{"product_id":"dwarflab-draco-smart-telescope","title":"DWARFLAB DRACO Smart Telescope","description":"\u003cp\u003eSmart telescopes started by making astrophotography easier. The DWARFLAB DRACO Standard Edition takes the idea considerably further: it puts much of what normally lives in a conventional imaging rig into one portable instrument without giving up the simplicity that made smart telescopes appealing in the first place.\u003c\/p\u003e\n\n\u003cp\u003eAt the center is a 90mm (3.54\") f\/3.8 telephoto optical system with a 340mm focal length, a cooled 50.33-megapixel main sensor, a separate monochrome guide camera, autofocus, physical sensor rotation for field derotation and framing, built-in astronomical filters, automated calibration, and individual exposures as long as 300 seconds. A second 50.33-megapixel ultra-wide camera handles broad views of the sky, Milky Way imaging, landscapes, star trails, and other wide-field work.\u003c\/p\u003e\n\n\u003cp\u003eThat sounds more like the equipment list for a conventional astrophotography setup than a smart telescope. The difference is that DRACO arrives with all of it integrated. Put the telescope outside, connect through the DWARFLAB app, choose a target, and the system can handle finding, focusing, tracking, guiding, calibration, stacking, and much of the processing on its own. When you want more control, Pro Mode opens up exposure, gain, filter selection, and other imaging settings.\u003c\/p\u003e\n\n\u003cp\u003eThe Standard Edition is the more versatile DRACO for someone who wants deep-sky imaging, lunar and planetary work, wide-field photography, and convenient solar imaging in the same instrument. Its OD 5 solar filter is built into the internal filter system, so DRACO can switch into white-light solar mode through the app without requiring you to install a separate filter on the front of the telescope first. That's convenient in the backyard and particularly useful if you plan to operate DRACO remotely.\u003c\/p\u003e\n\n\u003ch3\u003eFeatures\u003c\/h3\u003e\n\n\u003cul\u003e \u003cli\u003e\n\u003cstrong\u003e90mm f\/3.8 telephoto imaging system.\u003c\/strong\u003e A substantial aperture for a compact smart telescope with a fast focal ratio suited to building signal efficiently on galaxies, nebulae, clusters, and other deep-sky targets.\u003c\/li\u003e \u003cli\u003e\n\u003cstrong\u003eCooled 50.33MP main sensor.\u003c\/strong\u003e Active cooling helps control thermal noise during long sessions, while 2×2 binning produces approximately 12MP deep-sky images with 2.394-micron effective pixels.\u003c\/li\u003e \u003cli\u003e\n\u003cstrong\u003eUp to 300-second exposures without conventional polar alignment.\u003c\/strong\u003e A dedicated monochrome guide camera works with physical sensor derotation to compensate for tracking error and field rotation.\u003c\/li\u003e \u003cli\u003e\n\u003cstrong\u003eFour internal telephoto filter positions.\u003c\/strong\u003e Astronomy, dark-frame, 13nm Hα + O III dual-narrowband, and OD 5 solar ND — giving you broadband deep sky, emission-nebula imaging, and white-light solar capability without swapping hardware.\u003c\/li\u003e \u003cli\u003e\n\u003cstrong\u003eApp-switchable solar imaging.\u003c\/strong\u003e The internal solar filter can be moved into place electronically, making sunspot and eclipse imaging especially convenient and giving the Standard Edition an advantage for remote solar operation.\u003c\/li\u003e \u003cli\u003e\n\u003cstrong\u003eSecond 50.33MP ultra-wide camera.\u003c\/strong\u003e An approximately 85.7° diagonal field for the Milky Way, star trails, landscapes, and broad night-sky scenes.\u003c\/li\u003e \u003cli\u003e\n\u003cstrong\u003eAuto and Pro Modes.\u003c\/strong\u003e Let DRACO manage the complete imaging sequence or take greater control over exposure, gain, filters, and other settings when you're ready.\u003c\/li\u003e \u003cli\u003e\n\u003cstrong\u003eFITS and TIFF export.\u003c\/strong\u003e You aren't locked into the image produced by the app. DRACO can provide imaging data for further processing in the astrophotography software of your choice.\u003c\/li\u003e \u003c\/ul\u003e\n\n\u003ch3\u003eBuilt Like an Imaging Rig, Used Like a Smart Telescope\u003c\/h3\u003e\n\n\u003cp\u003eDRACO's 90mm aperture is substantial for a compact smart telescope, and at f\/3.8 the optical system is fast enough to make productive use of the clear hours you actually get. The 340mm focal length also lands in a useful middle ground: enough reach for galaxies, globular clusters, planetary nebulae, and smaller emission regions without becoming so narrow that larger deep-sky objects are difficult to frame.