- Mars probe program
: "This article is for the Russian (Soviet) series of space probes; for the moon designated as Mars II, see
Deimos (moon) ; for all missions to Mars, seeExploration of Mars ."The Mars program was a series of Mars unmanned
lander s andorbiter s launched or attempted to launch by theSoviet Union in the 1960s-1970s.First generation - Marsnik design
The first Soviet attempts to send a probe to Mars were the 2 probes of the
Marsnik program with mass of about 650 kg, which failed during launch in 1960.cite web|url=http://nssdc.gsfc.nasa.gov/planetary/chronology_mars.html|title=Chronology of Mars Exploration|work=National Space Science Data Center|accessdate=2008-03-19]Second generation - Mars 3MV-4A design
Mars 1 was launched in 1962 but failed en route to Mars. Two other Soviet launches at around the same time,Mars 1962A andMars 1962B , were likely similar or identical spacecrafts of "Mars 3MV-4A" 900-kg design but both of these failed during launch and did not leave Earth orbit. In 1964 similarZond 1964A andZond 2 probes failed on the start and on the way to Mars again.Heavy third generation
The Mars 2 through Mars 7 launched spacecraft in 1971-1973 years, like failed on starts
Mars 1969A andMars 1969B in 1969 andMars 1971C in 1971, were of a new, heavy design, weighing approximately 5metric ton s and requiring the heavy Proton booster for launch. They were designed to deliver an orbiter and a lander to Mars. The orbiter design was similar to the later heavyVenera probes to Venus (Veneras 9 through the Vega probes to Venus andHalley's comet in 1985). The orbiter bus design was likely somewhat rushed into service and immature, considering that it performed very reliably in the Venera variant after 1975. This reliability problem was common to much Soviet space hardware from the late 1960s and early 1970s and was largely corrected with a deliberate policy of consolidating (or "debugging") existing designs rather than introducing new ones which was implemented in the mid-1970s.Mars 1969A, Mars 1969B of M-69 project
Mars 1971C, Mars 2 and 3 of M-71 project
The Mars 2 and Mars 3 missions consisted of identical spacecraft, each with an orbiter and an attached lander; they were the first human artifacts to touch down on Mars. The failed on start in May 5, 1971 Cosmos 419 (Mars 1971C), third spacecraft of project M-71, was orbiter only that intended to be first artificial satellite of Mars beating American
Mariner 8 (failed) andMariner 9 (successfull) martian orbiters. The orbiters' primary scientific objectives were to image the Martian surface and clouds, determine the temperature on Mars, study the topography, composition and physical properties of the surface, measure properties of the atmosphere, monitor thesolar wind and the interplanetary and Martianmagnetic field s, and act as communications relays to send signals from the landers to Earth. Mars 2 and 3 were launched by Tyazheliy Sputniks.Mars 1971C
Mars 2
*Launch Date/Time:
**Mars 2:May 19 1971 at 16:22:44 UTC
*Launch mass (including fuel):
**Combined: 4650 kg
**Orbiter: 3440 kg
**Lander: 1210 kg
*On-orbit dry mass: 2265 kg
*Dimensions: 4.1 meters tall, 2 meters across (5.9 meters across with solar panels deployed)Mars 2 released the descent module 4.5 hours before reaching Mars on
November 27 ,1971 . The descent module entered the Martian atmosphere at roughly 6.0 km/s at a steeper angle than planned. The descent system malfunctioned and the lander crashed at 45° S, 302° W, delivering the Soviet Union coat of arms to the surface. Meanwhile, the orbiter engine performed a burn to put the spacecraft into a 1380 x 24,940 km, 18 hour orbit about Mars with an inclination of 48.9 degrees. Scientific instruments were generally turned on for about 30 minutes nearperiapsis .Mars 3
*Launch Date/Time:
**Mars 3:May 28 1971 at 15:26:30 UTC
*Launch mass (including fuel):
**Combined: 4650 kg
**Orbiter: 3440 kg
**Lander: 1210 kg
*On-orbit dry mass: 2265 kg
*Dimensions: 4.1 meters tall, 2 meters across (5.9 meters across with solar panels deployed)Mars 3's descent module was released at 09:14 UT on
