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Unistellar is a French manufacturer of computer-connected telescopes that allow non-professional skywatchers to observe astronomical objects at relatively low cost. The first product launched was named the eVscope, and used digital astrophotographic techniques. [1] [2] SETI Institute has partnered with Unistellar and will be able to send requests for information and notifications to users, and receive information about transient astronomical events.
The eVscope is a 114 mm (4.5 in)-diameter Prime focus reflector, focal length 450 mm. It projects its image onto a 4.8 mm × 3.6 mm (0.19 in × 0.14 in) CMOS color sensor with 1.3 million pixels. [2] The image is transmitted to a small screen in an eyepiece also mounted on the telescope. An electronic connection to a computer (smartphone, pad, or laptop) is required to make astronomical observations from the telescope. The digital technology allows multiple images to be stacked while subtracting the noise component of the observation producing images of Messier objects and faint stars as dim as an apparent magnitude of 15 with consumer-grade equipment.
The company was founded in Marseille, France, [3] in 2015, with incubator investment from Incubateur Impulse and Pépinières d'Entreprises Innovantes with subsequent VC round capital from private investors and a VC firm named Brighteye Ventures. [4] Unistellar unveiled their electronic telescope technology prototype in 2017 at CES2017 in Las Vegas [5] and at IFA Next in Berlin. [1]
The company experienced difficulties bringing the product to market. The consumer-grade electronic telescope was originally planned to be available in the "fall 2018" [1] which subsequently shifted to "early 2019," [6] then later in 2019.
By January 2020, the telescope was expected to be shipped worldwide between May and August 2020. [7] As of December 2021, over 5000 telescopes had been delivered to customers [8] The kit included a custom tripod and mount, a Bahtinov mask and a protective cap. [9] Later, Unistellar introduced two new telescopes, eVscope 2 with bigger FOV and better monitor which won the T3 Platinum Award, [10] and eQuinox with longer battery life and no monitor. [11]
As presented in AGU 2021 Fall Meeting, the eVscope had observed many astronomical objects up to December 2021, including the detection by 79 observers of 85 transits by Jupiter-sized exoplanets, 281 asteroid occultations (including forty-five positive ones), and three shape and spin solutions for near-Earth asteroids. The network also supported NASA's TESS mission by making transatlantic observations of an exoplanet transit, and NASA's Lucy mission by profiling Trojan asteroids this spacecraft will visit. These data are collected by observers in Europe, North America, Japan, Australia, and New Zealand. Unistellar aims to expand the network to the rest of Asia and to South America. [8]
The Unistellar Exoplanet (UE) campaign helped to improve the measurement accuracy of the orbital period of TOI 3799.01. The UE campaign also helps to refine the orbit of long-period exoplanets, such as the Jupiter-analog Kepler-167e and the eccentric planet HD 80606b, which have transit durations longer than 10 hours. This refinement will help with follow-up observations, such as JWST observation of HD 80606b. [12]
The Stellina astrophotography telescope by Vaonis is a similar technology-facilitated telescope that uses a digital display in lieu of an eyepiece and stacks images to get high-resolution images of deep-sky objects. [13]
Amateur astronomy is a hobby where participants enjoy observing or imaging celestial objects in the sky using the unaided eye, binoculars, or telescopes. Even though scientific research may not be their primary goal, some amateur astronomers make contributions in doing citizen science, such as by monitoring variable stars, double stars, sunspots, or occultations of stars by the Moon or asteroids, or by discovering transient astronomical events, such as comets, galactic novae or supernovae in other galaxies.
Astrophotography, also known as astronomical imaging, is the photography or imaging of astronomical objects, celestial events, or areas of the night sky. The first photograph of an astronomical object was taken in 1840, but it was not until the late 19th century that advances in technology allowed for detailed stellar photography. Besides being able to record the details of extended objects such as the Moon, Sun, and planets, modern astrophotography has the ability to image objects outside of the visible spectrum of the human eye such as dim stars, nebulae, and galaxies. This is accomplished through long time exposure as both film and digital cameras can accumulate and sum photons over long periods of time or using specialized optical filters which limit the photons to a certain wavelength.
A minor-planet moon is an astronomical object that orbits a minor planet as its natural satellite. As of January 2022, there are 457 minor planets known or suspected to have moons. Discoveries of minor-planet moons are important because the determination of their orbits provides estimates on the mass and density of the primary, allowing insights into their physical properties that are generally not otherwise accessible.
