Explore One STAR50APP User manual

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SUN HAZARD — Never look directly at the sun
with this device.
WARNING:
CHOKING HAZARD — Small parts.
Not for children under 3 years.
WARNING:
Contains button or coin cell battery.
Hazardous if swallowed — see instructions.
WARNING:
The lens contains lead that may be harmful.
Wash hands after touching.
WARNING:
This product can expose you to chemicals including lead,
which is known to the State of California to cause cancer
and birth defects or other reproductive harm.
For more information go to www.P65Warnings.ca.gov.
WARNING:
88-34550
EN
10 +
INCLUDED
X1
CR2032
3V
STAR50APP
50MM TELESCOPE W/PANHANDLE MOUNT
INSTRUCTION MANUAL

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Customer Service: Call 1-866-252-3811
• SUN WARNING: NEVER ATTEMPT TO OBSERVE THE SUN WITH THIS DEVICE! OBSERVING THE SUN  EVEN
FOR A MOMENT  WILL CAUSE INSTANT AND IRREVERSIBLE DAMAGE TO YOUR EYE OR EVEN BLINDNESS.
EYE DAMAGE IS OFTEN PAINLESS, SO THERE IS NO WARNING TO THE OBSERVER THAT THE DAMAGE HAS
OCCURRED UNTIL IT IS TOO LATE. DO NOT POINT THE DEVICE AT OR NEAR THE SUN. DO NOT LOOK
THROUGH THE DEVICE AS IT IS MOVING. CHILDREN SHOULD ALWAYS HAVE ADULT SUPERVISION WHILE OBSERVING.
• RESPECT PRIVACY: WHEN USING THIS DEVICE, RESPECT THE PRIVACY OF OTHER PEOPLE. FOR EXAMPLE, DO NOT
USE IT TO LOOK INTO PEOPLE’S HOMES.
• CHOKING HAZARD: CHILDREN SHOULD ONLY USE DEVICE UNDER ADULT SUPERVISION. KEEP PACKAGING
MATERIALS LIKE PLASTIC BAGS AND RUBBER BANDS OUT OF THE REACH OF CHILDREN AS THESE
MATERIALS POSE A CHOKING HAZARD.
• RISK OF BLINDNESS: NEVER USE THIS DEVICE TO LOOK DIRECTLY AT THE SUN OR IN THE DIRECT PROXIMITY OF THE
SUN. DOING SO MAY RESULT IN A PERMANENT LOSS OF VISION.
• RISK OF FIRE: DO NOT PLACE DEVICE, PARTICULARLY THE LENSES, IN DIRECT SUNLIGHT. THE CONCENTRATION OF
LIGHT RAYS COULD CAUSE A FIRE.
• DO NOT DISASSEMBLE THIS DEVICE: IN THE EVENT OF A DEFECT, PLEASE CONTACT YOUR DEALER. THE DEALER
WILL CONTACT THE CUSTOMER SERVICE DEPARTMENT AND CAN SEND THE DEVICE IN TO BE REPAIRED IF
NECESSARY.
• DO NOT SUBJECT THE DEVICE TO TEMPERATURES EXCEEDING 60 °C 140 °F.
• DISPOSAL: KEEP PACKAGING MATERIALS, LIKE PLASTIC BAGS AND RUBBER BANDS, AWAY FROM
CHILDREN AS THEY POSE A RISK OF SUFFOCATION. DISPOSE OF PACKAGING MATERIALS AS LEGALLY
REQUIRED. CONSULT THE LOCAL AUTHORITY ON THE MATTER IF NECESSARY AND RECYCLE MATERIALS
WHEN POSSIBLE.
• THE WEEE SYMBOL IF PRESENT INDICATES THAT THIS ITEM CONTAINS ELECTRICAL OR ELECTRONIC
COMPONENTS WHICH MUST BE COLLECTED AND DISPOSED OF SEPARATELY.
• NEVER DISPOSE OF ELECTRICAL OR ELECTRONIC WASTE IN GENERAL MUNICIPAL WASTE. COLLECT AND
DISPOSE OF SUCH WASTE SEPARATELY.
• MAKE USE OF THE RETURN AND COLLECTION SYSTEMS AVAILABLE TO YOU, OR YOUR LOCAL RECYCLING PROGRAM.
CONTACT YOUR LOCAL AUTHORITY OR PLACE OF PURCHASE TO FIND OUT WHAT SCHEMES ARE AVAILABLE.
• ELECTRICAL AND ELECTRONIC EQUIPMENT CONTAINS HAZARDOUS SUBSTANCES WHICH, WHEN DISPOSED OF
INCORRECTLY, MAY LEAK INTO THE GROUND. THIS CAN CONTRIBUTE TO SOIL AND WATER POLLUTION WHICH IS
HAZARDOUS TO HUMAN HEALTH, AND ENDANGER WILDLIFE.
• IT IS ESSENTIAL THAT CONSUMERS LOOK TO RE-USE OR RECYCLE ELECTRICAL OR ELECTRONIC WASTE TO AVOID IT
GOING TO LANDFILL SITES OR INCINERATION WITHOUT TREATMENT.
BUTTON/COIN BATTERY WARNING: THIS PRODUCT CONTAINS A BUTTON OR COIN CELL BATTERY. A SWALLOWED
BUTTON OR COIN CELL BATTERY CAN CAUSE INTERNAL CHEMICAL BURNS IN AS LITTLE AS TWO HOURS AND LEAD
TO DEATH. DISPOSE OF USED BATTERIES IMMEDIATELY. KEEP NEW AND USED BATTERIES AWAY FROM CHILDREN. IF
YOU THINK BATTERIES MIGHT HAVE BEEN SWALLOWED OR PLACED INSIDE ANY PART OF THE BODY, SEEK IMMEDIATE
MEDICAL ATTENTION.
IMPORTANT SAFETY INSTRUCTIONS
READ AND FOLLOW THE INSTRUCTIONS BEFORE USE.
KEEP THESE INSTRUCTIONS FOR LATER USE.