December 2 1971 , 4 hours 35 minutes before reaching Mars. The descent module entered the Martian atmosphere at roughly 5.7 km/s. Throughaerodynamic braking ,parachute s, andretrorocket s, the lander achieved a soft landing at 45° S, 158° W and began operations. However, after 20 seconds the instruments stopped working for unknown reasons, perhaps as a result of the massive surface dust storms raging at the time of landing. Mars 3 lander still managed to transmit a portion of the first picture of Martian surface. Meanwhile, the orbiter had suffered from a partial loss of fuel and did not have enough to put itself into a planned 25 hour orbit. The engine instead performed a truncated burn to put the spacecraft into a long 12 day, 19 hour period orbit about Mars with an inclination thought to be similar to that of Mars 2 (48.9 degrees).Both landers had a small Mars 'rover' on board, which would move across the surface on skis while connected to the lander with a 15-meter umbilical. Two small metal rods were used for autonomous obstacle avoidance, as radio signals from Earth would take too long to drive the rovers using remote control. Each rover had both a densitometer and a dynamic penetrometer, to test the density and the bearing strength of the soil. Because of the demise of the landers, neither rover saw action.
The Mars 2 and 3 orbiters sent back a large volume of data covering the period from December 1971 to March 1972, although transmissions continued through August. It was announced that Mars 2 and 3 had completed their missions by
22 August 1972 , after 362 orbits completed by Mars 2 and 20 orbits by Mars 3. The probes sent back a total of 60 pictures. The images and data enabled creation of surface relief maps, and gave information on the Martiangravity andmagnetic field s.Mars 4, 5, 6 and 7 of M-73 project
Mars 4, 5, 6, and 7 comprised an associated group of Soviet spacecraft launched towards Mars in July and August of 1973. The Mars 4 and 5 automatic stations were designed to orbit Mars and return information on the composition, structure, and properties of the Martian atmosphere and surface. The spacecraft were also designed to act as communications links to the Mars 6 and 7 landers. They were launched from Earth by Proton SL-12/D-1-e boosters.
The 1973 Mars launch window was inefficient and thus the
Proton rocket could not deliver the mass to Mars, as had been possible in 1971. Thus, the mission was split somewhat extravagantly into four separate, but lighter vehicles: two relay orbiters without landers and two orbiter type buses with landers but without fuel to enter orbit. The political purpose of these missions was to beat the American Viking probes (scheduled for 1975 launches) to be the first spacecraft to soft land on Mars, at which they did not succeed.Mars 4
*Launch Date/Time:
**Mars 4:July 21 1973 at 19:30:59 UTC
*On-orbit mass:
**Dry: 2270 kg
**Fully-fuelled: 3440 kgThe Mars 4 orbiter reached Mars on
10 February 1974 . Due to a flaw in thecomputer chip which resulted in degradation of the chip during the voyage to Mars, the retro-rockets designed to slow the craft into Mars orbit did not fire , and Mars 4 flew by the planet at a range of 2200 km. It returned one swath of pictures and some radio occultation data which constituted the first detection of the nightsideionosphere on Mars. It continued to return interplanetary data from solar orbit after the flyby.Mars 5
*Launch Date/Time:
**Mars 5:July 25 1973 at 18:55:48 UTC
*On-orbit mass:
**Dry: 2270 kg
**Fully-fuelled: 3440 kgMars 5 reached Mars on
February 12 1974 at 15:45 UT and was inserted into an elliptical 1755 by 32,555 km, 24 h 53 min orbit with an inclination of 35.3 degrees. Nearly synchronized with the rotation of the planet, its two phototelevision cameras could be commanded to take 12 pictures during each close approach. The "Vega" camera used a wide area 52mm lens with color filters, the "Zulfar" camera used a telescopic 350mm lens and long-pass orange filter. Images were transmitted in a rapid 220-line mode, and then selected pictures were retransmitted at 880 or 1760 line resolutioncite web | last=Mitchel |first=Don P | url=http://www.mentallandscape.com/C_CatalogMars.htm | title=Soviet Mars Images |work=Don P. Mitchell Homepage |accessdate=2007-03-28] . Mars 5 collected data for 22 orbits until a loss of pressurization in the transmitter housing ended the mission. About 60 images were returned over a nine day period showing swaths of the area south ofValles Marineris , from 5° N, 330° W to 20° S, 130° w.Mars 6
