Geotail is a satellite observing the Earth's magnetosphere. It was developed by Japan's ISAS in association with the United States' NASA, and was launched by a Delta II rocket on 24 July 1992 from Cape Canaveral Air Force Station.
![]() Geotail satellite (artist's concept) | |
Mission type | Earth observation |
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Operator | ISAS / NASA |
COSPAR ID | 1992-044A ![]() |
SATCAT no. | 22049 |
Website | www |
Mission duration | 20 years (planned) 30 years, 3 months, 21 days (in progress) |
Spacecraft properties | |
Launch mass | 980 kg (2,160 lb) |
Power | 273.0 watts |
Start of mission | |
Launch date | 24 July 1992, 14:26:00 (1992-07-24UTC14:26Z) UTC |
Rocket | Delta II 6925 |
Launch site | Cape Canaveral LC-17A |
Orbital parameters | |
Reference system | Geocentric |
Regime | HEO |
Semi-major axis | 127,367.75 km (79,142.65 mi)[1] |
Eccentricity | 0.5469845[1] |
Perigee altitude | 51,328 km (31,894 mi)[1] |
Apogee altitude | 190,664 km (118,473 mi)[1] |
Inclination | 10.51 degrees[1] |
Period | 7539.86 minutes[1] |
Epoch | 15 January 2015, 13:40:53 UTC[1] |
The primary purpose of this mission is to study the structure and dynamics of the tail region of the magnetosphere with a comprehensive set of scientific instruments. For this purpose, the orbit has been designed to cover the magnetotail over a wide range of distances: 8 REarth to 210 REarth from the earth. This orbit also allowed it to study the boundary region of the magnetosphere as it skims the magnetopause at perigees. In the first two years the double lunar swing-by technique was used to keep apogees in the distant magnetotail. This involved 14 lunar flybys.[2]
In 1993 the computer that controls the Low Energy Particles experiment locked up.[2] Attempts to reset it failed.[2] This problem was solved by changing the trajectory of the craft during a lunar flyby that took place on 26 September 1993 so that it passed through the shadow of the moon.[2] Power from the batteries was cut while this took place.[2] When the craft left the shadow of the moon, power returned and the computer started working again.[2]
The apogee was lowered down to 50 REarth in mid November 1994 and then to 30 REarth in February 1995 in order to study substorm processes in the near-Earth tail region. The present orbit is 9 REarth × 30 REarth with inclination of -7° to the ecliptic plane."
Geotail instruments studied electric fields, magnetic fields, plasmas, energetic particles, and plasma waves.[3]
In 1994 the principal investigator of the Plasma Wave Instrument (PWI), the experiment complement, was Professor Hiroshi Matsumoto of Kyoto University, with co-investigators from NASA, the University of Iowa, and STX Corporation.[4] Geotail is an active mission as of 2021[update].[5] Geotail, WIND, Polar, SOHO, and Cluster were all part of the International Solar-Terrestrial Physics Science Initiative (ISTP) project.[5]
In June of 2022, the second and final of Geotails two data recorders failed, jeopardizing future science if it cannot be brought back online. [6]
Geotail data has been used to show that flux transfer events move faster than the ambient medium through the Magnetosphere.[7] Those within the Magnetosheath were shown to move both faster and slower than the ambient medium.[7]
During the lunar flybys Geotail identified oxygen, silicon, sodium and aluminium in the lunar atmosphere.[2]
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Private miniaturized satellites |
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Reconnaissance |
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Magnetospherics | |
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Submagnetosphere |
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Earth's magnetosphere |
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Solar wind |
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Other magnetospheres |
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← 1991 · Orbital launches in 1992 · 1993 → | |
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Launches are separated by dots ( • ), payloads by commas ( , ), multiple names for the same satellite by slashes ( / ). Cubesats are smaller. Crewed flights are underlined. Launch failures are marked with the † sign. Payloads deployed from other spacecraft are (enclosed in parentheses). |
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