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What’s Included:
Available Downloads Visit:
www.esmanuals.com
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Parts Overview
1. 50 mm Objective Lens
2. Pan Tilt Mount
3. Tripod with accessory tray
4. Optical Tube Assembly (OTA) with Dew Shield
5. Focus Wheel
6. Diagonal
7. 1.25” Eyepieces (12.5 mm and 20 mm)
8. Smartphone Mount w/Bluetooth
9. Panhandle
10. Focuser
Phone not included.

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How To Set Up
Note: We recommend assembling your telescope for the first time in the daylight or in a lit room so
that you can familiarize yourself with assembly steps and all components.
• Open the tripod until the tripod spreaders are fully extended. Put the accessory tray in place
and turn it clockwise until stable. To set the tripod height, turn the pressure fitting on each leg
counterclockwise until loose. Extend or retract the leg to the desired setting, then tighten the
pressure fitting until snug.
• Thread the panhandle clockwise onto the tripod head.
• Set the optical tube assembly on the tripod head and align the tab on the bottom of the telescope
tube with the slot in the tripod head. Thread the front tension wheel until snug, then tighten the side
tension thumbscrew. Be careful not to over-tighten either screw.
• Insert the diagonal into the focuser and secure it by tightening the thumbscrews.
• Slide the red dot viewfinder into the finder bracket that is already mounted on the telescope tube.
• Place your chosen eyepiece into the diagonal. We recommend starting with the 20mm because it will
provide the widest field of view.
Using Your Telescope:
Put the 20mm eyepiece into the focuser to get the widest field of view. This wider field of view will
make it easier to locate and track objects. Use the panhandle to move the scope up, down and side to
side until your target comes into view in the eyepiece. It is important to remember that the rotation
of the Earth means objects will move out of your eyepiece fairly quickly. Once you have found and
focused on your desired target, you can track it as it journeys across the night sky using the panhandle.
To get a closer look at an object, take out the 20mm
eyepiece and replace it with the 12.5mm eyepiece.
This will increase the magnification from 30x to 48x.
Note: Terrestrial objects will appear reversed due to the
optical setup. This rotation is perfectly normal for a refractor using a standard diagonal, and it will
not affect astronomical viewing.
Cleaning:
Your telescope is a precision optical device and keeping the optics free of dust and dirt is crucial for
optimal performance. To clean the lenses (objective and eyepiece) use only a photo-grade soft brush
or a lint-free cloth, like a microfiber cloth. Do not press down too hard while cleaning, as this might
scratch the lens. If necessary, the cleaning cloth can be moistened with an optical glass cleaning fluid
and the lens wiped clean using very little pressure. The eyepiece is NOT waterproof so do not spray
fluids directly onto the glass or dip it in water. Never use harsh detergents! After you have finished
cleaning an eyepiece, allow it to fully dry before storing.
Make sure your telescope is always protected against dust and dirt.
After use, leave it in a warm room to dry off before storing.
Troubleshooting Guide:
Problem Solution
No picture Remove dust protection cap.
Blurred picture Adjust focus using focus wheel.
No focus possible Wait for temperature to balance out.
Bad quality Never observe through a glass surface such as a window.
Focal Length Eyepiece Magnification
600mm 20mm 30x
600mm 12.5mm 48x

