Telescope N 114/450 eVscope 2

He Unistellar eVscope 2 It is an ingenious combination of traditional GoTo telescope with the latest technology. It is equipped with a highly sensitive sensor that captures the faint light of distant galaxies and nebulae and projects it through the eyepiece on a modern OLED screen. In this way, it manages to combine the advantages of computer control with the image amplification of classic visual observation.

Smart and easy to handle
Simply turn it on and select the object you want to observe in the app, without the need for complicated alignments with the North Star or prior knowledge of the night sky. The eVscope telescope automatically orients itself with the help of an integrated compass, an acceleration sensor and an astrometric calibration system (for star field identification).
In addition, it is operated wirelessly and intuitively via a smartphone or tablet with the Unistellar application (for Android and iOS). The battery, which lasts all night, up to 10 hours, is integrated to avoid tangled cables or having to carry external batteries.

Automatic field identification ( Autonomous Field Detection )
This technology supersedes traditional GoTo systems! The eVscope's ingenious astrometric calibration procedure analyzes the stars within the field of view in seconds to calculate the current position of the telescope. This allows objects to be found and tracked across the night sky with astonishing precision.

Image amplification ( Enhanced Vision Technology )
In ordinary telescopes, less luminous objects, such as galaxies or nebulae, are only seen as faint points of light. But the eVscope has an image amplification function ( live stacking either live stacking ) that you can activate so that the telescope accumulates the captured light over longer periods of time, and not just in individual captures. Thus, in a matter of a few seconds you will be able to enjoy the object of your observation as no other telescope of this size is capable of representing it. As the minutes pass, you will be able to see firsthand how the image intensifies and gains clarity, with increasingly clear colors and structures.

Robust optics
The Newton telescope with 114 mm aperture and 450 mm focal length has a f/4 aperture ratio that sends an image particularly bright to the sensor. For its part, the parabolic main mirror reproduces the image without spherical or chromatic aberrations.
Thanks to the Bahtinov mask Integrated into the dust cover, focusing will be child's play: even without prior experience or knowledge you can achieve a sharp image in just a moment.
The eVscope replaces the secondary mirror with a sensor Sony IMX347 . Because its readout noise is so low, this CMOS sensor is installed in many high-sensitivity astrocameras.
The eVscope telescope processes the image captured by the sensor and presents it through the eyepiece. Then comes into play OLED screen with an extremely high contrast ratio. The result is comparable to a live observation through purely visual optics. In addition, the object of observation is also displayed on the screen of the smartphone or tablet.

Partnership with SETI
Thanks to the cooperation with SETI you will be able to collaborate in making scientific discoveries and be part of a world wide web of eVscope telescopes. The data from its eVscope captures will help scientists study supernovae, comets and asteroids.

Specifications