Explorer 27
 Depiction of Explorer 27 in orbit | |
| Names | BE-C Beacon Explorer-C Beacon-C NASA S-66C |
|---|---|
| Mission type | Ionospheric research |
| Operator | NASA |
| COSPAR ID | 1965-032A |
| SATCATno. | 01328 |
| Mission duration | 59 years, 2 months and 14 days (in orbit) |
| Spacecraft properties | |
| Spacecraft | Explorer XXVII |
| Bus | Beacon Explorer |
| Manufacturer | Johns Hopkins University Applied Physics Laboratory |
| Launch mass | 60.8 kg (134 lb) |
| Dimensions | 30 × 45 cm (12 × 18 in) |
| Power | 4 deployablesolar arraysandbatteries |
| Start of mission | |
| Launch date | 29 April 1965, 14:17:00GMT |
| Rocket | Scout X-4(S-136R) |
| Launch site | Wallops Flight Facility, |
| Contractor | Vought |
| Entered service | 29 April 1965 |
| End of mission | |
| Last contact | 20 July 1973 |
| Orbital parameters | |
| Reference system | Geocentric orbit[1] |
| Regime | Low Earth orbit |
| Perigee altitude | 927 km (576 mi) |
| Apogee altitude | 1,320 km (820 mi) |
| Inclination | 41.10° |
| Period | 107.70 minutes |
| Instruments | |
| Langmuir probes Laser Tracking Reflectors Radio Beacon Radio Doppler System | |
Explorer program | |
Explorer 27(orBE-CorBeacon Explorer-C,Beacon-CorS-66C) was a smallNASAsatellite, launched in 1965, designed to conduct scientific research in theionosphere.[2]It was powered by 4solar panels.One goal of the mission was to study in detail the shape of theEarthby way of investigating variations in its gravitational field.[3]It was the third and last of the Beacons in theExplorers program.The satellite was shut off in July 1973 so that its transmission band could be used by higher-priority spacecraft.[2]
Spacecraft[edit]
Built at theApplied Physics Laboratory(APL),[5]under the direction ofGoddard Space Flight Center,[4]Explorer 27 began as S-66C, the last of the five satellites in NASA's first stage of ionospheric exploration, and the first of five NASA geodetic satellites.[6]: 346 Its primary mission was "to conduct ionospheric measurements on a worldwide basis. The program will determine thetotal electron contentof a vertical cross-section of the ionosphere located between the satellite and the Earth. Accomplishing this objective will aid in establishing the behavior pattern of the ionosphere as a function of latitude, time of day, season, and solar cycle ".[4]
Weighing 60.8 kg (134 lb), the satellite was an octagonal spacecraft with a honeycombnylonandfiberglasshull, 45 cm (18 in) in diameter, 30 cm (12 in) high, with four solar panels 25 cm (9.8 in) wide and 170 cm (67 in) long.[4]
A three-axismagnetometerand Sun sensors provided information on the satellite attitude and spin rate.[7]There was notape recorderaboard so that satellite could be received only when the satellite was within range of a groundtelemetrystation. ContinuousDopplertransmitters operated at 162MHzand 324-MHz to permit precise tracking byTransittracking stations for navigation and geodetic studies.[2]Four other transmitters operated on 20, 40, 41, and 360-MHz to measure ionospheric density. Explorer 27's last experiment was an Electron Density Experiment designed for measuring charged particles in the immediate vicinity of the satellite.[4]
S-66 mounted 360 25 mm (0.98 in) "cube corner"retroreflectorsmade offused silica,[4]so that the satellite could be tracked via lasers beamed from mobile stations atWallops Flight Facility(WFF).[6]: 346 [8]
History[edit]
The first S-66 was scheduled for launch in late 1963. However, due to problems with theScout X-4,[4]the flight was rescheduled for the following year on aDelta B,fromCape CanaveralLC-17A.[9]On 19 March 1964, the first attempt to this S-66 ended in failure when the third stage of its Deltalaunch vehicleburned just 22 seconds instead of the programmed 40 seconds. This was only the second time the Delta launch vehicle had failed, and the incident followed 22 prior successes.[6]: 109
A second S-66 was launched, this time successfully, via a Scout X-4 launch vehicle at 03:01GMT,on 9 October 1964, from thePALC-Dlaunch facility atVandenberg Air Force Base.Once in space, it became known as Explorer 22.[9]Explorer 22's as-yet unnamed backup was scheduled for launch in March/April 1965 to extend the geodetic experiments of its predecessor.[10]Upon the backup's launch on 29 April 1965 at 14:17:00 GMT viaScout X-4fromWallops Island,this third S-66 satellite was designated Explorer 27.[9]
Experiments[edit]
Langmuir Probes[edit]
