http://twitter.com/NASAGoddardPix" rel="nofollow">Twitter</a></b>  <b>Like us on <a href="http://www.facebook.com/pages/Greenbelt-MD/NASA-Goddard/395013845897?ref=tsd" rel="nofollow">Facebook</a></b>  <b>Find us on <a href="http://instagram.com/nasagoddard?vm=grid" rel="nofollow">Instagram</a></b>
Snow in northeastern United States
New Moon. By the modern definition, New Moon occurs when the Moon and Sun are at the same geocentric ecliptic longitude. The part of the Moon facing us is completely in shadow then. Pictured here is the traditional New Moon, the earliest visible waxing crescent, which signals the start of a new month in many lunar and lunisolar calendars.  NASA's Lunar Reconnaissance Orbiter (LRO) has been in orbit around the Moon since the summer of 2009. Its laser altimeter (LOLA) and camera (LROC) are recording the rugged, airless lunar terrain in exceptional detail, making it possible to visualize the Moon with unprecedented fidelity. This is especially evident in the long shadows cast near the terminator, or day-night line. The pummeled, craggy landscape thrown into high relief at the terminator would be impossible to recreate in the computer without global terrain maps like those from LRO.  To download, learn more about this visualization, or to see what the Moon will look like at any hour in 2015, visit <a href="http://svs.gsfc.nasa.gov/goto?4236" rel="nofollow">svs.gsfc.nasa.gov/goto?4236</a>  <b><a href="http://www.nasa.gov/audience/formedia/features/MP_Photo_Guidelines.html" rel="nofollow">NASA image use policy.</a></b>  <b><a href="http://www.nasa.gov/centers/goddard/home/index.html" rel="nofollow">NASA Goddard Space Flight Center</a></b> enables NASA’s mission through four scientific endeavors: Earth Science, Heliophysics, Solar System Exploration, and Astrophysics. Goddard plays a leading role in NASA’s accomplishments by contributing compelling scientific knowledge to advance the Agency’s mission. <b>Follow us on <a href="http://twitter.com/NASAGoddardPix" rel="nofollow">Twitter</a></b> <b>Like us on <a href="http://www.facebook.com/pages/Greenbelt-MD/NASA-Goddard/395013845897?ref=tsd" rel="nofollow">Facebook</a></b> <b>Find us on <a href="http://instagram.com/nasagoddard?vm=grid" rel="nofollow">Instagram</a></b>
New Moon
New Moon. By the modern definition, New Moon occurs when the Moon and Sun are at the same geocentric ecliptic longitude. The part of the Moon facing us is completely in shadow then. Pictured here is the traditional New Moon, the earliest visible waxing crescent, which signals the start of a new month in many lunar and lunisolar calendars.  This marks the first time that accurate shadows at this level of detail are possible in such a computer simulation. The shadows are based on the global elevation map being developed from measurements by the Lunar Orbiter Laser Altimeter (LOLA) aboard the Lunar Reconnaissance Orbiter (LRO). LOLA has already taken more than 10 times as many elevation measurements as all previous missions combined.  The Moon always keeps the same face to us, but not exactly the same face. Because of the tilt and shape of its orbit, we see the Moon from slightly different angles over the course of a month. When a month is compressed into 12 seconds, as it is in this animation, our changing view of the Moon makes it look like it's wobbling. This wobble is called libration.  The word comes from the Latin for &quot;balance scale&quot; (as does the name of the zodiac constellation Libra) and refers to the way such a scale tips up and down on alternating sides. The sub-Earth point gives the amount of libration in longitude and latitude. The sub-Earth point is also the apparent center of the Moon's disk and the location on the Moon where the Earth is directly overhead.  The Moon is subject to other motions as well. It appears to roll back and forth around the sub-Earth point. The roll angle is given by the position angle of the axis, which is the angle of the Moon's north pole relative to celestial north. The Moon also approaches and recedes from us, appearing to grow and shrink. The two extremes, called perigee (near) and apogee (far), differ by more than 10%.  The most noticed monthly variation in the Moon's appearance is the cycle of phases, caused by the changing angle of the Sun as the Moon orbits the Earth. The cycle begins with the waxing (growing) crescent Moon visible in the west just after sunset. By first quarter, the Moon is high in the sky at sunset and sets around midnight. The full Moon rises at sunset and is high in the sky at midnight. The third quarter Moon is often surprisingly conspicuous in the daylit western sky long after sunrise.  Celestial north is up in these images, corresponding to the view from the northern hemisphere. The descriptions of the print resolution stills also assume a northern hemisphere orientation. To adjust for southern hemisphere views, rotate the images 180 degrees, and substitute &quot;north&quot; for &quot;south&quot; in the descriptions.  Credit: <a href="http://svs.gsfc.nasa.gov/index.html" rel="nofollow">NASA/Goddard Space Flight Center Scientific Visualization Studio</a>  <b><a href="http://www.nasa.gov/centers/goddard/home/index.html" rel="nofollow">NASA Goddard Space Flight Center</a></b> enables NASA’s mission through four scientific endeavors: Earth Science, Heliophysics, Solar System Exploration, and Astrophysics. Goddard plays a leading role in NASA’s accomplishments by contributing compelling scientific knowledge to advance the Agency’s mission.  <b>Follow us on <a href="http://twitter.com/NASA_GoddardPix" rel="nofollow">Twitter</a></b>  <b>Join us on <a href="http://www.facebook.com/pages/Greenbelt-MD/NASA-Goddard/395013845897?ref=tsd" rel="nofollow">Facebook</a></b>  <b>Find us on <a href="http://web.stagram.com/n/nasagoddard/?vm=grid" rel="nofollow">Instagram</a></b>