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To download the application:
Method 1:
Using your smart device, scan the QR code on the left
to download and install the ARTelescope-3L App.
Method 2:
Download and install the ARTelescope-3L App by
searching through the Apple Store or Google Play.
Using the ARTelescope-3L App:
After launching the application, tap the “Star Seeking” icon in the middle of the screen to access the
Bluetooth interface. Note: Bluetooth on your device will need to be enabled.
If the device is placed in the telescope bracket, click “Automatic Search” to match and enter the AR star
search module.
To access the language selection function:
Go to the home menu screen and click the globe icon in the upper left corner to enter the language
switch function.
To activate the application:
After installing, open the application. For the ARTelescope-3L to function
properly, you will need to allow it to access the camera, location and
Bluetooth functions on your smart device. Next, select your preferred
language. Activate the application by scanning the activation QR code
pictured here.
Important: Please keep this activation
code to be able to activate more devices.
Activation Code
Download the App
How to Install & Use the App
ARTelescope-3L

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To access the encyclopedia for constellations:
Go to the home menu screen, click the encyclopedia icon in the lower left corner to access information
on constellations and solar system objects. Tap on an object for information that includes pictures, text
and audio.
To access the encyclopedia for solar system objects:
Go to the encyclopedia screen, click the “solar system” icon to access information about the solar
system objects. Tap on an object for information that includes pictures, text and audio.
To access the 3D assembly animation:
Go to the home menu screen, click the upper right corner to enter the 3D assembly animation of
the telescope, and click the animation play button to watch the 3D assembly animation in the freely
rotating interface.

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To access the constellation quiz function:
Go to the main home screen and tap the icon in the lower left corner to enter the multiple
choice quiz mode.
To access the AR constellation photo function:
Go to the home menu screen, click the AR constellation function in the lower right. The names and
outlines of constellations in the viewing area will appear as you move your device across the night
sky. You can take a photo of the constellation in AR mode by allowing the application to access your
device’s camera.
Notes:
• The application needs to keep the device network in a normal state during the activation process.
• Permission to open the camera, album, and location of the device will pop up when the App is
launched for the first time. Please tap “Allow” to confirm approval.
• Gyroscope standard of the equipment. When the position deviation of the star finder module is large,
manual calibration of the equipment’s position and direction can be carried out by calibrating the
Magnetometer in settings.

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Observing Tips:
Star hopping
Star hopping is a technique used by amateur astronomers to navigate the night sky. By using easily
recognizable constellations and asterisms as a guide, an observer can locate stars and other objects.
For example, Polaris, which is commonly referred to as The North Star, can be located quickly using
star hopping. First, find the Big Dipper asterism in the Ursa Major constellation. The popular pattern is
defined by seven stars, and the two stars on the front edge of the Big Dipper’s “bowl” are Merak and
Dubhe. Next, draw an imaginary line from the bottom star (Merak) on this front edge through the top
star (Dubhe) on the front edge. Follow the line to the first bright star you see. That should be Polaris.
Finally, to verify your finding, locate the Little Dipper asterism. Polaris is the anchor star at the end of
the Little Dipper’s “handle.”
Image credit: Howard Eskildsen
Note: Images are for illustration purposes only. Quality of your image may very depending upon atmospheric conditions and location.
Possible Objects for Observation:
What you can observe at any one time in your telescope
depends on several factors beyond aperture and magnification.
These factors include location, date, time and sky conditions.
The following are all objects that can be seen with the unaided
eye and/or binoculars. Your telescope can enhance views of any
of these objects if the observing conditions are right.
The Moon:
Diameter: 3,476 km
Distance: Approximately 384,401 km
The Moon is the Earth’s only natural satellite, and it is the
second brightest object in the sky (after the Sun). Although it
is our closest neighbor, a lot of people have never really taken
a good long like at the Moon. With your telescope, you should
be able to see several interesting lunar features. These include
lunar maria, which appear as vast plains, and some of the larger
craters. The best views will be found along the terminator, which
is the edge where the visible and shadowed portions of the
Moon meet.
BIG DIPPER
LITTLE DIPPER
POLAR STAR
CASSIOPEIA
Caph
Zeta Beta
Kochab
Pherkad
Gamma
Eta
Epsilon
Delta
Alpha
Shedar
Cih
Ksora
Segin
Alkaid
Alcor Mizar
Alioth
Megrez
Phecda
Merak
Dubhe
Note: The positioning of the Big Dipper in relation to the Little Dipper does not change, but the
orientation of both in the night sky will rotate throughout the year due to the motion of the Earth.

