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Daystar Sol 80mm Dedicated Solar Telescope

SKU DAY-SOL80
Original price $2,995.00 - Original price $2,995.00
Original price
$2,995.00
$2,995.00 - $2,995.00
Current price $2,995.00
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  • 80mm Aperture Dedicated Hydrogen-Alpha Solar Telescope
  • 1400mm Effective Focal Length (f/17.5)
  • Chromosphere Model: 0.5Å FWHM Bandwidth or Narrower
  • Electronic PID-Controlled Thermal Tuning with ±0.5Å Manual Wing Shift
  • Integrated 4.3x Telecentric Barlow Optimized for 656nm
  • Daystar 12:1 Dual-Speed Helical Rack and Pinion Focuser
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  • Description
  • FAQ
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  • Daystar Sol 80mm Dedicated Solar Telescope

    The Daystar Sol 80mm Dedicated Solar Telescope is a complete, no-compromises instrument designed around an internal, thermally-tuned Hydrogen-Alpha filter system with a bandwidth of 0.5Å or narrower. Its 80mm achromatic doublet objective and integrated 4.3x telecentric barlow produce a 1400mm effective focal length at f/17.5, optimized specifically for high-contrast views of the Sun's chromosphere. The PID-controlled heating system maintains the etalon on the 6562.8Å wavelength and allows for a manual ±0.5Å wing shift in 0.1Å steps, all powered by a standard 5V, 1.5A USB connection.

    An Integrated 80mm Hydrogen-Alpha Telescope

    The Daystar Sol 80 is an all-in-one solar telescope that has its etalon, blocking filter and telecentric barlow built in, so there is no separate front filter or barlow to fit. From the 80mm objective to the 13mm blocking filter, the optical train is designed as a single unit, which offers safety and ease of use without the need for component matching.

    This design is intended for astronomers who want a dedicated, high-performance solar instrument that is ready to use out of its case. Weighing 2.8 kg (6.1 lb) with rings, it is a portable tool for detailed visual observation and imaging of the Sun's dynamic atmosphere.

    Observing the Sun's Chromosphere in 6562.8Å Light

    By isolating the specific 6562.8Å wavelength of Hydrogen-Alpha light, the Sol 80 reveals the Sun's chromosphere, a turbulent layer of gas just above the visible surface (photosphere). This allows you to witness a constantly changing landscape of magnetic activity that is invisible in white light.

    • Prominences and Filaments: See vast arcs of plasma extending from the solar limb, and their dark, ribbon-like counterparts silhouetted against the brighter disk.
    • Active Regions and Plages: Observe the bright, magnetically complex areas that often surround sunspots, indicating regions of intense solar activity.
    • Spicules and Flares: With good seeing, you can resolve the fine, jet-like spicules that form a "burning prairie" at the Sun's edge and witness the abrupt, brilliant energy release of solar flares.

    80mm Doublet with a 4.3x Telecentric Barlow

    The heart of the optical system is an 80mm air-spaced achromatic doublet objective. Light from this primary lens passes through an integrated, fully baffled 2-element 4.3x telecentric barlow. The barlow produces a slower focal ratio and a more parallel light beam, controlling the angle of light entering the temperature- and angle-sensitive etalon.

    This combination results in an effective focal length of 1400mm and a focal ratio of f/17.5. Because of the included barlow, a large magnification is achieved with normal focal length eyepieces and ample backfocus is available.

    A Sub-0.5Å Bandwidth with a 13mm Blocking Filter

    This Chromosphere model features a filter bandpass of 0.5Å FWHM or narrower. This extremely narrow window is the key to high-contrast views of surface features like filaments, plages, and active region details. While optimized for the chromosphere, this bandwidth is still wide enough to show prominences clearly against the blackness of space.

    The system has a 16mm clear etalon aperture (Daystar manual; Daystar's website gives a 19mm clear exit aperture) and an integrated 13mm blocking filter. The blocking filter is a non-removable, essential safety component that rejects out-of-band wavelengths before light reaches the eyepiece or camera. The entire filter assembly is self-contained and requires no user adjustment beyond the electronic tuning.

