From: Ron Baalke
Subject: Mars Global Surveyor Update - May 1, 1998
Mars Global Surveyor
Flight Status Report
Friday, 1 May 1998
This week, the Mars Global Surveyor flight team closed out a
successful month of dedicated science operations. For over sixty
consecutive orbits starting in early April and ending on Tuesday, the spacecraft's scientific instruments collected data near the low point of its 11.6-hour orbit. Every day of that month, Surveyor transmitted nearly
25 megabytes of data back to Earth.
Much of the publicity generated by April's science collection
activities focused on targeted observations of several selected sites on the Martian surface. Because explicit targeting is not part of the
Surveyor spacecraft's inherent abilities, these operations involved a substantial collaborative effort between Dr. Michael Malin's camera team, Dr. David Smith's laser altimeter team that assisted with Mars map
corrections, and project engineering elements such as mission planning, spacecraft systems, and navigation.
Major imaging highlights included three photographs of the Cydonia
region in the northern hemisphere. This area is home to a one-mile (1.5- km) wide object known popularly as the "face on Mars." One of the three Cydonia images shows the so-called face at 14.1-feet (4.3 meters) per pixel, a resolution about 10 times better than the best Viking Orbiter image from 1976.
In addition to the Cydonia images, Surveyor's camera also obtained
two photographs of the Viking 1 landing site in Chryse Planitia, and one image of the Mars Pathfinder landing site in the Ares Valles region. Some of the objects visible in the Pathfinder image include major landmarks photographed on July 4th, 1997, including the famous "twin peaks" and "big crater." However, the lander and rover are not discernible in part
because at the imaging range of about 497 miles (800 km), their size in the photograph is less than one pixel.
Despite this fact, the resolution of the current image still
exceeds the best photograph of Ares Valles taken during the Viking
Orbiter mission over twenty years ago. During mapping operations next year, the camera may have an opportunity to image the Pathfinder landing site again at ranges as low as 235 miles (378 km). In those images, small objects such as the lander and parachute may be visible.
The Viking 2 lander site at Utopia Planitia was also targeted by
the camera for observation. Unfortunately, clouds obscured the site during each one of the three attempts. Similar to the situation with the Pathfinder site, further attempts at imaging the Viking 2 site may occur next year during mapping operations.
Other experiments on the spacecraft have also been busy acquiring
data. Besides the camera, the laser altimeter, magnetometer, thermal emission spectrometer, and radio science investigation teams have also collected data since the beginning of April. These measurements include northern hemisphere topography by the laser, local and global magnetic properties by the magnetometer, atmosphere and mineralogy studies by the spectrometer, and atmosphere and gravity field experiments by the radio science team.
Of particular interest, Dr. David Smith's laser altimeter team has
been gathering data about the Martian north polar ice caps. On every orbit, the laser measures the cap's topography in order to calculate its thickness. In June, the ice cap's thickness will reach a maximum during the height of the northern winter season. Thickness measurements from April compared to those that will be taken in June will contribute toward a greater understanding of the Martian cap formation.
Although extremely successful, the flight team temporarily
suspended science operations on Tuesday in preparation for a month-long event called solar conjunction. Starting this weekend, communications with the spacecraft will degrade as Mars begins to pass behind the Sun's corona as viewed from the Earth. As a consequence, the radio signals sent to and from Surveyor will experience a noise effect from solar
electromagnetic interference. During the middle of the month, the Sun will directly eclipse the red planet and physically block radio
communications with the spacecraft.
Solar conjunction will end in late May as Mars moves out from
behind the Sun. At that time, the flight team will re-establish
commanding capability and resume science operations. Data collection will then continue until the restart of aerobraking on September 11th. The goal of this next phase of aerobraking will be to lower the current, highly elliptical, 11.6-hour orbit to a low, circular, two-hour mapping orbit by April 1999.
After a mission elapsed time of 540 days from launch, Surveyor is
229.36 million miles (369.12 million kilometers) from the Earth and in an orbit around Mars with a high point of 11,108 miles (17,877km), a low point of 108.3 miles (174.3 km), and a period of 11.6 hours. A special, multi-week solar conjunction command sequence is currently executing on the spacecraft, and all systems continue to perform as expected. The next status report will be released sometime late May.
Status report prepared by:
Office of the Flight Operations Manager
Mars Surveyor Operations Project
NASA Jet Propulsion Laboratory
California Institute of Technology
Pasadena, CA 91109
Reference: mayan-secrets.blogspot.com
