Hubble Space Telescope Primer for Cycle 11

2.1 Hubble Space Telescope Operations

---

The Hubble Space Telescope is a cooperative project of the National Aeronautics and Space Administration (NASA) and the European Space Agency (ESA) to operate a long-lived space-based observatory for the benefit of the international astronomical community. HST was first dreamt of in the 1940s, and designed and built in the 1970s and 80s. In April 1990 the Space Shuttle Discovery deployed it in low-Earth orbit (~600 kilometers). The initial complement of Scientific Instruments (SIs) was:

• The Fine Guidance Sensors (FGSs).
• The Faint Object Camera (FOC).
• The Faint Object Spectrograph (FOS).
• The Goddard High Resolution Spectrograph (GHRS).
• The High Speed Photometer (HSP).
• The Wide Field and Planetary Camera (WF/PC).

Soon after deployment it was discovered that the primary mirror suffers from spherical aberration, which limited the quality of HST data obtained in the first few years of operation.

2.1.1 Servicing Mission SM1

During servicing mission SM1 in December 1993, Space Shuttle astronauts successfully refurbished HST. They replaced the HSP with COSTAR, a corrective optics package. COSTAR's reflecting optics were deployed into the optical paths of the FOC, FOS and GHRS, which removed the effects of the primary mirror's spherical aberration. The performance of the FGSs was unaffected by COSTAR. The WF/PC was replaced by a new instrument:

• The Wide Field and Planetary Camera 2 (WFPC2).

The WFPC2 contains its own internal optics to correct the spherical aberration.

The astronauts also installed new solar arrays. This resolved the problem of the thermal vibrations of the old arrays during day/night transitions, which had affected the telescope's pointing performance.

2.1.2 Servicing Mission SM2

During servicing mission SM2 in February 1997, astronauts replaced the FOS and the GHRS with two new instruments:

• The Near Infrared Camera and Multi-Object Spectrometer (NICMOS).
• The Space Telescope Imaging Spectrograph (STIS).

Also, FGS-1 was replaced with an enhanced FGS, called FGS1R. FGS1R has an adjustable fold flat mirror, which is commandable from the ground. This enables realignment in the FGS optical path to lessen the effects of the primary mirror's spherical aberration. As a result, the astrometric performance of FGS1R significantly exceeds that of the original FGS.

2.1.3 Servicing Missions SM3A and SM3B

HST has six rate-sensing gyroscopes on board; three of these gyroscopes must be in working order to maintain accurate pointing. In the years after SM2, gyroscopes failed at a higher than expected rate, ultimately leading to a halt of HST observing in November 1999. In anticipation of this event, servicing mission SM3, which had been in planning for several years, was split into two separate missions: SM3A and SM3B.

2.1.4 Servicing Mission SM3A

In December 1999 Space Shuttle astronauts lifted off for servicing mission SM3A. Six new gyroscopes were successfully installed, which allowed HST to resume normal operations.

Along with the gyro replacements, the HST Project used this "unplanned" mission to make other planned upgrades and refurbishments:

1. Voltage/temperature Improvement Kits (VIKs) were installed to help regulate battery recharge voltages and temperatures.
2. The original DF224 spacecraft computer was replaced by a 486 upgrade, which provides a significant improvement in onboard computing power.
3. The FGS2 was replaced by a refurbished fine guidance sensor FGS2R, to enhance the performance of the pointing and control system (see Section 2.1.2).
4. The remaining tape recorder was replaced by a second Solid State Recorder (SSR), and a new transmitter was installed to replace one that had failed.

All of the upgrades have undergone successful in-orbit verification and calibration and the observatory's functionality has been completely restored.

2.1.5 Servicing Mission SM3B

The next servicing mission SM3B is currently anticipated to occur sometime in the Mid January 2002 time frame. During this mission, astronauts will replace the FOC with a new instrument:

• The Advanced Camera for Surveys (ACS).

Also, the astronauts will install the NICMOS Cooling System (NCS) to allow further use of NICMOS, which had exhausted its cryogen in January 1999. Installation of new solar arrays, along with various other engineering upgrades, including an orbit reboost, will also be performed. Basic capabilities of the newly installed ACS and the revived NICMOS are expected to be ready for scientific use about eight weeks following the servicing mission.

2.1.6 Servicing Mission SM4

In the final servicing mission SM4, currently planned for late 2003, Space Shuttle astronauts will replace COSTAR and WFPC2 with the last two instruments that are planned for use on HST:

• The Cosmic Origins Spectrograph (COS).
• The Wide Field Camera 3 (WFC3).

The Aft-Shroud Cooling System (ASCS), which will provide enhanced thermal control for the axial instruments, will also be installed.