Abstract: An equatorial mount for providing a telescope with a balanced weight distribution is described. The equatorial mount includes a base, a declination base, and a device support. The declination base is rotatable about a right ascension axis relative to the base. The device support is rotatable about a declination axis relative to the declination base. The declination axis intersects orthogonally with the right ascension axis and the declination axis intersects a midsection of the declination base. The declination base includes a counterweight assembly extending along a counterweight axis, the counterweight axis being spaced away from the declination axis along the right ascension axis.

Abstract: A swing seat unit may include a seat which is provided on a fixing frame and swings on the fixing frame; a dome frame which is provided to be spaced from a rear of the seat and extends upward to surround the rear of the seat; a hemispherical swing dome which is provided on an upper portion of the dome frame, swingable on the dome frame, and is opened downward toward a predetermined direction; and a second driving portion which is provided between the dome frame and the swing dome to provide power for swing the swing dome.

Abstract: An equatorial mount having a base, a right ascension base, a right ascension shaft, a declination base, a declination shaft, and a mount-rotation mechanism, the declination base rotatable about a right ascension axis relative to the right ascension base, and the declination shaft rotatable about a declination axis relative to the declination axis, wherein the mount-rotation mechanism is engageable and disenagageable from one or the other of the right ascension shaft and the declination shaft, to apply torque between the declination base and that shaft when engaged and to permit relative rotation of the shaft and the declination base when disengaged.

Abstract: A telescope mount assembly includes a hub section, a motor assembly, one or more legs extending away from the hub section, and a counterweight coupled to a portion of the hub section. The hub section includes one or more extensions that are each configured to rotate or translate about a fixed axis. The motor assembly is designed to rotate or translate one or more of the extensions. The counterweight includes a battery compartment configured to hold one or more batteries.

Abstract: A magnetic field sensor includes a first magnetic field sensing element configured to produce a first signal representing a detected external magnetic field; a circular vertical hall element configured to produce a second signal representing an amplitude of the external magnetic field; and an error compensation circuit coupled to receive the first and second signal, compute an error value based on the amplitude of the external magnetic field, and apply the error value to the first signal to compensate for an error in the first signal.

Abstract: An integrated system for precision actuation and support for large mobile structures, such as large telescopes, wherein an actuation is integrated on the basis of linear motors located in each of the frames that support the mobile structure on another fixed structure, the support of said frames on the fixed structure being carried out by means of hydrostatic feet. The connection between this frame and the driving structure is made via a flexible kinematic connection that permits relative movements between both (frame and structure), such that the mechanism is only affected in its operation through the small-scale deformations of the track via which it circulates, and not through the large-scale deformations of the structure.

Abstract: A display device includes a display panel including a non-driven area and a driven area symmetric relative to a first straight line passing on the figure center of the driven area and a covering portion covering a peripheral portion of the display panel and including an opening portion symmetric relative to a second straight line passing on the figure center of the opening portion. When the first straight line and the second straight line are viewed from a first direction side, the first straight line and the second straight line are disposed in parallel to each other on a plane, and when the plane is viewed in a plan view, one side portion and the other side portion that are included in the driven area and covered by the covering portion and that are located opposite each other with the first straight line located between the one side portion and the other side portion have mutually different lengths in a direction perpendicular to the first straight line.

Abstract: The present invention relates to a linear drive with a stator, a runner, and two rotative drive units provided for driving the runner. It is provided according to the invention that the linear drive comprises two magnetorheological clutches, wherein the first drive unit can be coupled to the runner using a first magnetorheological clutch and the second drive unit can be coupled to the runner using a second magnetorheological clutch. The output torque of the first drive unit acts upon the runner in the opposite direction to the output torque of the second drive unit.

Abstract: A technique for equatorially mounting a telescope includes a right ascension support having a first end coupled to a counterweight assembly and a second end coupled to a declination support. The right ascension support is coupled to a base and extends downwardly and backwardly from the first end to the second end. The resulting arrangement causes the act of balancing the telescope about its right ascension axis also substantially to balance the telescope about its base.