\u003c\/p\u003e\n\n\u003cp\u003eTargets such as M51, M81 and M82, M27, and M13 sit comfortably within its reach, while the Orion Nebula, Rosette Nebula, Lagoon Nebula, and other medium-sized emission regions remain natural subjects. When one frame isn't enough, DRACO's mosaic mode can automatically capture adjoining sections and combine them into a larger field.\u003c\/p\u003e\n\n\u003cp\u003eThe telephoto camera uses a 1\/1.3\" 50.33MP sensor with 1.197-micron native pixels. For deep-sky imaging, DRACO normally uses 2×2 binning, combining four adjacent pixels into one 2.394-micron effective pixel and producing approximately 12-megapixel output. The point isn't a larger megapixel number; the larger effective pixels improve signal collection for faint targets. For brighter objects such as the Sun, Moon, and planets, DRACO can use the finer native 1×1 sampling and crop around the target.\u003c\/p\u003e\n\n\u003cp\u003eA separate monochrome guide camera continuously watches star movement while the mount tracks. At the same time, DRACO physically rotates the main imaging sensor to compensate for field rotation. Together with the drive system, that allows individual exposures as long as 300 seconds without the conventional polar-alignment routine associated with a traditional equatorial imaging setup.\u003c\/p\u003e\n\n\u003cp\u003eThe sensor rotator also handles composition. Change the framing angle in the app and the imaging sensor physically rotates to follow it, so you're not stuck with whatever orientation the telescope happens to give you.\u003c\/p\u003e\n\n\u003cp\u003eSensor cooling helps control thermal noise during long sessions, while heat generated within the system is redirected to help resist dew on the main optics. Autofocus, dark-frame capture, flat and bias calibration data, guiding, and live stacking are all part of the system. An experienced imager will recognize every one of those jobs. DRACO simply removes much of the separate hardware, cabling, spacing work, and setup normally required to accomplish them.\u003c\/p\u003e\n\n\u003ch3\u003eThe Standard Edition Difference\u003c\/h3\u003e\n\n\u003cp\u003eThe Standard Edition carries four telephoto filter positions inside the telescope: an Astronomy filter, an opaque dark-frame position, a 13nm Hα + O III dual-narrowband filter, and an OD 5 neutral-density solar filter.\u003c\/p\u003e\n\n\u003cp\u003eFor galaxies, clusters, and other broadband targets, the Astronomy filter preserves a broad range of useful starlight. For emission nebulae, the Hα + O III dual-narrowband filter concentrates on the 656.3nm hydrogen-alpha and 500.7nm oxygen III emission lines while rejecting much of the broadband background. That makes targets such as the Rosette, Orion, Lagoon, Swan, Crescent, and other emission nebulae particularly well suited to the system.\u003c\/p\u003e\n\n\u003cp\u003eThe narrowband filter can also improve contrast on emission nebulae from suburban locations and extend useful imaging into nights when some moonlight is present. Darker skies still help — particularly on broadband targets such as galaxies — but you don't necessarily have to wait for a perfect moonless trip to a remote site every time you want to collect useful nebula data.\u003c\/p\u003e\n\n\u003cp\u003eThen there is the Sun.\u003c\/p\u003e\n\n\u003cp\u003eThe Standard Edition's OD 5 solar filter is already inside the telescope. Select solar imaging in the app and DRACO can move the proper filter into position without requiring you to attach a separate front filter first. The system can then locate, center, focus, and track the Sun automatically.\u003c\/p\u003e\n\n\u003cp\u003eThis is white-light solar imaging, so you're looking for sunspots, visible active-region structure, and events such as partial or total solar eclipses. It is not an H-alpha solar telescope and should not be confused with one.\u003c\/p\u003e\n\n\u003cp\u003eThe internal solar filter also gives the Standard Edition an important advantage for remote operation. With DWARFLAB's PhotonLink remote-access system, the telescope can move between nighttime and solar operation without someone having to physically visit the instrument just to install a solar filter.\u003c\/p\u003e\n\n\u003cp\u003eIf your priority is instead SHO\/Hubble-palette imaging of emission nebulae, the DRACO SHO Edition is the version to consider. It replaces the Standard model's internal solar-filter position with a second S II + O III dual-narrowband filter, giving the system access to the sulfur II, hydrogen-alpha, and oxygen III emission bands used for SHO processing. The SHO Edition includes an external magnetic solar filter for white-light solar imaging instead.