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1 GLOBE at Night: GLOBE at Night: A Citizen-Scientist A Citizen-Scientist Night Sky Brightness Night Sky Brightness Program to Measure Some slides adapted from the International Dark-Sky Association Some images courtesy of NOAA Connie Walker National Optical Astronomy Observatory 2 Light pollution is a global issue with local solutions…

GLOBE at Night: A Citizen-Scientist Program to Measure ... · The “classic” GLOBE at Night observations that anyone can have fun doing with their unaided eyes! An effort to obtain

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Page 1: GLOBE at Night: A Citizen-Scientist Program to Measure ... · The “classic” GLOBE at Night observations that anyone can have fun doing with their unaided eyes! An effort to obtain

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GLOBE at Night:GLOBE at Night: A Citizen-Scientist A Citizen-Scientist

Night Sky BrightnessNight Sky Brightness

Program to Measure

Some slides adapted from the International Dark-Sky Association

Some images courtesy of NOAA

Connie Walker

National Optical Astronomy Observatory

2

Light pollution is a globalissue with local solutions…

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…Increasing Over Time(Cinzano, Falchi, and Elvidge 2001)

4

Los Angeles in 1908

& 1988, as seen

from Mt. Wilson

Observatory

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A Little Sky Glow CanMake All the Difference

Before Curfew After Curfew

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Shielding the Streetlight- a Demonstration

• Make sure you are in a very dark roomwith a low ceiling and a white surface.

• Unscrew the reflectors from both “mini-lights” and turn 1 on (“candle mode”).

• Place the bulb top of the “mini-light”barely into the big hole at the bottom ofthe white paper cube.

• With the room lights off, project the“stars” from the white paper cube ontothe ceiling.

“candle mode”

Planetarium withlight inside

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Shielding the Streetlight- a Demonstration

continued…

• Using a 2nd “mini-light” as a “streetlight”, place it on a table and turn iton.

• What do you notice about thenumber of stars?

• Now place the PVC cap (or anothershield) above the 2nd “mini-light” torepresent a shielded streetlight.

• What difference do you notice withand without the shield?

“streetlight”

shielded light

8

Now you see the person…

Now you don’t…

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Unshielded vsShielded Fixtures

Unshielded

• Minimizes glare.

• Minimizes lightdirected upwardand skyglow.

• Minimizes lighttrespass.

• Minimizes energyuse & cost

Shielded

10

Light Trespass

Sky Glow

3 Main Types of

Light Pollution

Glare

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Issues of Safety, Security

and Energy

12The lights of the city of Tucson, Arizona, USA, as seen from the observatory on nearby Kitt Peak

The Effects on Astronomical Research

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The Effects on Wildlife

One main problem light pollution causes for wildlife:

disorientation (sea turtles, birds, moths etc)13

The Effects on

Human Health

One main problem light pollution causes for humans:

disruption of people’s 24 hour internal clock (circadian rhythm)14

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What can you do?

Light pollution may be a global problem,

but you can be part of a local solution…

Feb. 5, 2008 NSN Telecon on GLOBE at Night 16

Use Quality Lighting

• See the effect, not the source.

• Shine the light down.

• No glare.

• Light only where and when needed.

• Don’t over light.

• Use energy efficient sources.

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The GLOBE at Night Program:

2 Ways to Participate

! The “classic” GLOBE at Night

observations that anyone can

have fun doing with their

unaided eyes

! An effort to obtain more precise

measurements of the night sky

using digital sky-brightness

meters

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The GLOBE atNight Program

• To learn about the impact of artificial lighting on towns and

cities, and the ongoing loss of a dark night sky as a natural

resource for much of the world.

• Citizen-scientists (YOU!) record the brightness of the night

sky by matching its appearance toward the constellation

Orion with charts of different limiting magnitudes.

• You can also measure sky brightness with Sky Quality

Meters.

• Measurements are submitted on-line and resulting maps

of all worldwide observations are created.

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Almost 7000 measurements,over 60 countries

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The Globe at Night Websitehttp://www.globe.gov/GaN/

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Steps to Observe

(unaided eye observations)

• Step #1. Find the constellation

Orion; note sky conditions

• Step #2. Match night sky to a

magnitude chart

• Step #3. Report your obser-

vations on-line

• Step #4. Input your latitude

and longitude

• Step #5. Compare your observation(s) to thousands

around the world

http://www.globe.gov/GaN/observe.html

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Step #1: Find YourLatitude & Longitude

• Use a GPS unit where you take ameasurement.

• Visit http://eo.ucar.edu/geocode/,http://www.earth.google.com, orhttp://www.itouchmap.com/latlong.htmlon-line. Input your location. Or inputyour city; zoom in/out and pan arounduntil you find your location.

• Use topographic map of your area.

• Determine your latitude and longitudewith the interactive tool when reporting

http://www.globe.gov/globeatnight/observe_latlong.html

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Find Your Latitude & Longitude

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•Determine the darkest area where themost stars are visible.

•Wait 10 minutes for your eyes to darkadapt.