Abstract: Telescope assembly for tracking celestial bodies, comprising a telescope and a positioning device for the telescope, wherein the positioning device is provided with an under frame to be placed on a base, a first telescope holder placed on the under frame, a second telescope holder which at a first side is coupled to the first telescope holder and which bears the telescope, wherein the telescope assembly is provided with a third telescope holder which is coupled to a second side of the second telescope holder and which by means of a third rotary bearing can be rotated about a polar axis of rotation.

Abstract: A terminal device of an apparatus to automatically introduce a target celestial object includes an input operation section executing a command operation on the apparatus. An image display section indicates a star map image in accordance with a display scale factor. The input operation section includes a rotation command means that executes a rotational driving of the astronomical telescope in a telescope control mode. A scale factor input means executes an input specification of the display scale factor for the displayed star map image, which corresponds to a position on a celestial sphere toward which the astronomical telescope is headed, while a speed of rotation of the astronomical telescope controlled by the rotation command means changes in accordance with a decreasing function of the display scale factor.

Abstract: A technique for equatorially mounting a telescope includes a right ascension support having a first end coupled to a counterweight assembly and a second end coupled to a declination support. The right ascension support is coupled to a base and extends downwardly and backwardly from the first end to the second end. The resulting arrangement causes the act of balancing the telescope about its right ascension axis also substantially to balance the telescope about its base.

Abstract: An alt-az mount for supporting and orienting optical instruments comprises: a generally horizontally extending arm couple to a level surface by an azimuthal pivot joint which permits pivotal movement of the horizontally extending arm with respect to the level surface about a vertical azimuthal axis; a generally vertically extending arm pivotally coupled to the horizontally extending arm by an inter-arm pivot joint which permits pivotal movement of the vertically extending arm with respect to the horizontally extending arm about a vertical inter-arm axis; and an instrument coupling mechanism for coupling the mount to an optical instrument, the instrument coupling mechanism comprising an altitude pivot joint which permits pivotal movement of the optical instrument with respect to the vertically extending arm about a horizontal altitude axis.

Abstract: A system with a calibrated rotary encoder can be used for accurate telescope tracking along the Right Ascension (RA) rotation axis. The system includes an incremental quadrature optical encoder, a microcontroller unit (MCU), a timer, an electronic memory, and a control interface. The rotor of the encoder is coaxially attached to the RA drive shaft of the telescope mount in order to send angular position data for the RA drive shaft to the MCU. The MCU evaluates the angular position data for errors and send corrections to the control mechanism of the RA drive shaft. The electronic memory stores calibrated reference data, which is compared to the angular position data by the MCU. The calibrated reference data can be found by measuring the movement of a reference star across an image. The system can also calculate an accurate visible speed for the Earth's rotation in a desired direction.

Abstract: A mount for a telescope, which allows precise polar of the telescope. The mount comprises: a base with a fixed portion and a pivoting portion; a first rocking structure, mounted to the base, which rotates by 90° on a plane perpendicular to the base; a second rocking structure, mounted to the first structure, which defines an axis AR and rotates by 180° about AR; a polar telescope, mounted to the second structure, with the optical axis aligned with AR; rotating joints, mounted to the second structure, defining an axis D incident and perpendicular to AR; a hose clamp, mounted to the rotating joints, and defining a housing for a telescope; a finder telescope, mounted to the rotating joints or clamp, with the optical axis XC being aligned with the housing defined by the clamp.

Abstract: According to various embodiments, a telescope is automatically aligned without requiring user intervention and without requiring knowledge of actual local time or location. A mount model specifying a relationship between a telescope's internal coordinate system and a celestial coordinate system is generated using an arbitrary time, arbitrary telescope location, and a number of alignment reference points. A pointing error for the initial mount model is determined, for example using a plate solving technique to translate between plate coordinates and celestial coordinates for the alignment reference points. Time and location values are iteratively adjusted to reduce the pointing error until it is acceptably low. In one embodiment, adjustments are made by reference to a local sidereal time (LST) offset and/or a latitude value. In one embodiment, the iterative adjustment is performed using a two-phase methodology, including a coarse adjustment followed by a fine adjustment.

