News
News from Boulder, Colorado and Boulder Channel 1 News editors To advertise please call 303-447-8531
FEB. 23 NASA MISSION TO TOTE $28 MILLION CU-BOULDER INSTRUMENT AND TINY STUDENT SATELLITE
Feb 22nd
Designed and built by a team from CU-Boulder’s Laboratory for Atmospheric and Space Physics, the instrument called the Total Irradiance Monitor, or TIM, will point directly toward the sun to measure both short- and long-term fluctuations in the sun’s energy output as it reaches the top of Earth’s atmosphere. Such measurements are important because variations in the sun’s radiation can influence long-term climate change on Earth, said LASP researcher Greg Kopp, principal investigator on the TIM.
The Taurus XL rocket ferrying the Glory satellite also will be carrying a tiny CU-Boulder satellite designed and built by about 100 students, primarily undergraduates, who are participating in the Colorado Space Grant Consortium. The CubeSat satellite will be ejected from the rocket at about 400 miles in altitude to orbit the Earth and study new space communications techniques.
The CU-Boulder solar instrument on Glory is the most accurate instrument ever made to study the energy output from the sun and will continue a 32-year-long data record of solar radiation by NASA and other agencies, said Kopp. NASA’s Solar Radiation and Climate Experiment, a $100 million satellite designed, built and operated by CU-Boulder’s LASP and launched in 2003, is equipped with a first-generation TIM instrument as well as three other solar measuring instruments.
“We’d like to know how the sun’s energy changes over both the short and long term,” said Kopp. “This spacecraft is carrying extremely sensitive instruments for monitoring solar variability, which makes the mission especially relevant given climate change on Earth and the importance of determining the natural influence on those changes.”
Glory will join five other NASA Earth-observing satellites as part of the Afternoon Constellation, or “A-Train,” a tightly grouped series of spacecraft that circle the globe several times each day to gather information on Earth’s biosphere and climate, including hurricane behavior and climate change. The A-Train spacecraft follow each other in close formation, flying mere minutes apart. The A-Train orbits Earth about once every 100 minutes.
The second primary instrument on the Glory mission, called the Aerosol Polarimetry Sensor, or APS, was built by Raytheon Space and Airborne Systems in El Segundo, Calif. Scientists hope to learn how tiny liquid and solid aerosols — most smaller than the diameter of a human hair — influence climate on Earth.
Using Glory as well as prior and subsequent missions to measure solar radiation changes, scientists hope to determine how much energy reaches Earth on timescales of decades to centuries, influencing Earth’s long-term climate.
Scientists previously have shown that the overall output of the sun can change up to about 0.1 percent over the duration of a solar cycle, which lasts about 11 years. But such short-term variations cannot explain the warming seen on Earth in the past several decades. The vast majority of climate scientists agree global warming is due primarily to human-produced greenhouse gases building up in the atmosphere.
“In attributing climate change causes, solar variability measurements such as those from Glory are necessary to discriminate the natural from the human-caused effects on the climate,” Kopp said.
LASP has a long record of measuring solar radiation with various satellites and sounding rockets, including the Solar Mesosphere Explorer satellite that flew from 1981 to 1988 and which was dubbed “The Classroom in Space.” SME measured ozone and solar radiation and involved undergraduate and graduate students in virtually every phase of the effort, from design and development to hands-on control of the satellite from campus.
Because of technological advances, the TIM riding on Glory is expected to be three times more accurate than the TIM flying on CU-Boulder’s SORCE satellite, according to Kopp. The improvement is due in large part to better electrical design and more precise calibrations of solar space instruments that are being made using a new NASA-funded facility at LASP.
The second CU-Boulder payload, a CubeSat satellite dubbed Hermes that was designed and built by students, primarily undergraduates, is about four inches on a side — roughly the size of a Rubik’s Cube. The goal is to improve communications systems in tiny satellites through orbital testing that may pave the way for scientists to downlink large quantities of information, said Colorado Space Consortium Director Chris Koehler.