    PID-Controlled Heating and ±0.5Å Manual Wing Shift

    Daystar's etalons are tuned by precisely controlling their temperature. The Sol 80 uses an electronic PID (Proportional-Integral-Derivative) controller to heat the etalon to its target temperature and hold it there. An LED indicator shows the status: yellow while settling (approximately 5-6 minutes), green when on-band and ready to observe, and red for a fault such as low voltage.

    A manual tuning knob allows for a ±0.5Å wing shift in 0.1Å increments. This lets you slightly shift the filter's center wavelength off the main H-alpha line. This is used to enhance the visibility of Doppler-shifted features, moving toward or away from you: a feature moving towards you will be brighter in blue (counter-clockwise) wing shift, and one moving away will be reddened (clockwise). After each adjustment allow approximately 5-10 minutes for the filter to settle.

    12:1 Dual-Speed Rack & Pinion with Motor Support

    The Sol 80 is equipped with a Daystar-manufactured 12:1 dual-speed helical rack and pinion focuser. The mechanism provides smooth, precise focus adjustments, with a locking brake to hold position once focus is achieved. The focuser's ample travel accommodates a wide range of configurations, from a camera body mounted flush to the filter to visual use with a 2" diagonal.

    Designed with imagers in mind, the focuser is compatible with most third-party focus motors. It provides standard shaft sizes of 6mm (coarse) and 4mm (fine), along with three female M4 threaded holes for attaching motor brackets, enabling remote-controlled focusing during an imaging session.

    Eyepiece Selection for the 1400mm Focal Length

    Due to the long f/17.5 focal ratio, eyepiece choice is critical for performance. High-quality Plössl eyepieces in the 25mm to 40mm range are recommended. These designs offer high contrast and minimal internal scattering, which is essential for solar viewing. At long focal ratios a high-powered eyepiece can exceed Dawes' limit, so an eyepiece of 32mm or greater gives the best results; higher powers give a fuzzy disk without the ability to focus well.

    In Daystar's eyepiece comparisons, zooms and other fast wide-field designs typically performed very badly on Daystar applications. For best results, use eyepieces with fully multi-coated optics and blackened lens edges to maximize contrast and reveal the most subtle chromospheric details.

    Solar Imaging: Cameras, Reducers, and the Included Flat Cap

    For imaging, use a monochrome camera, as color sensors only use 1 in 4 pixels for red light, reducing both resolution and sensitivity. Short exposures (e.g., 1/15s to 1/500s) are necessary to "freeze" atmospheric seeing.

    • Newton's Rings: To combat interference patterns (Newton's Rings) common in monochromatic imaging, a tilt adapter may be required between the telescope and camera.
    • Focal Reducers: The 1400mm focal length produces a large image scale. To fit the full solar disk onto smaller camera sensors, an optional focal reducer can be used.
    • Flat Cap: An imaging Flat Cap is included in the box. This is used to take calibration frames (flat fields) to correct for dust motes and illumination variations.

    5V, 1.5A USB Power for Thermal Control

    The etalon's heating and tuning system requires a continuous power source for operation. The telescope is powered via a standard micro-B USB port and requires a 5V supply capable of delivering at least 1.5A. The manual notes that any user-supplied power source, such as a field battery, should be rated for at least 2 amps at 5 volts.

    An AC wall adapter (90-240VAC) is included, with interchangeable plugs for the US, UK, Europe, and Australia, allowing you to power the scope from any standard outlet. Computer USB ports and cell phone chargers do not normally supply the 1.5A this telescope needs.

    Daystar's Guidelines for Safe Solar Observation

    The Daystar Sol 80 is a fully integrated and safe solar telescope when used as directed. The internal filters are permanent and essential for safety. Never attempt to disassemble the telescope, focuser, or filter housing. Removal of any internal component will void the warranty and could result in unfiltered light which can cause blindness or damage to equipment.