Abstract: A plate solving methodology determines celestial coordinates of an image. Star locations are extracted from the image in terms of pixel coordinates. A group of four stars, referred to as a “test quad”, is identified. A signature for the test quad is generated. In one embodiment, this test signature is derived by determining the separations of the four stars in the test quad, normalized by the largest separation. In one embodiment, the signature also includes the sum of these normalized separations. A query is performed, using the generated signature, against a database of reference signatures for known groups of stars (referred to as “reference quads”). A geometric transform is determined, establishing the relationship between the test quad and a reference quad that matches within a specified tolerance. This geometric transform defines the celestial coordinates of the image. Additional verification steps can be performed to confirm the accuracy of the match.

Abstract: A terminal device of an apparatus to automatically introduce a target celestial object includes an input operation section executing a command operation on the apparatus. An image display section indicates a star map image in accordance with a display scale factor. The input operation section includes a rotation command means that executes a rotational driving of the astronomical telescope in a telescope control mode. A scale factor input means executes an input specification of the display scale factor for the displayed star map image, which corresponds to a position on a celestial sphere toward which the astronomical telescope is headed, while a speed of rotation of the astronomical telescope controlled by the rotation command means changes in accordance with a decreasing function of the display scale factor.

Abstract: A polar scope for a telescope mount includes a reticle having a pattern with multiple markings that allows users to accurately position pole stars for precise polar alignment. A system and mount may be provided including a polar scope of this kind. The polar scope may be provided with a controller that calculates the apparent position of a pole star, while accounting for errors, such as proper motion, precession of the earth's axis, and/or atmospheric refraction.

Abstract: A terminal device of an apparatus to automatically introduce a target celestial object includes an input operation section executing a command operation on the apparatus. An image display section indicates a star map image in accordance with a display scale factor. The input operation section includes a rotation command means that executes a rotational driving of the astronomical telescope in a telescope control mode. A scale factor input means executes an input specification of the display scale factor for the displayed star map image, which corresponds to a position on a celestial sphere toward which the astronomical telescope is headed, while a speed of rotation of the astronomical telescope controlled by the rotation command means changes in accordance with a decreasing function of the display scale factor.

Abstract: A Dobsonian telescope apparatus having a first motor for rotating the telescope about a first axis, a second motor for rotating the optical tube assembly about a second axis, and a handheld control device. The first and second axes are perpendicular to each other. The apparatus avoids the erratic manual nudging by the user needed to align a conventional Dobsonian telescope.

Abstract: A digitally controlled platform for precise celestial tracking of astronomical telescopes, generally those having an independent pointing mechanism. A movable stage carrying the telescope is moved relative to a base by three digitally controlled actuators each of which determines the distance between a point fixed in the base and a point fixed stage. The base and stage otherwise are connected by a mechanism that holds a single point fixed in the base in coincidence with a single point fixed in the stage. It functions without approximation at any digitally specified latitude and longitude, enabling astrophotography with alt/azimuth mounted telescopes and diurnal tracking through the zenith. The digital controller may be a personal computer laptop running a multitasking operating system linked to the platform electronics by a Universal Serial Bus cable. Novel software design allows precise tracking, control, and calibration in spite of operating system and Universal Serial Bus latency.

Abstract: An apparatus for the focusing of incident light includes a base assembly that is adapted to support a primary mirror. The primary mirror includes an outside circumference and an inside aperture. An upright member is attached to the base assembly at a first end thereof at a first location that is disposed inside the aperture and at a second location that is disposed outside the primary mirror. The upright member includes a second end that is distally disposed with respect to the first end. The second end is adapted to receive a turret that includes a secondary mirror and is adapted to pivot between two positions. An IMU is attached to the base assembly proximate the primary mirror.