\u003c\/p\u003e\n\n\u003ch3\u003eFrom First Image to Your Own Processing\u003c\/h3\u003e\n\n\u003cp\u003eThe smart part of DRACO isn't simply GoTo. Auto Mode can manage the complete imaging sequence for someone who wants to select an object and start collecting data without first learning every part of a traditional astrophotography system. Target acquisition, autofocus, guiding, tracking, calibration, live stacking, and processing can all take place within the DWARFLAB workflow.\u003c\/p\u003e\n\n\u003cp\u003eThat doesn't mean you're locked into automatic processing. Pro Mode gives you more control over the capture settings, while FITS and TIFF export let you take the imaging data into your preferred astrophotography software and decide for yourself how the final image should look.\u003c\/p\u003e\n\n\u003cp\u003eMulti-night stacking lets you continue building signal on the same target over several sessions rather than treating every night as a separate project. Scheduled imaging can also be set in advance, allowing DRACO to wake, acquire the target, track, and capture while you're doing something else — including sleeping.\u003c\/p\u003e\n\n\u003cp\u003eMosaic mode handles targets that won't comfortably fit into a single telephoto frame. Extend the area in the star map and DRACO automatically captures the adjoining sections needed to build the larger view.\u003c\/p\u003e\n\n\u003cp\u003eThe second ultra-wide camera adds another side to the instrument. With a 23.3mm full-frame-equivalent focal length and roughly 85.7° diagonal field, it can record the Milky Way, star trails, landscapes, and broad night-sky scenes while the 340mm telephoto system handles deeper work. You're not limited to one scale of photography simply because you brought one telescope.\u003c\/p\u003e\n\n\u003cp\u003eAll of this is packaged into a 12.1 lb (5.5 kg) body with a built-in 10,000mAh battery rated for approximately five hours of operation. Internal storage is 128GB, and Wi-Fi, Bluetooth, NFC, and USB-C connectivity are built in. USB Ethernet connectivity is also supported when a wired connection makes more sense for a long-term or remote installation.\u003c\/p\u003e\n\n\u003ch3\u003eWhat's Included\u003c\/h3\u003e\n\n\u003cul\u003e \u003cli\u003eDWARFLAB DRACO Standard Smart Telescope\u003c\/li\u003e \u003cli\u003eDRACO tripod\u003c\/li\u003e \u003cli\u003eUSB-C data cable\u003c\/li\u003e \u003cli\u003eLens cleaning cloth\u003c\/li\u003e \u003c\/ul\u003e\n\n\u003ch3\u003eFrequently Asked Questions\u003c\/h3\u003e\n\n\u003cp\u003e\u003cstrong\u003eWhat is the difference between the DRACO Standard and SHO versions?\u003c\/strong\u003e\u003cbr\u003e Both versions share the same main optics, cameras, guiding system, cooling, mount, storage, and software platform. The difference is the fourth telephoto filter position. The Standard Edition uses an internally switchable OD 5 solar filter. The SHO Edition uses that position for an S II + O III dual-narrowband filter instead and includes an external magnetic solar filter for white-light solar work.\u003c\/p\u003e\n\n\u003cp\u003e\u003cstrong\u003eDo I need to polar align DRACO for long exposures?\u003c\/strong\u003e\u003cbr\u003e No. DRACO combines built-in guiding with physical sensor derotation to compensate for tracking error and field rotation, allowing individual exposures as long as 300 seconds without the conventional polar-alignment routine of a traditional equatorial imaging setup.\u003c\/p\u003e\n\n\u003cp\u003e\u003cstrong\u003eWhy does a 50-megapixel sensor produce roughly 12MP deep-sky images?\u003c\/strong\u003e\u003cbr\u003e For deep-sky work, DRACO normally uses 2×2 pixel binning. Four 1.197-micron native pixels are combined into one 2.394-micron effective pixel, improving signal collection while producing approximately 12-megapixel output. For brighter solar-system targets, the telescope can use the finer native 1×1 sampling.\u003c\/p\u003e\n\n\u003cp\u003e\u003cstrong\u003eCan I process DRACO data myself?\u003c\/strong\u003e\u003cbr\u003e Yes. DRACO supports FITS and TIFF output for users who want to take the processing further themselves, along with JPG and PNG formats for quicker sharing and finished-image workflows.\u003c\/p\u003e\n\n\u003cp\u003e\u003cstrong\u003eCan DRACO work from a light-polluted location?\u003c\/strong\u003e\u003cbr\u003e Yes. Brighter broadband targets remain accessible, and the built-in Hα + O III dual-narrowband filter can substantially improve contrast on emission nebulae by rejecting much of the broadband background. Darker skies will still improve what the telescope can record, especially on faint galaxies and other broadband targets.\u003c\/p\u003e\n\n\u003cp\u003e\u003cstrong\u003eCan the Standard Edition make SHO\/Hubble-palette images?\u003c\/strong\u003e\u003cbr\u003e Not in the same way as the SHO Edition. The Standard model has an Hα + O III dual-narrowband filter but does not have the SHO model's additional S II + O III filter. If SHO\/Hubble-palette imaging is one of the main reasons you're buying DRACO, choose the SHO Edition.