Mars 6 successfully lifted off on August 5, 1973, into an intermediate Earth orbit on a Proton SL-12/D-1-e booster and then launched into a Mars transfer trajectory. Total fueled launch mass of the lander and bus was 3260 kg. It reached Mars on
March 12 1974 . The descent module separated from the bus at a distance of 48,000 km from Mars. The bus continued on into a heliocentric orbit after passing within 1600 km of Mars. The descent module entered the atmosphere at 09:05:53 UT at a speed of 5.6 km/s. The parachute opened at 09:08:32 UT after the module had slowed its speed to 600 m/s byaerobraking . During this time the craft was collecting data and transmitting it directly to the bus for immediate relay to Earth. Contact with the descent module was lost at 09:11:05 UT in "direct proximity to the surface", probably either when the retrorockets fired or when it hit the surface at an estimated 61 m/s. Mars 6 landed at 23.90° S, 19.42° W in theMargaritifer Terra region of Mars. The landed mass was 635 kg. The descent module transmitted 224 seconds of data before transmissions ceased, the first data returned from theatmosphere of Mars . Unfortunately, much of the data were unreadable due to a flaw in a computer chip which led to degradation of the system during its journey to Mars.Mars 7
Mars 7 successfully lifted off on August 9, 1973, into an intermediate Earth orbit on a Proton SL-12/D-1-e booster and then launched into a Mars transfer trajectory. Total fueled launch mass of the lander and bus was 3260 kg. It reached Mars on
March 9 1974 . Due to a problem in the operation of one of the onboard systems (attitude control or retro-rockets) the landing probe separated prematurely (4 hours before encounter) and missed the planet by 1300 km. The early separation was probably due to a computer chip error which resulted from degradation of the systems during the trip to Mars. The intended landing site was 50° S, 28° W. The lander and bus continued on into heliocentric orbits.Cancelled superheavy designs and missions
Mars 4NM andMars 5NM projects intended by Soviet Union for heavy Marsokhod (in 1973 according to initial plan of 1970) and Mars sample return missions (planned to 1975) by launching on N1 superrocket that never flown successfully. [http://www.novosti-kosmonavtiki.ru/content/numbers/213/50.shtml] .Later design and missions
Phobos
spacecraft were launched in 1988 to study Mars and its moon Phobos. Phobos 1 failed due to an error in a command sent to the spacecraft. Phobos 2 gathered data and took photographs of Mars and Phobos from orbit. However, it failed before launching two Phobos landing probes.
Mars 96
Mars 96 was an orbiter launched in 1996 byRussia and not directly related to the Soviet series of probes.References
ee also
*
Exploration of Mars
*Space exploration
*Robotic spacecraft
*Marsnik program External links
* [http://www.mentallandscape.com/C_CatalogMars.htm catalog of Soviet Mars images]
* [http://nssdc.gsfc.nasa.gov/planetary/planets/marspage.html NASA's mars probe website]
* [http://solarsystem.nasa.gov/missions/profile.cfm?MCode=USSR_Mars Mars Series (USSR) Profile] by [http://solarsystem.nasa.gov NASA's Solar System Exploration]
* [http://www.strykfoto.org/mars4and5.htm Ted Stryk's page on the Mars 4-7 probes]
* (Wikisource )
* [ftp://ftp.seds.org/pub/info/newsletters/ejasa/1989/jasa8910.txt "The Rocky Soviet Road to Mars" by Larry Klaes - EJASA October, 1989]
* [http://klabs.org/richcontent/Reports/mars/difficult_road_to_mars.pdf "The Difficult Road to Mars" By V. G. Perminov]
Wikimedia Foundation. 2010.