| James S. Aber |
| Early photography | Shuttle photography |
| Space station | References |
Systematic manned space photography was undertaken during the Skylab missions of 1973 and 1974. Skylab was a orbiting space station that was utilized for extended Earth observations (Wilmarth et al. 1977). The overall objectives were to determine the quality and quantity of photographic and observational data that could be collected by astronauts with benefit from preflight training and ground support during flight. It was recognized that astronauts needed much additional preflight scientific and operational training to take multidisciplinary photographs (Wilmarth et al. 1977). Skylab 4 was most successful; about 2000 photographs were obtained of more than 850 features and phenomena. The lessons learned during Skylab missions formed the basis for the program of space-shuttle photography in the 1980s and '90s.

See MRS--Platform, Skylab.
| Near vertical | View straight down to Earth's surface. |
| Low oblique | View toward side--horizon not visible. |
| High oblique | View toward side--horizon visible. |
Space-shuttle photography is the result of systematic Earth and environmental science training given to each astronaut crew prior to flight. Much of the photography consists of revisits to targets previously photographed. Each day during flight, astronauts are given instructions for photographs based on cloud-cover and orbital conditions. Astronauts are also free to take photographs of any interesting or attractive scenes. Special advantages of astronaut photography include (Lulla et al. 1993) the following.
See MRS--Sensor, LFC.
| Color visible | Normal color film sensitive to blue, green and red light. |
| Color infrared | Color-IR film sensitive to green, red, and near-infrared energy. |
The electronic still camera (ESC) is a charged-couple device that produces near-film-quality images in digital format. It has been utilized routinely on missions since 1991. The ESC system has three components: (1) hand-held fully digital and programmable, high-resolution camera, (2) lap-top computer for onboard image processing and downlink, and (3) ground station for reception, processing, and distribution of digital data and images (Lulla and Holland 1993). The camera can operate a 2048x2048 black-and-white pixel array or a 1024x1024 array for three-band color and color-infrared. Current spectral response range is 0.4 to 1.1 µm, which is significantly greater than films now in use.
The ground coverage of space-shuttle photography is determined by factors of orbit geometry that vary with each mission. The most important factor is orbit inclination, ±28.5° for most missions, which limits photographs to low-latitude locations. This includes about one-half of the Earth's surface, an area with more than 75% of the world's human population. Orbital inclinations from ±34.3° to a maximum of ±57° are used on some special missions. For the latter, regions up to around ±60° latitude can be photographed in low-oblique views. High-latitude areas above the Arctic and Antarctic circles are photographed only rarely in high-oblique views.
See MRS--Platform, Space shuttle.
Space-shuttle photography has been utilized for several global-change studies (Lulla et al. 1991). These include monitoring of inland water bodies in climatically sensitive areas: Great Salt Lake, Aral Sea, Lake Chad, etc. Photographs have also been used to document changes in deltaic and estuarine environments, for example the Omo delta of Lake Turkana. Space-shuttle photographs are also valuable for studies of ephemeral events, such as volcanic eruptions and dust, auroras, and dust storms. Color-infrared photographs are useful for establishing biomass (vegetation).
Smoke from natural or man-made fires is a feature of special interest. Compared to other forms of space-based remote sensing, space-shuttle photography excels for imaging smoke from burning biomass (Glasser and Lulla 1998). Space-shuttle photography proved especially valuable for monitoring oil-field fires during the Kuwait War (Lulla and Helfert 1991). Pictures were acquired during two shuttle missions in April and May of 1991.
The presence of human photographers in space has demonstrated some important capabilities to:
The international space station has become operational early in the 21st century. It includes a nadir window dedicated to Earth observation experiments. This window is a multilayer composite, for which the optical properties may be changed. It facilitates high-quality remote sensing in the visible, near-infrared, and mid-infrared portions of the spectrum. Equipment racks around the window provides support, power, and communciations for various kinds of cameras and sensors. The space station also has external mounts for securing remote sensing devices outside the hull.
Continuous, long-term operation of the space station provides unparalleled opportunity for Earth observation. The space station orbits at inclination ± 51.6°, which covers more than 75% of the Earth's surface, containing 95% of the human population. Beneath this orbit, every ground locality is revisited each three days. Earth-observation experiments are now underway, and many kinds of scientific missions are anticipated (Lulla, 1998, pers. com.).
International Space Station
During the period 1995-98, Shuttle/Mir missions paved the way for development of a permanently manned space station. Known as International Space Station, Phase 1, more than 20,000 new photographs were acquired during these missions. Most of the images are not yet cataloged (Glasser and Lulla 1998).
Further Information on
Space Photography
Nearly a quarter million photos
References
ES 771 schedule or ES 771 homepage