\u003c\/p\u003e\n\n\u003cp\u003e\u003cstrong\u003eCan I use DRACO for solar imaging?\u003c\/strong\u003e\u003cbr\u003e Yes. The Standard Edition has an OD 5 neutral-density solar filter built into the telescope and switchable through the app. It is intended for white-light solar imaging, including sunspots and eclipses. It is not an H-alpha solar telescope.\u003c\/p\u003e\n\n\u003cp\u003e\u003cstrong\u003eWhy choose the Standard Edition instead of the SHO?\u003c\/strong\u003e\u003cbr\u003e Choose the Standard Edition if you want the broadest all-around DRACO and value convenient solar imaging alongside galaxies, clusters, emission nebulae, lunar and planetary work, and wide-field photography. Its internally switchable solar filter is particularly useful for remote operation because no one has to visit the telescope to install a filter before changing from nighttime to solar imaging.\u003c\/p\u003e\n\n\u003cp\u003e\u003cstrong\u003eWho is the Standard Edition for?\u003c\/strong\u003e\u003cbr\u003e It's the version we'd choose for someone who wants DRACO to do a little of almost everything. It gives you serious deep-sky capability, narrowband Hα + O III imaging, lunar and planetary imaging, a second ultra-wide camera, and white-light solar imaging without requiring you to attach a separate front filter each time.\u003c\/p\u003e\n\n\u003ch3\u003eFinal Thoughts\u003c\/h3\u003e\n\n\u003cp\u003eThe Standard Edition makes the most sense when versatility is the priority. Its 90mm f\/3.8 optical system gives it meaningful deep-sky capability, the dedicated guide camera and physical sensor derotation make long exposures practical without building a conventional equatorial imaging rig, and the Hα + O III filter gives emission-nebula imaging a real place in the system.\u003c\/p\u003e\n\n\u003cp\u003eThen, when the Sun comes up, the telescope isn't finished for the day. The built-in solar filter can be switched into place through the app and DRACO becomes a white-light solar imager without adding another piece of hardware to the front of the telescope.\u003c\/p\u003e\n\n\u003cp\u003eYou can begin with something as simple as, “find this and photograph it for me,” then grow into longer integrations, multi-night projects, mosaics, manual capture settings, and your own processing of the exported data. You aren't forced to learn all of that before the telescope becomes useful, and you don't have to replace it simply because you decide you want more control later.\u003c\/p\u003e\n\n\u003cp\u003eThat's where the Standard Edition earns its place. It isn't the DRACO with fewer features than the SHO model. It's the DRACO built for the observer who would rather have one instrument that can move easily from galaxies and nebulae at night to the Moon, planets, Milky Way, and Sun whenever the opportunity presents itself.\u003c\/p\u003e\n\u003ch2\u003eTech Details:\u003c\/h2\u003e\n\u003ctable style=\"width:100%; border-collapse: collapse;\"\u003e\u003ctbody\u003e\n\u003ctr style=\"background-color: #f0f4f8;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003eTelephoto Aperture\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003e90mm (3.54\")\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr style=\"background-color: #ffffff;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003eTelephoto Focal Length\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003e340mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr style=\"background-color: #f0f4f8;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003eFocal Ratio\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003ef\/3.8\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr style=\"background-color: #ffffff;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003eTelephoto Astronomy FOV\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003e2.059° diagonal\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr style=\"background-color: #f0f4f8;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003eWide-Angle Focal Length\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003e5.56mm; 23.3mm full-frame equivalent\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr style=\"background-color: #ffffff;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003eWide-Angle FOV\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003e85.74° diagonal\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr style=\"background-color: #f0f4f8;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003eTelephoto Sensor\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003eOV50Q40, 50.33MP, 1\/1.3\" format\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr style=\"background-color: #ffffff;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003eWide-Angle