•Comment on the sky conditions & yourobserving location, such as street lights.

http://www.globe.gov/globeatnight/observe_finder.html

• Locate Orion with Finder Charts at www.globe.gov/globeatnight/observe_finder.html.

• Between March 16-28, 2009, Orion will be midway between South& West. Orion will be 2 to 3 clenched fists (held at arm’s length)above the horizon between 7-10 pm. Orion looks like an “hourglass”.

Step #2: Finding Orion©

T.

Cre

dn

er

& S

. K

oh

le, A

llth

eS

ky.c

om

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Step #3: Match Night SkyStep #3: Match Night Sky

to a Magnitude Chart.to a Magnitude Chart.

Estimate cloud coverageEstimate cloud coverage..

Fill out the observationFill out the observation

sheet.sheet.

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Step #4. Report

Step #4. Report

observations on-

observations on-

line.line.

Observe anytime

Observe anytime

between March

between March

16-28, 2009.

16-28, 2009.

Do it again fro

m a

Do it again fro

m a

different lo

cation!

different lo

cation!

/report.cfmhttp://www.globe.gov/globeatnight/report.html

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85 miles 5 miles

Zoom in with “Map Viewer”

It is important to have many observations at about 1 km to 1mile apart. Then we can map out light pollution within cities…and show how safe, quality lighting can make a difference inprotecting night skies!

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Zoom in with “Map Viewer”

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Helpful Information

• Brightness or magnitude of

stars

• Finding Orion (interactive tool)

• Orion mythology

• Light pollution

• How number of stars changes

with light pollution and

how latitude affects the

orientation of Orion

(interactive tool)

http://www.globe.gov/GaN/learn.html

30July 19th, 2008 ALCON 2008

LP

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Data Input for GLOBE at Night

• REQUIRED INPUT:

– Date and Local Time !!!

– Latitude and Longitude

– Unaided eye observation

– Meter Reading!(from Sky Quality Meter)

• OPTIONAL INPUT

– Various additional comments

http://www.globe.gov/GaN/report.html

Report Form

DateTime

Orion data

SQM entry

SQM serial

number

Lat/Long

http://www.globe.gov/GaN/report.html

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The Sky Quality Meter

! Press start button

here:

! Light enters

here:

! Read-out numbers

here:

http://www.globe.gov/GaN/learn_SQM.html

The SQM is Easy to Use!

• Point the SQM’s sensor straight up

(toward zenith).

• The SQM should be held at or above

head level so that shadows or

reflections from your body do not

interfere with the reading.

• Avoid using in areas that are shaded

by trees or buildings or lit by lights.

Be at least as far away from those

objects as they are high.

• After you press the button to take a reading, the SQM will beep

while it is accumulating photons. The beeping will stop once the

reading is ready to be viewed.

http://www.globe.gov/GaN/learn_SQM.html

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What do the Sky QualityMeter Readings Mean?

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What to Watch Out ForWhen Using the SQM

• 4 other numbers are displayed when youpress and hold the button a second time:

The temperature in °C and °F andthen the model and serial numbers

• The meter readings are somewhattemperature dependent.

_ Leave the meter outside for a coupleof minutes before taking measure-ments depending on the temperaturedifferential.

_ the SQM company advises to toss outthe very first measurement.

• You should have an Orion measurementfor every SQM measurement.

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Unaided Eye Observationswith Population Density (Tucson)

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Take Back the Night!Participate in the

GLOBE at Night Campaign

• At least 2 out of 5 Americans have neverseen 90% of the stars in our night sky.

• With half the world's population now living incities, this problem is only getting worse.

• Yet you can easily be part of a local solutionto a global problem.

• Become a local coordinator.

• Take a few minutes to monitor your localnight sky brightness.

• Help preserve our natural heritage forgenerations to come.

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GLOBE at NightHow Many Stars?

Great World Wide Star Count• GLOBE at Night

Next GLOBE at Night campaign is March 16 - 28, 2009

Orion and Sky Quality Meters

www.globe.gov/globeatnight/

! How Many Stars?

Jan, Feb, April-Sept, Nov, Dec 2009

Little Dipper and 3 belt stars in Orion

www.sternhell.at/

! Great World Wide Star Count

Oct. 9 - 23, 2009

Cygnus and Sagittarius

www.starcount.org 39

Dark Skies Awareness

Global IYA Cornerstone

PROGRAMS

Citizen Science, Star-HuntingCitizen Science, Star-Hunting

Programs (e.g. GLOBE at Night)Programs (e.g. GLOBE at Night)Education ToolkitEducation Toolkit

Earth Hour Planetarium Show

Quiet Skies Traveling Exhibit, Posters, Brochures

Earth & Sky Photo Contest Great Switch Out

Dark Skies Discovery Sites Second-Life, Facebook, MySpace

Nights in the (National) Parks Podcasts

International Dark Sky Week &

World Night in Defense of Starlight

International Dark-Sky Communities,

Parks, & Reserves

www.darkskiesawareness.org 40

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Thank-you foryour kind attention!

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For more information

! Websites of interest:www.darkskiesawareness.org

www.globe.gov/GaN/

! Contact: Connie Walker1-520-318-8535 or

[email protected]

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QUESTIONS?

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