Abstract: A portable astronomical telescope includes the cylinder body, on which three telescopic legs are hinged through a joint to form a tripod stand. The bottom of aforementioned cylinder body is fixed by means of connection element and mounted with part box. On the bottom end of this part box, a bottom cover is insert-mounted. On the upper end of the part box, limit connection elements of the connected telescopic leg are hinged. Within the aforementioned cylinder body, a guide bush is fixed and installed, inside of which telescope base is mounted. On the side of this telescope base, a guide pin is established. On the side of the guide sleeve, an L-shaped feed-through slot is established to accommodate the guide sleeve. On the tail end of the above feed-through slot, one guide pin residence slot is connected. The aforementioned telescope base is activated by the lug and mounted with bellows. This product can be used without need for separate assembly, and eliminates the need for a separate package.

Abstract: A terminal device of an apparatus to automatically introduce a target celestial object includes an input operation section executing a command operation on the apparatus. An image display section indicates a star map image in accordance with a display scale factor. The input operation section includes a rotation command means that executes a rotational driving of the astronomical telescope in a telescope control mode. A scale factor input means executes an input specification of the display scale factor for the displayed star map image, which corresponds to a position on a celestial sphere toward which the astronomical telescope is headed, while a speed of rotation of the astronomical telescope controlled by the rotation command means changes in accordance with a decreasing function of the display scale factor.

Abstract: A first aspect of the invention relates to a mount (1) for a telescope (5). The mount comprises: a basement (2) with a fixed portion (3) and a pivoting portion (4); a first rocking structure (7), mounted to the basement, which rotates by 90° on a plane perpendicular to the basement; a second rocking structure (8), mounted to the first structure, which defines an axis AR and rotates by 180° about AR; a polar telescope (12), mounted to the second structure, with the optical axis aligned with AR; rotating joints (13), mounted to the second structure, defining an axis D incident and perpendicular to AR; a hose clamp (14), mounted to the rotating joints, and defining a housing for a telescope; a finder telescope (15), mounted to the rotating joints or clamp, with the optical axis Xc being aligned with the housing defined by the clamp. A second aspect of the invention relates to a method for the precise polar position of a telescope supported by this mount.

Abstract: An energy signal processing system (10) includes a first shaft assembly (14) rotatable about an azimuth axis (16), and a second shaft assembly (18) coaxially mounted for rotation about the azimuth axis (16). The first shaft assembly (14) defines a zenith plane (20) inclined with respect to the azimuth axis (16). The system (10) includes an energy signal processing element (22) rotatable about a processing element axis (24) that intersects and is generally perpendicular to the azimuth axis (16), as well as a means for rotating the element (22) about the element axis (24) such that: energy signals travelling substantially along a preselected path axis (12) and impinging the energy signal processing element (22) are processed or deflected substantially along the azimuth axis (16); or vice versa; or energy signals generated by the energy signal processing element (22) are directed substantially along the preselected path axis (12).

Abstract: An automatic introduction apparatus for automatically introducing a target celestial object by controlling a rotation of an astronomical telescope around at least two axes comprises: an image-capturing means capable of capturing an image of a celestial object at a plurality of focal distances; a celestial object database; an image processing section for extracting a set of information of each celestial object from the image of celestial object captured by the image-capturing means; and a celestial object identification means for identifying the celestial object whose image has been captured, by comparing the information of each celestial object extracted by the image processing sections with the celestial object information stored in the celestial object database.

Abstract: The present invention relates to a mount for telescopes, particularly of a portable type for amateur or semi-amateur telescopes, though it can be also applied to fixed telescopes and professional telescopes. Particularly, the present invention relates to a support for a telescope comprising a mount and means for resting said mount on the ground, wherein said mount comprises a primary rocking element allowing one to set the latitude of the observation place, to said primary rocking element being pivotally fastened a frame which allows moving the telescope about the right ascension axis and/or about the declination axis.