The students will be in contact with the Hermes satellite from atop the Discovery Learning Center, part of CU-Boulder’s College of Engineering and Applied Science, said senior aerospace engineering sciences major Nicole Doyle, Hermes project manager. Ten CU-Boulder students will be traveling to California for the Hermes launch.
Hermes is part of NASA’s Educational Launch of Nanosatellites, or ELaNa, project. Two other CubeSat satellites will be aboard the Taurus rocket with Glory, one from Montana State University and one from Kentucky Space, a consortium of Kentucky state institutions.
Doyle said when she first came to CU-Boulder she was surprised to discover that undergraduates had regular opportunities to design, build, test and fly spacecraft. “This has been an incredible experience for me,” she said. “We learn from other CU students who are working on other space projects and who have experience in the kinds of research we are doing with Hermes. This is a great opportunity for students like me who want to work in the aerospace industry after college.”
Other LASP personnel on Glory include Project Manager Tom Sparn, lead systems engineer Brian Boyle, lead mechanical engineer Alan Yehle, lead electrical engineer Aref Nammari and lead integration and test engineer David Gathright. LASP students, including several undergraduates in conjunction will several professionals, will operate the orbiting TIM instrument from LASP’s Mission Operations Center on CU-Boulder’s East Campus.
Glory is managed by NASA’s Goddard Space Flight Center in Greenbelt, Md. Launch management is provided by NASA’s Launch Services Program at the agency’s Kennedy Space Center in Florida.
For more information about NASA’s Glory Mission visit http://www.nasa.gov. For more information on LASP visit http://lasp.colorado.edu/home/. For more information on the Colorado Space Grant Consortium visit http://spacegrant.colorado.edu/.
-CU-
CU’S GLENN MILLER ARCHIVE ACQUIRES ONE OF WORLD’S BEST BIG BAND ERA COLLECTIONS
Feb 21st
The Glenn Miller Archive at the University of Colorado Boulder American Music Research Center has acquired one of the world’s most significant collections of Big Band Era recordings and memorabilia.
The Ed Burke Collection – named for its shepherd and founder – contains approximately 1,400 reel-to-reel tapes containing hundreds of hours of live radio programs featuring virtually every musician of major importance during the Big Band Era.
“This collection is especially extraordinary as the material is in a live radio context,” said Professor Tom Riis, director of the American Music Research Center in the College of Music. “We have the announcer’s voice, the advertising, everything. It is also in remarkably good condition, as the tapes were made directly from the transcription discs loaned to Ed by the radio stations.”
The vast collection includes performances by almost every Big Band musician and entertainer who appeared on records or radio between 1930 and 1960, including broadcasts by Glenn Miller, Louis Armstrong, Tommy Dorsey, Count Basie, Duke Ellington and Benny Goodman. The collection has been transferred in its entirety to the Glenn Miller Archive for permanent preservation.
In addition to the historically valuable collection of live recordings – which includes original material never distributed commercially – the collection also includes photographs, magazines, documents and other memorabilia from the unique era in American popular music. An avid fan and collector, Ed Burke founded and operated the independent record and compact discs labels Fanfare, Jazz Hour and Soundcraft.
“The Glenn Miller Archive honors and preserves the legacy of our distinguished alumnus, Glenn Miller,” said archive curator Alan Cass, “and we are grateful to Ed Burke for his lifelong dedication to preserving an important segment of American popular music.”
To view a short sound slide on the Ed Burke Collection visit http://www.colorado.edu/news and click on the story headline.
For those interested in hearing the music of the era brought to life, the award-winning musicians of CU Jazz Ensemble I from the College of Music are staging the inaugural Spring Swing concert Feb. 27 at 2 p.m. in Macky Auditorium. Big Band Era favorites scheduled for the performance include “In the Mood,” “Moonlight Serenade” and “A String of Pearls.”