Sensor\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003eOV50E40, 50.33MP\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr style=\"background-color: #f0f4f8;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003eGuide Sensor\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003eOS04C1B monochrome, 4.09MP\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr style=\"background-color: #ffffff;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003eNative Pixel Size\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003e1.197µm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr style=\"background-color: #f0f4f8;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003eDeep-Sky Effective Pixel Size\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003e2.394µm with 2×2 binning\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr style=\"background-color: #ffffff;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003eDeep-Sky Output\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003eApproximately 12MP\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr style=\"background-color: #f0f4f8;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003eMaximum Single Exposure\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003e300 seconds\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr style=\"background-color: #ffffff;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003eStandard Telephoto Filters\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003eAstronomy 440–680nm; dark; Hα + O III dual-narrowband, 13nm each; OD 5 solar ND\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr style=\"background-color: #f0f4f8;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003eField Derotation\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003ePhysical CMOS sensor rotation\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr style=\"background-color: #ffffff;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003eGuiding\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003eBuilt-in monochrome guide camera\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr style=\"background-color: #f0f4f8;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003eCooling\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003eBuilt-in main-sensor cooling\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr style=\"background-color: #ffffff;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003eStorage\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003e128GB internal\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr style=\"background-color: #f0f4f8;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003eBattery\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003eBuilt-in 7.7V, 10,000mAh; approximately 5-hour rated operation\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr style=\"background-color: #ffffff;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003eConnectivity\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003eWi-Fi, Bluetooth, NFC, USB-C; USB Ethernet supported\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr style=\"background-color: #f0f4f8;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003eFile Formats\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003eJPG, PNG, MP4, FITS, TIFF\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr style=\"background-color: #ffffff;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003eCompatible Mobile OS\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003eiOS and Android\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr style=\"background-color: #f0f4f8;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003eWeight\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003e12.1 lb (5.5 kg)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr style=\"background-color: #ffffff;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003eDimensions\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003eApprox. 15.2 × 7.7 × 5.2\" (385.85 × 196.28 × 133.25mm)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr style=\"background-color: #f0f4f8;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003eOperating Temperature\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003e-4° to 113°F (-20° to 45°C)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003c\/tbody\u003e\u003c\/table\u003e","brand":"Dwarflab","offers":[{"title":"Default Title","offer_id":56109215744073,"sku":"DRACO","price":1399.0,"currency_code":"USD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0573\/7974\/9961\/files\/img_draco_page_40_tripod_gallery_4.webp?v=1789501069","url":"https:\/\/astronomics.com\/products\/dwarflab-draco-smart-telescope","provider":"Astronomics","version":"1.0","type":"link"}