Abstract: A celestial tracking device (10) for mounting an instrument thereon, the celestial tracking device (10) comprising first and second arms (12, 14) rotatably attached together at one end (13) and a drive means (20) rotatably connected between the other ends (15) of the first and second arms (12, 14) for relative rotation thereof between a home position and a deployed position. Advantageously, in the home position the drive means (20) is rotatable either clockwise or anticlockwise for use in the Northern or Southern hemispheres respectively. A further advantage is that the arms (12, 14) are stowed overlapping one another so that the device is compact and easily portable.

Abstract: The present invention provides a telescope system having enhanced capabilities for configuring and calibrating a telescope, operation and control of the telescope, and viewing of imagines from the telescope. The present invention employs a control system for controlling the position and orientation of the telescope. In one embodiment, the system uses GPS systems and the like to determine the position of the telescope. The system may use either the light detected by the telescope or measurements of stars within the field of view to determine the orientation of the telescope. Following calibration, the user may operate a control system to reorient the telescope to the desired field of view. Further, the user may operate software that allows the user to select stars, constellations, or other objects of interest. Based on this selection, the system operates the telescope to alter its field of view to view the selected object.

Abstract: Disclosed is a light collimating system for mounting at the primary focus of a Schmidt-Cassegrain telescope (SCT) in place of the secondary mirror. The system comprises a housing containing a plurality of lens elements optimized to reduce optical aberrations. The resulting system has a focal ratio of approximately f/2, a short exposure time for optical imaging, and a wide field of view with very little distortion. The housing is attached to the corrector plate of the SCT by a pair of rings held together by a plurality of screws that further facilitate the alignment and rotation of the light collimating system.

Abstract: A coude gimbal structure includes a two-axis gimbal system having an outer gimbal pivotable about a first rotational axis, and an inner gimbal supported on the outer gimbal and pivotable about a second rotational axis which intersects the first rotational axis at an intersection point. A folded afocal three-mirror anastigmat has a positive-optical-power primary mirror, a negative-optical-power secondary mirror, and a positive-optical-power tertiary mirror, and a first flat fold mirror, and a second flat fold mirror. A beam path incident upon the primary mirror is reflected from the primary mirror to the secondary mirror. The tertiary mirror lies on the second rotational axis, the first flat fold mirror redirects the beam path reflected from the secondary mirror to the tertiary mirror, and the second flat fold mirror lies at the intersection point and redirects the beam path reflected from the tertiary mirror along the first rotational axis.

Abstract: A portable astronomical telescope includes the cylinder body, on which three telescopic legs are hinged through a joint to form a tripod stand. The bottom of aforementioned cylinder body is fixed by means of connection element and mounted with part box. On the bottom end of this part box, a bottom cover is insert-mounted. On the upper end of the part box, limit connection elements of the connected telescopic leg are hinged. Within the aforementioned cylinder body, a guide bush is fixed and installed, inside of which machine base is mounted. On the side of this machine base; a guide pin is established. On the side of the guide sleeve, an L-shaped feed-through slot is established to accommodate the guide sleeve. On the tail end of the above feed-through slot, one guide pin residence slot is connected. The aforementioned machine base is activated by the lug and mounted with bellows. This product can be used without need for separate assembly, and eliminates the need for a separate package.

Abstract: Embodiments of the present disclosure include presenting data related to image information captured by a telescope on an electronic display, such as, for example, a high definition display. For example, a telescope control system may advantageously output video or other signals to one or more displays in a multi-media or image presentation. In certain preferred embodiments, such display comprises high definition displays, or the like. For example, such display may comprise entertainment, academic or other presentations.