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Orion Nebula(M42):
Right ascension: 05: 35.4 (hours: minutes)
Declination: -05: 27 (degrees: minutes)
Distance: Approximately 1,344 light years
The Orion Nebula is a vast star-forming region located in
the “sword” branching off of the famous Orion’s Belt. Also
known as Messier 42, this diffuse nebula is bright enough to
see with the unaided eye — although it will only appear as a
slightly foggy star. However, with your telescope, you can see
many of the beautiful details, such as the billowing clouds of
gas and dust where new stars are being born.
Image credit: NASA, ESA, M. Robberto (Space Telescope Science Institute/ESA)
and the Hubble Space Telescope Orion Treasury Project Team
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Pleiades Star Cluster(M45):
Right ascension: 03: 47.0 (hours: minutes)
Declination: +24: 07 (degrees: minutes)
Distance: Approximately 444 light years
The Pleiades Star Cluster is a group of brilliant blue
stars located in the Taurus Constellation. Also known
as Messier 45 or “Seven Sisters”, this open star cluster
consists of more than 1,000 confirmed stars, although
an average of only six are visible to the unaided eye.
With your telescope, you can quickly reveal some
of the more elusive members of this legendary and
beautiful cluster.
Image credit: NASA/JPL-Caltech/UCLA
Dumbbell Nebula(M27)
Right ascension: 19:59.6 (hours: minutes)
Declination: +22:43 (degrees: minutes)
Distance: Approximately 1,360 light years
The Dumbbell Nebula was the first planetary nebula
ever discovered. It is one of the most popular sights
in the Vulpecula constellation. Easy to find with
binoculars and amazing in a telescope, the shape of
this bright, double-lobed nebula has been compared
to a dumbbell, an hourglass or an apple core. As an
added bonus, the white dwarf that lies at the heart of
the Dumbbell Nebula is larger than any other star of
its kind.
Image credit: NASA/JPL-Caltech/Harvard-Smithsonian CfA
Andromeda Galaxy(M31):
Right ascension: 00: 42.7 (hours: minutes)
Declination: +41: 16 (degrees: minutes)
Distance: Approximately 2.54 million light years
The Andromeda Galaxy is the closest major galaxy
to our own Milky Way. Also known as Messier 31,
this famous spiral galaxy is part of the Local Group
of galaxies. Although it is technically bright enough
to see with the unaided eye under a very dark sky,
your telescope may show its bright center, hints of
its spiral structure and its much smaller companion
galaxies known as M32 and M110.
Image credit: NASA/JPL-Caltech
Note: Images are for illustration purposes only. Quality of your image may very depending upon atmospheric conditions and location.