New Moon
In October 1963, the Project Mercury Summary Conference was held in the Houston, TX, Coliseum.  This series of 44 photos is documentation of that conference.            A view of the Houston, TX, Coliseum, and parking area in front with a Mercury Redstone Rocket setup in the parking lot for display (S63-16451).            A view of an Air Force Atlas Rocket, a Mercury Redstone Rocket, and a Mercury Spacecraft on a test booster on display in the front area of the Coliseum (S63-16452).        A view an Air Force Atlas Rocket and a Mercury Redstone Rocket set up for display with the Houston City Hall in the background (S63- 16453).          This view shows the Atlas Rocket, Mercury Redstone, and Mercury Test Rocket with the Houston, TX, Coliseum in the background (S63- 16454).            A balcony view, from the audience right side, of the attendees looking at the stage (S63-16455).         A view of the NASA Space Science Demonstration with equipment setup on a table, center stage and Space Science Specialist briefing the group as he pours Liquid Oxygen into a beaker (S63-16456).        View of the audience from the balcony on the audience right showing the speakers lecturn on stage to the audience left (S63-16457).            A view of attendees in the lobby.  Bennet James, MSC Public Affairs Office is seen to the left of center (S63-16458).    Another view of the attendees in the lobby (S63- 16459).            In this view, Astronaut Neil Armstrong is seen writing as others look on (S63-16460).            In this view of the attendees, Astronauts Buzz Aldrin and Walt Cunningham are seen in the center of the shot.  The October Calendar of Events is visable in the background (S63-16461).        Dr. Charles Berry is seen in this view to the right of center, seated in the audience (S63-16462).           View of " Special Registration " and the five ladies working there (S63-16463).           A view from behind the special registration table, of the attendees being registered (S63-16464).        A view of a conference table with a panel seated. (R-L):  Dr. Robert R. Gilruth, Hugh L. Dryden, Walter C. Williams, and an unidentified man (S63- 16465).           A closeup of the panel at the table with Dr. Gilruth on the left (S63-16466).           About the same shot as number S63-16462,  Dr. Berry is seen in this shot as well (S63-16467).            In this view the audio setup is seen.  In the audience, (L-R):  C. C. Kraft, Vernon E. (Buddy) Powell, Public Affairs Office (PAO); and, in the foreground mixing the audio is Art Tantillo; and, at the recorder is Doyle Hodges both of the audio people are contractors that work for PAO at MSC (S63-16468).             In this view Maxime Faget is seen speaking at the lecturn (S63-16469).          Unidentified person at the lecturn (S63-16470).         In this view the motion picture cameras and personel are shown documenting the conference (S63-16471).         A motion picture cameraman in the balcony is shown filming the audience during a break (S63- 16472).         Family members enjoy an exhibit (S63-16473).         A young person gets a boost to look in a Gemini Capsule on display (S63-16474).        A young person looks at the Gemini Capsule on display (S63-16475).         Dr. Robert R. Gilruth is seen at the conference table (S63-16476).        Walt Williams is seen in this view at the conference table (S63-16477).        Unidentified man sitting next to Walt Williams (S63-16478).        (L-R):  Seated at the conference table, Dr. Robert Gilruth, Hugh L. Dryden, and Walt Williams (S63- 16479).         Group in lobby faces visable, (L-R):  Walt Williams, unidentified person,  Dr. Robert Gilruth, Congressman (S63-16480).          Man in uniform at the lecturn (S63-16481).         Astronaut Leroy Gordon Cooper at the lecturn (S63-16482).         Astronaut Cooper at the lecturn with a picture on the screen with the title, " Astronaut Names for Spacecraft " (S63-16483).         Dr. Gilruth at the lecturn (S63-16484).         Walt Williams at the lecturn (S63-16485).         Unidentified man at the lecturn (S63-16486).         John H. Boynton addresses the Summary Conference (S63-16487).        (L-R):  Astronaut Leroy Gordon Cooper, Mrs. Cooper, Senator Cris Cole, and Mrs. Cole (S63- 16488).        In this view in the lobby, Senator and Mrs. Cris Cole, with Astronaut Gordon Cooper standing near the heatshield, and Mrs. Cooper; next, on the right is a press photographer (S63-16489).           (L-R):  Astronaut L. Gordon Cooper and Mrs. Cooper, unidentified man, and Senator Walter Richter (S63-16490).         (L-R):  Eugene Horton, partially obscured, briefs a group on the Mercury Spacecraft, an unidentified person, Harold Ogden, a female senator, Senator Chris Cole, Mrs. Cole, an unidentified female, Senator Walter Richter, Jim Bower, and an unidentified female (S63-16491).         In this view, Mrs. Jim Bates is seen in the center, and Senator Walter Richter to the right (S63- 16492).         The next three (3) shots are 4X5 CN (S63-16493 - S63-16495).         In this view a NASA Space Science Demonstration is seen (S63-16493).        In this view a shot of the conference table is seen, and, (L-R):  Dr. Robert R. Gilruth, Hugh L. Dryden, Mr. Walter Williams, and an unidentfied man (S63-16494 - S63-16495).        HOUSTON, TX
PROJECT MERCURY SUMMARY CONFERENCE - NASA - HOUSTON, TX