Abstract: An apparatus for the focusing of incident light includes a base assembly that is adapted to support a primary mirror. The primary mirror includes an outside circumference and an inside aperture. An upright member is attached to the base assembly at a first end thereof at a first location that is disposed inside the aperture and at a second location that is disposed outside the primary mirror. The upright member includes a second end that is distally disposed with respect to the first end. The second end is adapted to receive a turret that includes a secondary mirror and is adapted to pivot between two positions. An IMU is attached to the base assembly proximate the primary mirror.

Abstract: Autonomous operation of ground telescope and CCD imaging systems is a highly desirable mode of conducting amateur and professional astronomy. Many current systems allow remote operation to some degree, but no commercial system permits complete autonomous operations suitable for precise pointing and imaging. In particular, the initial alignment of the telescope to the celestial coordinates is a manual operation for all but the highest end commercial systems. Even for the systems that permit a crude automatic initial alignment, operational alignments require manual intervention.

Abstract: A disc-based altitude-azimuth telescope mount for mounting and adjusting a telescope along altitude and azimuth axes. The telescope mount includes an azimuth disc assembly for facilitating adjustment of the telescope along the azimuth axis and an altitude disc assembly for facilitating adjustment of the telescope along the altitude axis. A friction adjusting mechanism operably engages the azimuth disc assembly and the altitude disc assembly to prevent inadvertent movement of the telescope along both axes. A digital setting circle may be operably connected to the disc assemblies to facilitate automatic adjustment of the telescope, as desired.

Abstract: Embodiments of the present disclosure include user-directed automated telescope alignment systems and methods. In various embodiments, the automated alignment procedure provides for user-direction in selecting astronomical alignment objects. For example, in an embodiment, after the telescope is aligned according to a first approximation alignment, the user may direct the field of view of the telescope system to a viewable, sufficiently bright astronomical object. Upon bringing the object into the field of view, the alignment procedure advantageously identifies the likely astronomical object based on the first approximation alignment. The procedure also updates the first approximation alignment based on known information about the identified object. The process of user-direction to additional viewable bright astronomical objects provides for more precise and accurate mappings of telescope movements to celestial field of view.

Abstract: A system for operating an astronomical observatory made up of astronomical hardware, utilizing a web browser operated by a user, and a web server connected to the observatory, wherein both the control to, and feedback from the observatory are displayed to the user in real time independent of personnel support at the observatory site. The user submits a request to the observatory via the web browser, which displays the status and results of the request. A web server, coupled to the various astronomical hardware, processes the request on behalf of the user and responds with the status and results of the request. The status and/or results ae then displayed by the web browser to the user. Requests may be made by the user interactively, or in the form of a script. The system may be used over wide area networks, like the Internet, or any other type of network.

Abstract: A portable altitude/azimuth telescope mount having an integral locator system with a magnetic encoder mechanism for facilitating location of astronomical objects and telescope positioning for observation thereof. A microprocessor receives signals from the encoder mechanism and translates such into position data for display. The locator system also includes a database of astronomical objects, including their locations and other relevant information. The mount is preferably provided with a drive mechanism adapted to allow for automatically or manually positioning the telescope to view astronomical objects and for automatically repositioning or steering the telescope in order to track the astronomical objects during extended viewing. When moved manually, components of the drive act as a clutch mechanism that effectively disengages the drive motor to avoid damage. An instance of the drive may be provided for each axis of movement.

Abstract: A solar telescope is disclosed that facilitates safe observation of the sun with minimal setup, targeting effort or operator skill. The folded solar telescope of the invention includes a friction stabilized telescope support system that is capable of maintaining a specified telescope orientation. The telescope further includes a targeting system that comprises one or more pointing aids to simplify the process of aligning the telescope with the sun so a solar image is projected onto a viewing surface.

Abstract: From a plurality of pictures 1-1 through 1-3 captured at successive time intervals, pictures 2-1 through 2-3 of regions determined in accordance with the movement of the celestial object are cut out. By deriving median values in regard to the same pixels in each of the cut-out pictures 2-1 through 2-3, a median value picture 3-1 is created. By deriving median values, the influence of large numbers of fixed starts that hinder the detection of the moving celestial object that moves in the cut-out pictures is eliminated, and only the moving celestial object is permitted to remain. When deriving median value, pixel values indicating singular values are eliminated in advance, so that the effects of the images of large bright light sources and the lost pixels that output no pixel values are effectively reduced.