Two cylindrical electrostatic probes of theLangmuir probetype were used. They consisted of a collector electrode extending from the central axis of a cylindrical guard ring. The guard ring extended 5 cm (2.0 in) from the spacecraft and the probe extended 23 cm (9.1 in). A 2-Hzsawtooth voltage of -3 to +5voltswas swept to either of the probes, and the resulting current profile to the probe was telemetered. From this profile, theelectron density,electron temperature,and meanionmass were determined. This experiment performed nominally from launch until 13 August 1968, when solar cell degradation resulting from radiation prevented operation of all systems on the satellite. The probe was not operated after that time. No archival data were produced since the experiment was a back-up for theExplorer 22(BE-B) mission, which had been flown successfully.[11]
Laser Tracking Reflectors[edit]
The passive optical laser experiment, which consisted of nine panels on the spacecraft, was used to determine the spacecraft range and angle. Each panel was covered with 40quartzcube-corner prismsthat provided laser tracking capabilities for optical tracking studies. The ground-based optical transmitter was a pulsed 1-msruby laser.Aphotodetectordetermined whether the laser beam interrupted the spacecraft.[12]
Radio Beacon[edit]
A radio beacon radiated a plane-polarized signal at 20.005 MHz, 40.010 MHz, 41.010 MHz, and 360.090 MHz, all harmonics of 1.00025 MHz. The plane of polarization of the three lower frequencies underwent an appreciable number of rotations due to electron concentration. The polarization plane of highest frequency did not rotate appreciably. Several methods were used to analyze these rotations and determine the total electron content between the satellite and a ground receiver. The beacons were on until the satellite operation terminated on 6 May 1968. On 13 February 1970, the beacons were again turned on to replace the Explorer 22 (1964-064A - BE-B) beacons which had completely failed by the end of January 1970.[13]
Radio Doppler System[edit]
Two coherent, unmodulated CW transmitters, operating on frequencies of 162 and 324 MHz, allowed the Tranet Doppler Network to obtain data for studies of dynamicgeodesy.The frequencies were generated from redundant, dual, ultra-stable crystal oscillators operating on a frequency of 5 MHz minus 80 ppm. The system operated as planned.[14]
Results[edit]
Explorer 27 was turned off on 20 July 1973 because it was interfering with other, more important satellites. Tracking of the satellite via its passive laser reflectors continued at least into the 21st century.[15]
See also[edit]
References[edit]
- ^"Trajectory: Explorer 27 (BE-C) 1965-032A".NASA. 28 October 2021.Retrieved8 November2021.
This article incorporates text from this source, which is in thepublic domain.
- ^abc"Display: Explorer 27 (BE-C) 1965-032A".NASA. 28 October 2021.Retrieved8 November2021.This article incorporates text from this source, which is in thepublic domain.
- ^"Explorer Series of Spacecraft".NASA.Retrieved12 April2018.
- ^abcdefgTysdal, R. M. (October 1964)."Environmental test program of the beacon explorer spacecraft"(PDF).NASA.Retrieved23 October2019.
- ^Brian Harvey (24 November 2017).Discovering the Cosmos with Small Spacecraft: The American Explorer Program.Springer. pp. 91–.ISBN978-3-319-68140-5.
- ^abcEmme, E. M. (January 1965)."Astronautics and Aeronautics, 1964"(PDF).NASA.Retrieved23 October2019.This article incorporates text from this source, which is in thepublic domain.
- ^Ludwig Combrinck, 2010. Sciences of Geodesy (Cap. 9)Springer-VerlagRetrieved June 9, 2018
- ^Vonbun, F. O. (1977)."Goddard laser systems and their accuracies".Philosophical Transactions of the Royal Society.284(1326). London: McGraw Hill Publishing Company: 443–444.Bibcode:1977RSPTA.284..443V.doi:10.1098/rsta.1977.0017.hdl:2060/19760015443.S2CID122709982.Retrieved21 October2019.
- ^abcMcDowell, Jonathan (21 July 2021)."Launch Log".Jonathan's Space Report.Retrieved8 November2021.
- ^"Beacon Explorer Surveys Ionosphere".Aviation Week and Space Technology.19 October 1964. p. 35.Archivedfrom the original on 30 October 2019.Retrieved21 October2019.
- ^"Experiment: Langmuir Probes".NASA. 28 October 2021.Retrieved7 November2021.This article incorporates text from this source, which is in thepublic domain.
- ^"Experiment: Laser Tracking Reflectors".NASA. 28 October 2021.Retrieved7 November2021.This article incorporates text from this source, which is in thepublic domain.
- ^"Experiment: Radio Beacon".NASA. 28 October 2021.Retrieved7 November2021.This article incorporates text from this source, which is in thepublic domain.
- ^"Experiment: Radio Doppler System".NASA. 28 October 2021.Retrieved7 November2021.This article incorporates text from this source, which is in thepublic domain.
- ^"Beacon-C".International Laser Ranging Service.Retrieved8 November2021.This article incorporates text from this source, which is in thepublic domain.
