Kosmos 27 Explained

Kosmos 27
Mission Type:Venus impact probe
Operator:OKB-1
Cospar Id:1964-014A
Satcat:00770
Spacecraft Type:3MV-1
Manufacturer:OKB-1
Dry Mass:948 kg
(including an impact
probe of 285 kg)
Launch Mass:6520 kg[1]
Launch Date:27 March 1964, 03:24:43 GMT
Launch Rocket:Molniya 8K78
s/n T15000-27
Launch Site:Baikonur, Site 1/5
Launch Contractor:OKB-1
Decay Date:28 March 1964
Orbit Epoch:27 March 1964
Orbit Reference:Geocentric[2]
Orbit Regime:Low Earth
Orbit Periapsis:167 km
Orbit Apoapsis:198 km
Orbit Inclination:64.8°
Orbit Period:88.7 minutes
Apsis:gee
Programme:Venera
Previous Mission:Venera 3MV-1 No.2
Next Mission:Venera 2

Kosmos 27 (Russian: Космос 27 meaning Cosmos 27), also known as Zond 3MV-1 No.3 was a space mission intended as a Venus impact probe. The spacecraft was launched by a Molniya 8K78 carrier rocket from Baikonur. The Blok L stage and probe reached Earth orbit successfully, but the attitude control system failed to operate.[3]

Launch

Kosmos 27 was launched at 03:24:43 GMT on 27 March 1964, atop a Molniya 8K78 s/n T15000-27 carrier rocket flying from Site 1/5 at the Baikonur Cosmodrome.

Spacecraft

Kosmos 27 was a "third-generation" deep space planetary probes of the 3MV series of the Soviet Union. The Soviet engineers planned four types of the 3MV, the 3MV-1 (for Venus impact), 3MV-2 (for Venus flyby), 3MV-3 (for Mars impact), and 3MV-4 (for Mars flyby). The primary difference over the second-generation was vastly improved (and in many cases doubled) orientation system elements as well as improved onboard propulsion systems. While these four versions were meant to study Mars and Venus.[4]

Mission

The probe was the first dedicated 3MV spacecraft that the Soviets launched (earlier missions had been of the test "Object-Probe" versions as Kosmos 21). It was designed to accomplish atmospheric entry into Venus followed by descent and impact. On 27 March 1964, it had a perigee of 167km (104miles) and an apogee of 198km (123miles), with an inclination of 64.8° and an orbital period of 88.7 minutes. The spacecraft successfully reached Earth orbit but failed to leave for Venus when the Blok L upper stage malfunctioned. The upper stage lost stable attitude due to a failure in the circuit of the power supply circuit that powered the valves for the attitude control system; hence, the stage remained uncontrollable and not ready to initiate a burn to leave Earth orbit. The problem was traced to a design error, the examination of telemetry data found that the failure was due to a design flaw in the circuitry of the BOZ unit, which resulted in power not being transferred to the attitude control jets on the Blok L stage, rather than one related to quality control. The spacecraft burned up in Earth's atmosphere the following day, on 28 March 1964. If successful, this mission would have been given a "Venera" designation.[4]

See also

Notes and References

  1. https://nssdc.gsfc.nasa.gov/nmc/spacecraft/display.action?id=1964-014A - 27 February 2020
  2. https://nssdc.gsfc.nasa.gov/nmc/spacecraft/displayTrajectory.action?id=1964-014A - 27 February 2020
  3. Web site: Wade. Mark . Venera 3MV-1. https://web.archive.org/web/20020227125252/http://www.astronautix.com/craft/vena3mv1.htm. 2002-02-27 . Encyclopedia Astronautica. dead. 17 February 2017.
  4. Book: Beyond Earth: A Chronicle of Deep Space Exploration, 1958–2016. https://web.archive.org/web/20190424211923/https://www.nasa.gov/sites/default/files/atoms/files/beyond-earth-tagged.pdf . 2019-04-24 . live . 58. Siddiqi. Asif A.. 2017059404. 9781626830424. NASA History Program Office. second. 2018 . SP2018-4041. The NASA history series. Washington, D.C..