1010
Light
Light
Secondary Mirror
Primary Mirror
(Objective)
Focuser
Focuser
Light
Light
Objective Lens
Light
Light
Secondary Mirror
Primary Mirror (Objective)
Correcting Lens
Reflector
(Newtonian)
Refractor
Catadioptric
(Maksutov-Cassegrain/
Schmidt-Cassegrain)
Light
Light
Secondary Mirror
Primary Mirror
(Objective)
Focuser
Focuser
Light
Light
Objective Lens
Light
Light
Secondary Mirror
Primary Mirror (Objective)
Correcting Lens
Reflector
(Newtonian)
Refractor
Catadioptric
(Maksutov-Cassegrain/
Schmidt-Cassegrain)
Light
Light
Secondary Mirror
Primary Mirror
(Objective)
Focuser
Focuser
Light
Light
Objective Lens
Light
Light
Secondary Mirror
Primary Mirror (Objective)
Correcting Lens
Reflector
(Newtonian)
Refractor
Catadioptric
(Maksutov-Cassegrain/
Schmidt-Cassegrain)
Reflector
A reflector telescope uses mirrors to gather and focus light. Light enters the telescope through its
open front end and travels to the concave primary mirror at the back. From there the light is reflected
back up the tube to a flat secondary mirror, which sits at a 45° angle in relation to the eyepiece. Light
bounces off of this secondary mirror and out through the eyepiece. A reflector telescope is designed
for astronomical use. Terrestrial objects may appear inverted, sideways or at an angle depending on
how your tube is oriented due to optical design. This rotation is perfectly normal on all Newtonian
reflectors and will not affect astronomical viewing.
Refractor:
A refracting telescope uses a collection of lenses to gather and focus light. A refractor’s views will
be upside down if a diagonal is not in use. A standard diagonal will generate a “right side up” image,
however, it will rotate the image on the vertical axis (mirror image). To get the “right side up” image
without the rotation, you will need to use a special diagonal with an erect image prism.
Catadioptric:
A catadioptric telescope uses a combination of mirrors and lenses to gather and focus light. Popular
catadioptric designs include the Maksutov-Cassegrain and Schmidt-Cassegrain.
Types Of Telescopes:

1111
Aperture:
This figure, which is usually expressed in millimeters, is the diameter of a telescope’s light-gathering
surface (objective lens in a refractor or primary mirror in a reflector). Aperture is the key factor in
determining the brightness and sharpness of the image.
Objective Lens:
The objective lens is the main light-gathering component of a refractor telescope. It is actually
composed of several lens elements.
Diagonal:
This accessory houses a mirror that deflects the ray of light 90 degrees. With a horizontal telescope
tube, this device deflects the light upwards so that you can comfortably observe by looking downwards
into the eyepiece. The image in a standard diagonal mirror appears upright, but rotated around its
vertical axis (mirror image). To get an image without this rotation, you will need to use a special
diagonal with an erect image prism.
Eyepiece:
An eyepiece is an optical accessory comprised of several lens elements. It determines the magnification
of a particular observing setup.
Primary Mirror:
The primary mirror is the principle light-gathering surface of a reflector telescope.
Secondary Mirror:
A secondary mirror is a small mirror that sits at a 45° angle in relation to the primary mirror of a
reflecting telescope. Light from the primary mirror is reflected back up the tube to the secondary
mirror. The light is directed from this mirror up into the eyepiece.
Objective Lens
Aperture
(mm)
Aperture
(mm)
Eyepiece
Diagonal Focal Point
Focal Point
Focal Length Telescope
(mm)
Focal Length Telescope
(mm)
Focal Length
Eyepiece
(mm)
Focal Length
Eyepiece
(mm)
Focuser
Secondary
Mirror
Primary Mirror
(Objective)
Focuser
Eyepiece
Telescope Terms to Know:

1212
Magnification:
The magnification corresponds to the difference between observation with the naked eye and
observation through a magnifying device like a telescope. If a telescope configuration has a
magnification of 30x, then an object viewed through the telescope will appear 30 times larger than
it would with the naked eye. To calculate the magnification of your telescope setup, divide the focal
length of the telescope tube by the focal length of the eyepiece. For example, a 20mm eyepiece in a
telescope with a 1000mm focal length will result in 50x power, which will make the object appear 50
times larger. If you change the eyepiece, the power goes up or down accordingly.
Focal ratio
The focal ratio of a telescope is determined by dividing the telescope’s focal length by its aperture
(usually expressed in millimeters). It plays a key role in determining a telescope’s field of view and
significantly impacts imaging time in astrophotography. For example, a telescope with a focal length of
1000mm and a 100mm clear aperture has a focal ratio of f/10.
Focal length (Telescope):
The focal length is the distance in millimeters between the objective lens or primary mirror and the
point at which entering light rays converge — otherwise known as the focal point. The focal lengths of
the telescope tube and the eyepiece are used to determine magnification.
Focal length (Eyepiece):
The focal length is the distance in millimeters between the center of the first lens element in an
eyepiece and the focal point. The focal lengths of the telescope tube and the eyepiece are used
to determine magnification. Short eyepiece focal lengths produce higher magnifications than long
eyepiece focal lengths.
Exit Pupil
The exit pupil is the diameter of the beam of light coming out of the eyepiece. To calculate exit pupil,
divide the focal length of your eyepiece by your telescope’s focal ratio. For example, if you use a 20mm
eyepiece with an f/5 telescope, the exit pupil would be 4mm.
Magnification = Telescope Focal Length
Eyepiece Focal Length
Focal Ratio = Telescope Focal Length
Telescope Aperture
Exit Pupil = Eyepiece Focal Length
Telescope Focal Ratio
Eyepiece Lens
Long Eye Relief Distance
Eyepiece Lens
Short Eye Relief Distance
Eyepiece Lens
Exit Pupil (mm)
Telescope Focal Length
1000mm
Eyepiece
Focal Length
20mm
Aperture
102mm

