Ranger program
The Ranger program was a series of
unmanned space missions by the
United States in the 1960s whose objective was to obtain the first close-up images of the surface of the
Moon. The Ranger spacecraft were designed to collide with the lunar surface, returning imagery until they were destroyed upon impact.
Ranger was originally designed, beginning in 1959, in three distinct phases, called "blocks." Each block had different mission objectives and progressively more advanced system design. The
JPL mission designers planned multiple launches in each block, to maximize the engineering experience and scientific value of the mission and to assure at least
Encyclopedia
The
Ranger program was a series of
unmanned space missions by the
United States in the 1960s whose objective was to obtain the first close-up images of the surface of the
Moon. The Ranger spacecraft were designed to collide with the lunar surface, returning imagery until they were destroyed upon impact.
Ranger was originally designed, beginning in 1959, in three distinct phases, called "blocks." Each block had different mission objectives and progressively more advanced system design. The
JPL mission designers planned multiple launches in each block, to maximize the engineering experience and scientific value of the mission and to assure at least
one successful flight.
Total research, development, launch, and support costs for the Ranger series of spacecraft was approximately $170 million.
Block 1 missions
Block 1, consisting of two spacecraft launched into Earth orbit in 1961, was intended to test the
Atlas/
Agena launch vehicle and spacecraft equipment without attempting to reach the Moon.
Most elements of spacecraft technology taken for granted today were untested before Ranger. Perhaps the most important of these was three-axis attitude stabilization, meaning that the spacecraft is fixed in relation to space instead of being stabilized by spinning. This would permit pointing large solar panels at the Sun, a large antenna at Earth, and cameras and other directional scientific sensors at their appropriate
targets. Rocket propulsion carried aboard the spacecraft was another critically important new technology, needed for accurate targeting at the Moon or distant planets.
In addition, two-way communication and closed-loop tracking, requiring spacecraft and ground system development, and the use of on-board computing and sequencing combined with commands from the ground, all had to be developed and tried out in flight. Unfortunately, problems with the early version of the launch vehicle left
Ranger 1 and
Ranger 2 in short-lived, low-Earth orbits in which the spacecraft could not stabilize themselves, collect solar power, or survive for long. In 1962, JPL utilized the Ranger 1 & 2 design for the failed
Mariner 1 and successful
Mariner 2 deep-space probes to
Venus.
Block 2 missions
Block 2 of the Ranger project launched three spacecraft to the Moon in 1962, carrying a TV camera, a radiation detector, and a seismometer in a separate capsule slowed by a rocket motor and packaged to survive its low-speed impact on the Moon’s surface. The three missions together demonstrated good performance of the Atlas/Agena B launch vehicle and
the adequacy of the spacecraft design, but unfortunately not all on the same attempt.
Ranger 3 was launched into deep space, but an
inaccuracy put it off course and it missed the Moon entirely.
Ranger 4 had a perfect launch, but the spacecraft was completely disabled. The project team tracked the seismometer capsule to impact just out of
sight on the lunar far side, validating the communications and navigation system.
Ranger 5 missed the Moon and was disabled. No significant science information was gleaned from these missions. The craft weighed 331 kg.
Block 3 missions
Ranger's Block 3 embodied four launches in 1964-65. These spacecraft boasted a television instrument designed to observe the lunar surface during the approach; as the spacecraft neared the Moon, they would reveal detail smaller than the best Earth telescopes could show, and finally details down to dishpan size. The first of the new series,
Ranger 6, had a flawless flight, except that the television system was disabled by an in-flight accident and could take no pictures.
The next three Rangers, with a redesigned television, were completely successful.
Ranger 7 photographed its way down to target in a lunar plain, soon named Mare Cognitum, south of Copernicus crater. It sent more than 4,300 pictures from six cameras to waiting scientists and engineers. The new images revealed that craters caused by impact were the dominant features of the Moon's surface, even in the seemingly smooth and empty plains. Great craters were marked by small ones, and the small with tiny impact pockmarks, as far down in size as could be discerned -- about 50 centimeters . The light-colored streaks radiating from Copernicus and a few other large craters turned out to be chains and nets of small craters and debris blasted out in the primary impacts.
In February 1965,
Ranger 8 swept an oblique course over the south of
Oceanus Procellarum and
Mare Nubium, to crash in
Mare Tranquillitatis where
Apollo 11 would land 4½ years later. It garnered more than 7,000 images, covering a wider area and reinforcing the conclusions from Ranger 7. About a month later,
Ranger 9 came down in the 90 km diameter crater Alphonsus. Its 5,800 images, nested concentrically and taking advantage of very low-level sunlight, provided strong confirmation of the crater-on-crater, gently rolling contours of the lunar surface.
Thus, after a long trouble-plagued start that taught the system engineers a great deal and the scientists virtually nothing, Project Ranger finished with three flights that greatly advanced the lunar scientists' knowledge of the surface and whetted their appetites for a closer look.
The Ranger spacecraft
Each Ranger spacecraft had 6 cameras on board. The cameras were fundamentally the same with differences in exposure times, fields of view, lenses, and scan rates. The camera system was divided into two channels, P and F . Each channel was self-contained with separate power supplies, timers, and transmitters. The F-channel had 2 cameras: the wide-angle A-camera and the narrow angle B-camera. The P-channel had four cameras: P1 and P2 and P3 and P4 . The final F-channel image was taken between 2.5 and 5 s before impact and the last P-channel image 0.2 to 0.4 s before impact . The images provided better resolution than was available from Earth based views by a factor of 1000.
Total research, development, launch, and support costs for the Ranger series of spacecraft was approximately $170 million.
Mission list
- Block 1
- Ranger 1, launched 23 August 1961, lunar prototype, launch failure
- Ranger 2, launched 18 November 1961, lunar prototype, launch failure
- Block 2
- Ranger 3, launched 26 January 1962, lunar probe, spacecraft failed, missed moon
- Ranger 4, launched 23 April 1962, lunar probe, spacecraft failed, impact
- Ranger 5, launched 18 October 1962, lunar probe, spacecraft failed, missed
- Block 3
- Ranger 6, launched 30 January 1964, lunar probe, impact, cameras failed
- Ranger 7
- Launched 28 July 1964
- Impacted Moon 31 July 1964 at 13:25:49 UT
- Latitude 10.35 S, Longitude 339.42 E - Mare Cognitum
- Ranger 8
- Launched 17 February 1965
- Impacted Moon 20 February 1965 at 09:57:37 UT
- Latitude 2.67 N, Longitude 24.65 E - Mare Tranquillitatis
- Ranger 9
- Launched 21 March 1965
- Impacted Moon 24 March 1965 at 14:08:20 UT
- Latitude 12.83 S, Longitude 357.63 E - Alphonsus crater
External links
Both links lead to a whole book on the program. For the HTML one, scroll down to see the table of contents link.
See also