Abstract: A fully automated telescope system is able to be fully operable in both Alt-Az and polar configurations. In either configuration, the telescope aligns itself to the celestial coordinate system following a simplified initialization procedure during which the telescope tube is first pointed north and then pointed towards a user's horizon. A command processor, under application software program control orients the telescope system with respect to the celestial coordinate system given the initial directional inputs. The initial telescope orientation may be further refined by initially inputting a geographical location indicia, or by shooting one or two additional celestial objects. Once the telescope's orientation with respect to the celestial coordinate system is established, the telescope system will automatically move to and track any desired celestial object without further alignment invention by a user.

Abstract: An automated telescope includes an optical system and respective altitude and azimuth motor systems. Each motor system is configured to rotate the optical system about a corresponding altitude or azimuth axis. Each of the altitude and azimuth motor systems includes a motor and a microprocessor configured to control its respective motor. A third microprocessor is connected to microprocessors of both the altitude and azimuth motor systems. The third microprocessor is programmed to determine a relationship between a celestial coordinate system and an altitude-azimuth coordinate system and to generate motion control commands based at least in part on the determined relationship. Each microprocessor of the altitude and azimuth motor systems then controls its respective motor based at least in part on the motion control commands.

Abstract: A telescope support stand system for side cutaway view of the present invention in the contracted position. The telescope support stand system includes a base that is permanently secured to a floor, a lower tube attached to the base, an upper tube slidably positioned about the lower tube, an elevating unit within the lower tube for elevating the upper tube, and a support plate attached to the upper tube for mounting a telescope thereto. The outer tube preferably includes a plurality of alignment plates for providing a reduced friction guide surface for sliding about the lower tube.

Abstract: A portable altitude/azimuth telescope mount having an integral locator system with a magnetic encoder mechanism for facilitating location of astronomical objects and telescope positioning for observation thereof. A microprocessor receives signals from the encoder mechanism and translates such into position data for display. The locator system also includes a database of astronomical objects, including their locations and other relevant information. The mount is preferably provided with a drive mechanism adapted to allow for automatically or manually positioning the telescope to view astronomical objects and for automatically repositioning or steering the telescope in order to track the astronomical objects during extended viewing. When moved manually, components of the drive act as a clutch mechanism that effectively disengages the drive motor to avoid damage. An instance of the drive may be provided for each axis of movement.

Abstract: An equatorial tracking platform for a telescope that comprises two rolling surfaces, each in contact with a pair of rollers which each have an adjustment for the latitude setting. One rolling surface is a complex 3-dimensional contour, which provides for a differing radius for each latitude setting, while the other rolling surface is of fixed radius. By varying the angle of the roller pairs, the virtual axis of rotation is changed to be aligned parallel to the earth's rotational axis, thus allowing a telescope to accurately track a celestial object.

Abstract: The polar-axis telescope has an objective lens, a focal plate, an eyepiece, a zoom optical system, and a zoom optical system driver. The objective lens forms an object image, and the focal plate is arranged on a focal plane of the objective lens. The eyepiece is arranged backward of the focal plate and forms an observed image. The zoom optical system is arranged between the objective lens and the eyepiece. The zoom optical system makes the observed image appear gradually bigger while maintaining an in-focus situation. The zoom optical system driver shifts the zoom optical system along a polar-axis, corresponding to an optical axis of the polar-axis telescope, so as to change a magnification.

Abstract: An apparatus and method for stabilizing an optical tube on a base wherein a tension adjuster adapted to adjust the tension between the optical tube and sideboard of the base is secured between a the optical tube and the sideboard. By turning the tension adjuster, tension can be added or reduced to stabilize the optical tube.