GRAA NEWSLETTER
P.O. Box 1184, Greenbelt, MD 20768-1184
August 2019 | http://graa.gsfc.nasa.gov | 35th Year of Publication |
IMPORTANT DATES
August 13 | Mark your calendar for the GRAA Luncheon starting at 11:15 a.m. at the Greenbelt American Legion Post #136 at 6900 Greenbelt Road. Reservations are required, so please contact Alberta Moran on her cell phone at 301-910-0177 or via her email address at bertiemae90@gmail.com not later than noon on August 9th. Dr. Gary Blackwood, Program Manager for the NASA Exoplanet Exploration Program at the Jet Propulsion Laboratory, will describe the inherent challenges in building systems to image planets around distant stars that are light years away. He has entitled his presentation “Show Me the Planets! NASA’s Exoplanet Exploration Program.” |
September 10 | GRAA Luncheon starting at 11:15 a.m. Dr. Donald Jennings, an Astrophysics/Engineer in GSFC’s Detector Systems Branch, will be our featured speaker with his talk entitled “New Horizons Visits Ultima Thule. In 2016, he spoke about the GSFC-built instrument Linear Etalon Imaging Spectral Array (LEISA) images captured during the New Horizons flyby of Pluto in 2015. The spacecraft then continued on for another billion miles to visit Ultima Thule, a second Kuiper Belt object. |
COMMENTS FROM TONY COMBERIATE, GRAA PRESIDENT: Our July speakers were GRAA members and original GSFC employees Ron Muller and Ed Habib who described key developments in the founding of the Center. In addition, Raquel Marshall, GFSC’s Education Program Manager who coordinates the GSFC Intern program, brought 14 interns and their mentors. These interns are undergraduate and graduate students from universities throughout the country, as far away as the state of Washington and as near as the University of Maryland, Baltimore County and Bowie State University, majoring in several branches of engineering, computer science, astrophysics, business, communications, finance and marketing. They introduced themselves and their mentors and spoke about the exciting work they are doing at GSFC this summer.
Ron Muller’s presentation was entitled “1957: The Year the Space Age Began,” and he described what it was like in 1957 when he worked for the Naval Research Laboratory (NRL) helping develop the Vanguard spacecraft and tracking the Russian Sputnik spacecraft which was launched that year. The Vanguard satellite was the first spacecraft with solar cells and also the first spacecraft to separate from its launch vehicle. Ron was one of the 159 Vanguard Project employees who were transferred from NRL to NASA on November 16, 1958, once President Eisenhower signed his executive order. In December of that year, another 62 NRL employees transferred to NASA, most of them to Langley Research Center (LRC). On January 22, 1959, the Beltsville Space Center was established with four divisions reporting directly to NASA HQ. On March 16, 1959, the Center was dedicated and officially renamed the Goddard Space Flight Center on May 1st of that year. Ron showed photos of the Center that indicated how quickly it developed during its early days. In its first decade, GSFC launched 89 successful missions.
Ed Habib described the beginnings of the NASA satellite-tracking program. Ed, also an NRL Vanguard Project employee who was transferred to GSFC in 1958, headed the branch that developed the tracking, telemetry and command systems essential for a space program. In 1955, as part of the US contribution to the International Geophysical Year, an artificial Earth satellite was to be launched in a civilian program with three objectives: 1) to deliver a satellite into Earth orbit; 2) to prove that it is in orbit; and 3) to conduct a scientific experiment. Ed spoke about the origin of the Minitrack System, which was developed to verify the second objective. It was based on interferometry, tracing back to the Viking program of the 1950s and utilizing the internationally-agreed upon satellite frequency of 108 MHz.
The Minimum Trackable Satellite (Minitrack) concept was proposed by Milt Rosen, John Mengel and Roger Easton at NRL. This concept involves measurement of the phase difference between radio waves from distant transmitters as detected by antenna pairs on the ground. The original stations utilized an array of 8 antennas up to 500 feet apart (or 50 wavelengths at 108 MHz) and had to be built on flat land in a radio silent area. To determine the orbit of a satellite travelling at 25,000 ft/sec accurate to one milliarcsecond, the system had to be able to measure a fraction of a wavelength to one part in 1,000. The 8 antennas provided coarse, medium, and fine phase sensing as well as ambiguity resolution. Each station had to have accurate timing calibrated to National Bureau of Standards (re: WWV) universal time broadcasts (Ed also managed this effort). The first Minitrack station, in Blossom Point, MD, became operational in July 1956 and became a training facility for a network of Minitrack stations along the 75th meridian with stations in places like Havana, Panama, Lima, Antofagasta, and Santiago. A ‘radio fence’ of stations with overlapping antenna patterns was needed to cover the planned orbital inclination of the Vanguard satellite. The system was tested with aircraft transmitter overflights and later with arrays of observers with telescopes marking the time a satellite crossed a field-of-view during twilight.
Right after the Minitrack network became operational, the Soviet Union unexpectedly launched Sputnik, which transmitted at 20MHz and 40MHz, and the 108 MHz Minitrack system was unable to track it. However, engineers immediately began cutting 40MHz dipoles and made other modifications that allowed the system to track the Russian satellites.
THOUGHT FOR AUGUST: Growing old can definitely be hard work… The mind says “yes,” but the body says, “What were you thinking?”
REMEMBERING OUR FORMER COLLEAGUES:
FROM THE GODDARD ARCHIVES – IT HAPPENED IN AUGUST: On August 21, 1996, a Pegasus XL rocket launched the Fast Auroral SnapshoT Explorer (FAST) successfully from Vandenberg Air Force Base, CA, into its intended orbit. The spacecraft investigated the plasma physics of auroral phenomena at extremely high time and spatial resolution using the full complement of particle and field instruments. FAST is the second spacecraft (SAMPEX was first) in the Small Explorer (SMEX) program at NASA-GSFC. SMEX was established to provide rapid (3-year development mission opportunities (1 per year) and low cost ($35M development) to the space science community using a single designated Principal Investigator. The FAST electric field instrument stopped providing meaningful data around 2002; however, all other instruments and systems continued to function normally. Although the FAST mission duration was intended to be a year, operations did not end until May 4, 2009.
TREASURER'S REPORT: Treasurer Jackie Gasch received tax-deductible donations from Helmut Cline, Alberta Moran (in memory of Priscilla Struthers), Thomas Underwood, and Charles E. White (in memory of William Witt).