    Always exercise caution and ensure all components are securely attached before pointing the telescope at the Sun. Never look up along the telescope towards the Sun, and do not leave the telescope unattended unless remote monitoring systems are in place. Daystar also asks owners to inform guest or novice observers of the special nature of the telescope so as not to imply that telescopic observing of the Sun is safe without proper filtration.

    2.8 kg Weight, Integrated Finder, and Vixen Dovetail

    Engineered for portability, the Sol 80 weighs just 2.8 kg (6.1 lb) with its mounting rings attached. The clever carry handle also incorporates a simple and effective solar finder: simply adjust the telescope's pointing until the bright dot of sunlight is centered on the finder's rear white screen.

    The telescope includes a Vixen-compatible dovetail bar for mounts that accept a Vixen-style dovetail. The dovetail also features a standard 1/4-20 tapped hole, allowing it to be mounted directly onto a sturdy photographic tripod for quick setup and grab-and-go observing sessions.

    Daystar Sol 80 vs. a Quark on an 80mm Refractor

    A common alternative to a dedicated solar scope is adding a Daystar Quark filter to an existing refractor. The two approaches differ in how the system is put together.

    • Quark: Daystar designs the Quark for F/4 to F/9 refractors, and its Quark manual recommends an Energy Rejection Filter on telescopes of 80mm aperture or more, or when tracking the Sun for long periods.
    • Sol 80: The objective, 4.3x telecentric barlow, 13mm blocking filter and etalon are built into one telescope, so there is no separate filter or barlow to fit and the solar finder is part of the carry handle.
    • Accessories: The Sol is compatible with Daystar's Quark accessories, including the 2" eyepiece adapter, imaging tilt adapters, focal reducers and battery.

    The Sol 80 suits observers who want an integrated H-alpha telescope; a Quark suits those who want to use a refractor they already own.

  • What is the difference between the Daystar Sol 80 Chromosphere and Prominence models?

    This is the Chromosphere model, which has a narrow bandpass of 0.5Å or less. This is ideal for maximizing contrast on solar surface details like filaments, plages, and active regions. Daystar also offers a Prominence model with a wider bandpass (more than 0.5Å FWHM), which can make prominences on the limb appear brighter, but at the cost of some surface contrast.

    What eyepiece works best to see the full disk with the Sol 80's 1400mm focal length?

    To view the full solar disk (which is about 0.5 degrees wide), you need a low-power eyepiece. With the Sol 80's 1400mm focal length, a 32mm or 40mm Plössl eyepiece is recommended. These will provide a wide enough true field of view to frame the entire Sun with room to spare, which is perfect for watching prominences on opposite limbs.

    Can I image the full solar disk with the Daystar Sol 80 and my camera?

    It depends on your camera's sensor size. The 1400mm focal length creates a large image. Many cameras with smaller sensors (like 1/3" or 1/2") will only capture a portion of the disk. To image the full disk with a smaller sensor, you would need to use an accessory focal reducer, which Daystar offers separately.

    Why does the Daystar Sol 80 telescope need USB power to work?

    The core of the filter is a solid etalon that must be precisely tuned to the 6562.8Å H-alpha wavelength. This is achieved by an internal heater that brings the etalon to a specific, stable temperature. The USB power runs this heating and control system. Without power, the filter is not on-band and you will not see any solar detail.

    What does the ±0.5Å wing shift tuning let me do?

    This feature allows you to slightly change the filter's target wavelength. It's used to study the Doppler effect in solar features. A solar flare or prominence moving towards you is "blue-shifted," and one moving away is "red-shifted." By tuning into the "blue wing" (counter-clockwise knob turn) or "red wing" (clockwise turn), you can make these moving features stand out with higher contrast.

    Do I need an Energy Rejection Filter (ERF) with the Daystar Sol 80?

    No separate front filter is needed. The Sol 80 is an integrated solar telescope: its built-in blocking filter transmits wavelengths near H-alpha and reflects the rest back out, and the etalon then passes a very narrow range of wavelengths. Never remove or disassemble any part of the filter assembly.

    How do I use the Sol 80's integrated solar finder?