An optical telescope is a telescope that gathers and focuses light mainly from the visible part of the electromagnetic spectrum, to create a magnified image for direct visual inspection, to make a photograph, or to collect data through electronic image sensors.
90 Antiope is a double asteroid in the outer asteroid belt. It was discovered on 1 October 1866, by Robert Luther. In 2000, it was found to consist of two almost-equally-sized bodies orbiting each other. At average diameters of about 88 km and 84 km, both components are among the 500 largest asteroids. Antiope is a member of the Themis family of asteroids that share similar orbital elements.
45 Eugenia is a large asteroid of the asteroid belt. It is famed as one of the first asteroids to be found to have a moon orbiting it. It was also the second triple asteroid to be discovered, after 87 Sylvia.
An eyepiece, or ocular lens, is a type of lens that is attached to a variety of optical devices such as telescopes and microscopes. It is named because it is usually the lens that is closest to the eye when someone looks through an optical device to observe an object or sample. The objective lens or mirror collects light from an object or sample and brings it to focus creating an image of the object. The eyepiece is placed near the focal point of the objective to magnify this image to the eyes. The amount of magnification depends on the focal length of the eyepiece.
A robotic telescope is an astronomical telescope and detector system that makes observations without the intervention of a human. In astronomical disciplines, a telescope qualifies as robotic if it makes those observations without being operated by a human, even if a human has to initiate the observations at the beginning of the night or end them in the morning. It may have software agents using artificial intelligence that assist in various ways such as automatic scheduling. A robotic telescope is distinct from a remote telescope, though an instrument can be both robotic and remote.
The Haute-Provence Observatory is an astronomical observatory in the southeast of France, about 90 km east of Avignon and 100 km north of Marseille. It was established in 1937 as a national facility for French astronomers. Astronomical observations began in 1943 using the 1.20 m telescope, and the first research papers based on observations made at the observatory were published in 1944. Foreign observers first used the observatory in 1949, when Geoffrey and Margaret Burbidge visited.
An astronomical survey is a general map or image of a region of the sky that lacks a specific observational target. Alternatively, an astronomical survey may comprise a set of images, spectra, or other observations of objects that share a common type or feature. Surveys are often restricted to one band of the electromagnetic spectrum due to instrumental limitations, although multiwavelength surveys can be made by using multiple detectors, each sensitive to a different bandwidth.
An astrograph is a telescope designed for the sole purpose of astrophotography. Astrographs are mostly used in wide-field astronomical surveys of the sky and for detection of objects such as asteroids, meteors, and comets.
The Panoramic Survey Telescope and Rapid Response System located at Haleakala Observatory, Hawaii, US, consists of astronomical cameras, telescopes and a computing facility that is surveying the sky for moving or variable objects on a continual basis, and also producing accurate astrometry and photometry of already-detected objects. In January 2019 the second Pan-STARRS data release was announced. At 1.6 petabytes, it is the largest volume of astronomical data ever released.
Franck Marchis, astronomer and planetary scientist, is best known for his discovery and characterization of multiple asteroids, his study of Io volcanism and imaging of exoplanets, planets around other stars.
In amateur astronomy, "GoTo" refers to a type of telescope mount and related software that can automatically point a telescope at astronomical objects that the user selects. Both axes of a GoTo mount are driven by a motor and controlled by a computer. It may be either a microprocessor-based integrated controller or an external personal computer. This differs from the single-axis semi-automated tracking of a traditional clock-drive equatorial mount.
John "Jack" Borden Newton is a Canadian astronomer, best known for his publications and images in amateur astrophotography.
The Givatayim Observatory is a public observatory that was founded in 1968 by the Israeli Astronomical Association and the Givatayim municipality.
The Mirasteilas Observatory is an astronomical observatory in Falera in the canton of Grisons in Switzerland. With its 90-centimeter telescope it is the largest publicly accessible observatory in Switzerland.
Observatory Robert A. Naef is an astronomical observatory located at Épendes, Canton of Fribourg, Switzerland at 7.13938 degrees east of Greenwich and 46.76236 degrees north latitude. Its parallax constants are : ρ sin φ' = 0.68632 and ρ cos φ' = +0.72501.
An autoguider is an automatic electronic guidance tool used in astronomy to keep a telescope pointed precisely at an object being observed. This prevents the object from drifting across the field of view during long-exposures which would create a blurred or elongated image.
Afocal photography, also called afocal imaging or afocal projection is a method of photography where the camera with its lens attached is mounted over the eyepiece of another image forming system such as an optical telescope or optical microscope, with the camera lens taking the place of the human eye.
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