PROCYON explained

PROCYON
Mission Type:Asteroid flyby, technology demonstration
Operator:University of Tokyo / JAXA
Cospar Id:2014-076D
Launch Mass:Total: 67kg (148lb)
Dry Mass:64.5kg (142.2lb)
Dimensions:0.55xx
Power:25
Launch Rocket:H-IIA 202
Launch Site:LA-Y, Tanegashima Space Center
Interplanetary:
Type:flyby
Arrival Date:3 December 2015
Type:flyby
Arrival Date:Intended: 2016
Apsis:apsis
Previous Mission:Hodoyoshi 4
Next Mission:EQUULEUS

PROCYON (Proximate Object Close flyby with Optical Navigation) was an asteroid flyby space probe that was launched together with Hayabusa2 on 3 December 2014 13:22:04 (JST). It was developed by University of Tokyo and JAXA.It was a small (70 kg, approx. 60 cm cube), low cost spacecraft.[1]

It was intended to flyby the asteroid in 2016,[2] but the plan was abandoned due to the malfunction of the ion thruster.

Mission overview

PROCYON was launched as secondary payload together with the Hayabusa2 asteroid landing probe. After separation from the carrier rocket, PROCYON was left on a heliocentric orbit. On 22 February 2015, the ion engine was started, with the intention of adjusting the orbit so that an Earth flyby in December 2015 would direct the probe towards asteroid .[3] Initial results were favourable - the engine delivered 330 μN of thrust rather than the designed 250 μN - but the engine failed on 10 March and could not be restarted; PROCYON flew past Earth on 3 December 2015, but was unable to make a controlled orbit change. Shortly after the Earth flyby, contact with the spacecraft was lost.[4]

The 70 kg spacecraft had a specific impulse of 1000 seconds, for a delta-V budget of about 500 ms−1; the intention was to use 20% of the xenon propellant for the initial orbit correction, and the rest of the propellant between the Earth flyby and the asteroid flyby to ensure a controlled flyby distance of 30 km.[5]

A novel subsystem tested by PROCYON involved feeding both the main ion engine and the eight attitude control cold-gas thrusters from the same tank (containing 2.5 kg of xenon at launch)

Instruments

Science results

PROCYON observed the Lyman-alpha emission of comet 67P/Churyumov–Gerasimenko to determine its overall coma structure.[7] PROCYON captured the first complete image of the geocorona, confirming for the first time that it has north-south symmetry.[8]

See also

External links

Notes and References

  1. Web site: http://mainichi.jp/select/news/20150509k0000m040022000c.html . ja:プロキオン:小惑星への接近観測断念 . . 8 May 2015 . 8 May 2015 . dead . https://web.archive.org/web/20150518083332/http://mainichi.jp/select/news/20150509k0000m040022000c.html . 18 May 2015 .
  2. Web site: http://senews.jp/satellite/2015/04/07/528 . ja:超小型探査機「PROCYON」 二重小惑星を目指して航行中 . Very Small Probe PROCYON Cruising Toward a Binary Asteroid . Space Elevator News . 7 April 2015 . 7 April 2015 . https://web.archive.org/web/20170316141240/http://senews.jp/satellite/2015/04/07/528 . 16 March 2017 . dead .
  3. Web site: Low-thrust trajectory design and operations of PROCYON, the first deep-space micro spacecraft.
  4. Web site: On the situation of ultra small deep space explorer "PROCYON (Proquion)". ISAS (Institute of Space and Astronautical Science). 23 March 2018.
  5. Web site: 50kg- class Deep Space Exploration Technology Demonstration Micro-spacecraft PROCYON. digitalcommons.edu.
  6. Web site: http://www.space.t.u-tokyo.ac.jp/nlab/PROCYON_public_jp_150115.pdf . ja:超小型深宇宙探査機 PROCYON(プロキオン) . PROCYON development team . ja . 14 May 2015.
  7. Web site: Micro spacecraft investigates cometary water mystery . National Astronomical Observatory of Japan . 24 January 2017 . 26 January 2017.
  8. Ecliptic North‐South Symmetry of Hydrogen Geocorona . Geophysical Research Letters . 44 . 23 . 11,706–11,712 . 9 November 2017 . 10.1002/2017GL075915 . Kameda . S. . Ikezawa . S. . Sato . M. . Kuwabara . M. . Osada . N. . Murakami . G. . Yoshioka . K. . Yoshikawa . I. . Taguchi . M. . Funase . R. . Sugita . S. . Miyoshi . Y. . Fujimoto . M. . 2017GeoRL..4411706K . free .