For more information on the concert visit http://music.colorado.edu/events.
-CU-
Full Moon NOW!! It’s a Werewolf Moon!!! Science story:
Feb 18th
Amateur astronomers have a love-hate relationship with the full moon. While beautiful to look at, the full moon also floods the night sky with natural “light pollution,” dimming otherwise visible stars and especially the astronomers’ favorite deep sky objects.
The full moon of February, known as the Wolf Moon, will arrive Friday (Feb. 18).
While some astronomers may opt to watch reruns of the space science TV show “Cosmos” when their precious deep sky targets are too faint to see, they are missing one of the special treats of astronomy: observing the full moon with only their eyes, or perhaps binoculars.
Ads by GoogleCurrent Moon PhaseSee the current moon phase based on your location. Add it iGoogle!www.google.com/igDate Of Full MoonSearch multiple engines for date of full moonwww.webcrawler.comWhat is Quantum Jumping?Discover Why Thousands of People are “Jumping” to Change Their Lifewww.QuantumJumping.com
Each full moon during the year has a traditional name in different human cultures. February’s full moon is best known as the Wolf Moon among some Native American tribes.
The Algonquian peoples of North America called it the Snow Moon. Other names are Hunger Moon, Storm Moon, and Candles Moon. In Hindi it is known as Magh Poornima. Its Sinhala (Buddhist) name is Navam Poya.
The official time of the full moon this month is Feb. 18 at 8:36 Universal Time. The full moon takes place at exactly the same time everywhere in the world, but the local time depends on the time zone.
For people in eastern North America that is Eastern Standard Time: 3:36 a.m. EST. On the west coast it’s at 12:36 a.m. PST
Full moon mechanics revealed
For some people, the fact that the full moon has specific date and time (rather than an entire night) may be puzzling. But it’s really all about geometry and moon mechanics.
When the sun, Earth and moon – in that order – fall in a straight line, or as close to a straight line as they can get, the moon is full. Because the moon’s orbit is slightly tilted to the ecliptic, there is usually a slight kink in the lineup, and the Earth’s shadow passes above or below the moon.
That’s why there is not a lunar eclipse every month.
This is also the only time in the month when the moon is exactly opposite the sun in Earth’s sky. On this date, and this date only, the moon rises as the sun sets, shines all night long, and sets as the sun rises.
Every other night in the month, there is at least a little time each night when the moon is not in the sky. By the same token, there is at least a bit of time when the moon is in the daytime sky.
The rising full moon often appears large and has an orange or red hue. The large size is an optical illusion; the moon is always the same size no matter where it is in the sky.
The color (except during a lunar eclipse) is just due to light being scattered in the Earth’s atmosphere.
“Seas” of the moon
It’s amazing how much detail can be seen on the full moon with just the naked eye.
Notice first the difference between the darker top half of the moon and the brighter bottom half, caused by the different reflecting power of the northern half’s predominant lava plains (called “seas” by early astronomers) and the south’s mountainous highlands.
The top half of the moon is clearly divided into three major “seas”: left to right (in the northern hemisphere) they are the Mare Imbrium, Mare Serenitatis and Mare Crisium. Those are the fanciful Latin names, which translate to: Sea of Rains, Sea of Serenity, and Sea of Crises.
Two prominent craters mark the moon’s equator: Aristarchus on the left and Copernicus towards the center. South of these is the Oceanus Procellarum, the Ocean of Storms.
The brighter highlands that make up the southern half of the moon are dominated by the brilliant white crater Tycho and its complex system of rays. The asteroid that formed Tycho sent material flying in all directions in low orbit, only to be deposited on the darker underlying surface.
Although the full moon is an instantaneous event, the moon looks full to the naked eye for a day or two on either side of the instant of full moon.
This article was provided to SPACE.com by Starry Night Education, the leader in space science curriculum solutions.
Source: Space, Starry Night Software