Abstract: A user obtains, views and stores image data of a selected celestial object from a network of available telescopes using a computer-generated user interface. Based on the selected object, information is accessed regarding each telescope from data sources such as databases and/or live data feeds to automatically select telescopes that are suitable for imaging the object, e.g., according to factors such as telescope type, power and configuration, location, weather conditions, visibility, and altitude. The user may select a particular telescope and imaging time from a schedule of available telescopes and imaging times. At the scheduled time, an image is recorded of the celestial object and communicated to a central data store for access by the user, e.g., via a web site.

Abstract: A user obtains, views and stores image data of a selected celestial object from a network of available telescopes using a computer-generated user interface. Based on the selected object, information is accessed regarding each telescope from data sources such as databases and/or live data feeds to automatically select telescopes that are suitable for imaging the object, e.g., according to factors such as telescope type, power and configuration, location, weather conditions and altitude. The user may select a particular telescope and imaging time from a schedule of available telescopes and imaging times. At the scheduled time, an image is recorded of the celestial object and communicated to a central data store for access by the user, e.g., via a web site The user may be charged for the service based on factors such as exposure time, scheduling priority, type of telescope and the like.

Abstract: A user obtains, views and stores image data of a selected celestial object from a network of available telescopes using a computer-generated user interface. Based on the selected object, information is accessed regarding each telescope from data sources such as databases and/or live data feeds to automatically select telescopes that are suitable for imaging the object, e.g., according to factors such as telescope type, power and configuration, location, weather conditions and altitude. The user may select a particular telescope and imaging time from a schedule of available telescopes and imaging times. At the scheduled time, an image is recorded of the celestial object and communicated to a central data store for access by the user, e.g., via a web site The user may be charged for the service based on factors such as exposure time, scheduling priority, type of telescope and the like.

Abstract: A reach is formed by the creation of a protective corridor or conduit which itself becomes the instrument of reach. Extension of a reach is achieved by advancing material required to extend the reach through the protective corridor to the leading edge where it becomes incorporated into the outer protective corridor in a manner that extends the protective corridor and hence causing an extension of the reach. In a reverse process retraction of the reach is achieved. Direction control for a reach is achieved by providing operator control over the corridor extension process. Alternately direction control can be determined by the immediate environment or a combination of operator control and immediate environment. Direction control during retraction of a reach is inherent in the reaching method as the outer protective corridor is retracted back into itself at the leading edge thereby retracting the reach along the reverse course of prior extension.

Abstract: A user obtains, views and stores image data of a selected celestial object from a network of available telescopes using a computer-generated user interface. Based on the selected object, information is accessed regarding each telescope from data sources such as databases and/or live data feeds to automatically select telescopes that are suitable for imaging the object, e.g., according to factors such as telescope type, power and configuration, location, weather conditions and altitude. The user may select a particular telescope and imaging time from a schedule of available telescopes and imaging times. At the scheduled time, an image is recorded of the celestial object and communicated to a central data store for access by the user, e.g., via a web site The user may be charged for the service based on factors such as exposure time, scheduling priority, type of telescope and the like.