| Mission type | Venus impact probe |
|---|---|
| Operator | OKB-1 |
| COSPAR ID | 1964-014A |
| SATCAT no. | 00770 |
| Spacecraft properties | |
| Spacecraft type | 3MV-1 |
| Manufacturer | OKB-1 |
| Launch mass | 6520 kg[1] |
| Dry mass | 948 kg (including an impact probe of 285 kg)[2] |
| Start of mission | |
| Launch date | 27 March 1964, 03:24:43 GMT |
| Rocket | Molniya 8K78 s/n T15000-27 |
| Launch site | Baikonur, Site 1/5 |
| Contractor | OKB-1 |
| End of mission | |
| Decay date | 28 March 1964 |
| Orbital parameters | |
| Reference system | Geocentric[3] |
| Regime | Low Earth |
| Perigee altitude | 167 km |
| Apogee altitude | 198 km |
| Inclination | 64.8° |
| Period | 88.7 minutes |
| Epoch | 27 March 1964 |
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.[4]
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.[2]
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 167 kilometres (104 mi) and an apogee of 198 kilometres (123 mi), 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.[2]
See also
References
- ↑ https://nssdc.gsfc.nasa.gov/nmc/spacecraft/display.action?id=1964-014A - 27 February 2020
- 1 2 3 Siddiqi, Asif A. (2018). Beyond Earth: A Chronicle of Deep Space Exploration, 1958–2016 (PDF). The NASA history series (second ed.). Washington, D.C.: NASA History Program Office. p. 58. ISBN 9781626830424. LCCN 2017059404. SP2018-4041. Archived (PDF) from the original on 24 April 2019.
- ↑ https://nssdc.gsfc.nasa.gov/nmc/spacecraft/displayTrajectory.action?id=1964-014A - 27 February 2020
- ↑ Wade, Mark. "Venera 3MV-1". Encyclopedia Astronautica. Archived from the original on 27 February 2002. Retrieved 17 February 2017.