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Eyepiece Lens
Long Eye Relief Distance
Eyepiece Lens
Short Eye Relief Distance
Eyepiece Lens
Exit Pupil (mm)
Eyepiece Lens
Long Eye Relief Distance
Eyepiece Lens
Short Eye Relief Distance
Eyepiece Lens
Exit Pupil (mm)
Eye Relief
Eye relief is all about a comfortable viewing experience because it is the distance at which you
need to position your eye from the eyepiece’s outermost surface to enjoy the full field of view. This
characteristic is of special concern to observers who wear glasses to correct an astigmatism, because a
long enough eye relief is necessary to allow room
for glasses.
Huygenian Eyepieces:
A Huygenian eyepiece uses two plano-convex lenses separated by an air gap. They have a fairly narrow
apparent field of view.
Kellner Eyepieces:
A Kellner eyepiece uses three lens elements - two of which are paired together in an achromatic
doublet design to minimize chromatic aberrations. They typically produce an apparent field of view
around 45°.
Plössl Eyepieces:
A Plossl eyepiece uses two doublets (a pairing of lens) for a total of four lens elements. This eyepiece
design delivers sharp views and an apparent field of view of approximately 50°, which works well for
both planetary and deep sky viewing.
Barlow Lens:
A Barlow lens effectively increases the focal length of a telescope. It is inserted between the eyepiece
and the focuser/diagonal (depending on the optical setup) and multiplies the magnification power of
the eyepiece.
For example, a 2x Barlow will double the magnification of a particular eyepiece.
Barlow Lens
2 Lens Elements
Huygenian Eyepiece
2 Lens Elements
Light
Kellner Eyepiece
3 Lens Elements
Light
Plössl Eyepiece
4 Lens Elements
Light
Light
Eye Lens
Field Lens
Eye Lens
Field Lens
Field Lens

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Caution: The user is cautioned that changes or modifications not expressly approved by the party
responsible for compliance could void the user’s authority to operate the equipment.
Note: This equipment has been tested and found to comply with the limits for a Class B digital device,
pursuant to part 15 of the FCC Rules. These limits are designed to provide reasonable protection
against harmful interference in a residential installation. This equipment generates uses and can radiate
radio frequency energy and, if not installed and used in accordance with the instructions, may cause
harmful interference to radio communications. However, there is no guarantee that interference will not
occur in a particular installation. If this equipment does cause harmful interference to radio or television
reception, which can be determined by turning the equipment off and on, the user is encouraged to try
to correct the interference by one or more of the following measures:
—Reorient or relocate the receiving antenna.
—Increase the separation between the equipment and receiver.
—Connect the equipment into an outlet on a circuit different from that to which the receiver is
connected.
—Consult the dealer or an experienced radio/TV technician for help.
FCC RF Radiation Exposure Statement:
This equipment complies with FCC radiation exposure limits set forth for an uncontrolled environment.
This equipment should be installed and operated with a minimum distance of 20cm between the
radiator and any part of your body.
FCC Supplier’s Declaration of Conformity
Product name / model number: Smartphone Mount w/Bluetooth / AR5588
This device complies with part 15 of the FCC Rules. Operation is subject to the following two conditions:
(1) This device may not cause harmful interference, and (2) this device must accept any interference
received, including interference that may cause undesired operation.
Explore Scientific, LLC
1010 South 48th Street, Springdale, AR 72762
866.252.3811
www.explorescientific.com

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Notes:

161616
©2020 Explore Scientic, LLC.
1010 S 48th Street, Springdale, AR 72762
explorescienticusa.com | 866.252.3811
All rights reserved. Made in China.
CONTENTS AND COLORS MAY VARY
CONFORMS TO THE SAFETY REQUIREMENTS OF ASTM F963
V042020