    The carry handle has a built-in solar finder. It's a projection system. Point the telescope in the general direction of the Sun and look at the small white screen on the back of the handle. You will see a bright dot of light. Simply adjust the telescope's pointing until that bright dot is centered on the target screen. This means the Sun is now in the field of view of your eyepiece.

    What do the different LED colors on the Daystar Sol 80 mean?

    The LED indicates the status of the filter's thermal tuning system:

    • Yellow: The filter is settling to its operating temperature. This takes about 5-6 minutes.
    • Green: The filter is on-band and ready for observation.
    • Red: Indicates a fault such as low voltage. Ensure you are using the included AC adapter or a USB battery pack rated for at least 5V and 2A.

    My images have a strange pattern of rings or bands. How do I fix this?

    This pattern is called Newton's Rings, an interference effect in monochromatic H-alpha light: the sensor and its cover slip form a small interferometer inside the camera. To remove them, you need to slightly tilt the camera sensor. Optional tilt adapters are available specifically for this purpose.

    Can I see granulation with the Daystar Sol 80?

    No. Granulation is a feature of the photosphere, seen with a white-light solar filter, not a Hydrogen-Alpha feature. The Sol 80 shows the chromosphere: prominences, filaments, active regions, solar flares and spicules.

    What kind of mount do I need for the 2.8 kg Sol 80 telescope?

    With a weight of 2.8 kg (6.1 lb), the Sol 80 is quite light. It can be used on a sturdy photo tripod with a fluid head for quick visual sessions, or on a tracking mount for imaging. The included dovetail is Vixen-compatible, with a 1/4-20 tapped hole for a camera tripod.

  • Optical Design Achromatic air-spaced doublet, dedicated Hydrogen-Alpha solar telescope
    Aperture 80mm (3.15")
    Effective Focal Length 1400mm
    Focal Ratio f/17.5
    Field of View Passes the full solar disk
    Wavelength 6562.8 Å (656.28 nm), Hydrogen-Alpha
    Bandwidth Chromosphere model, 0.5Å FWHM or narrower (still shows prominences)
    Tuning Electronic PID-controlled thermal tuning, manual ±0.5Å wing shift in 0.1Å steps
    Settling Time Approximately 5-6 minutes after power-up or a wing shift
    Barlow Integrated, fully baffled 2-element 4.3x telecentric barlow optimized for 656nm
    Blocking Filter Integrated, 13mm
    Clear Aperture 16mm clear etalon aperture (manual); 19mm clear exit aperture (Daystar website)
    Eyepiece Side 1.25" female drawtube with brass compression ring; optional 2" accessory
    Focus Travel From a camera flush to the filter to visual use through a 2" diagonal; optimized for mid travel (1.25" eyepiece and diagonal)
    Focuser Daystar 12:1 dual-speed helical rack and pinion with locking brake
    Focus Motor Compatibility 6mm coarse and 5/32" (4mm) fine shafts; three female M4 holes for motor brackets; 34mm fine-focus reduction cone with knobs removed
    Dew Shield Locking, retractable
    Solar Finder Integrated in the carry handle
    Dovetail Vixen-compatible with 1/4-20 tapped hole for a camera tripod
    Power Required USB 5V, 1.5A, micro-B connector (required for operation)
    Power Supply Included 90-240VAC adapter with US, UK, Euro and Australian plugs
    Optional Battery 8-hour battery pack
    LED Indicator Yellow while settling, green when on band, red for a fault such as low voltage
    Operating Temperature 40-100°F ambient
    Dimensions 125mm wide, 166mm tall, 450-516mm long
    Weight 2.8 kg (6.1 lb) with rings
    Mount Included No
    Warranty 5 years
    Focal Length 1400 mm
    • Mounting Rings & Dovetail

      × 1

    • Carry Handle with Integrated Solar Finder

      × 1

    • Front and Rear Covers

      × 1

    • Flat Cap for Imaging

      × 1

    • AC Power Supply with US, UK, Euro & Australian Plugs

      × 1

    • USB Power Cable

      × 1

    • 1.25" Eyepiece Adapter

      × 1

    • Hard Case

      × 1

    • User Manual

      × 1

  • Daystar Filters Warranty