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lunar

It's not the math, formulas or physics. Astronomy is the personal awareness, the insight, that aha, the satori, that you get when you see beautiful celestial objects or events.
Created 6/1/2002

Updated 7/28/2003

© 2002-3 Eric Flescher.

All Rights Reserved.

Lunar Eclipse Information

by Dr. Eric Flescher (KCStarguy@aol.com)  

created 6/3/2000 Updated 11/10/2003

http://members.aol.com/kcstarguy/blacksun/lunar.htm

Lunar eclipses

coming up

How can you rate the darkness of the eclipse? Use this scale
Participate in lunar eclipse observations/research to be listed here
Columbus was helped by an eclipse- did you know that?
photograph

the lunar eclipse

lunar links
interested in seeing the next solar eclipse in June 2001 Africa?
Additional information from the Astronomical Society of Kansas City
 

rate the lunar eclipses

danjon scale

eclipse ratings using danjon scale
Danjon table
danjon ratings by observers around the world
lunar eclipse view from space
lunar eclipse accounts
list of lunar eclipses coming up-

coming soon

 

Lunar Eclipse Resources

EJAWs mode
objective
websites examples Click on numbers to find out furthter information

EJAWs ACTION

Search

THINKING

research

ACTIVITIES FOCUS

exploration

general information about eclipses

Lunar Eclipses for Beginners

http://www.mreclipse.com/Special/LEprimer.html

EJAWs ACTION

Search

THINKING

research

ACTIVITIES FOCUS

exploration

learn what causes a lunar eclipse

 

what is a lunar eclipse?

more links listed

Q: What is the Lunar eclipse darkness measuring scale?

A: One of the simplest and most telling total lunar-eclipse observations is

estimating the Moon's luminosity value at various times during totality.

Early in the twentieth century, the French astronomer André-Louis Danjon

devised a clever five-point scale for rating the darkness of a total lunar

eclipse. The Danjon scale, reproduced in Table 4.1, has since gone on to

become the standard by which all total eclipses are judged.

 

Table 4.1

Danjon Lunar Eclipse Luminosity Scale

(More informtion below scale)

Danjon rating

Darkness

description simple

L = 0.0

Very dark eclipse.

Moon almost invisible, especially at mid-totality.

L = 1.0

Dark eclipse

gray or brownish coloration; lunar-surfacedetails distinguishable only with difficulty.

L = 2.0

Deep red or rust-colored eclipse

central part in the umbra

dark, but outer rim of the umbra relatively bright.

L = 3.0

Brick-red eclipse

usually with a brighter (frequently yellow) rim to the umbra.

L = 4.0

Very bright copper-red or orange eclipse

, with a bluish,

very bright umbral rim.

The Danjon scale should be used to estimate the appearance of a total

eclipse only with the naked eye. Surprisingly, the often-subtle colors of

a total eclipse tend to fade as magnification increases. The late Joseph

Ashbrook suggested that this might be due to a reduction in surface

brightness to near or below the threshold for color perception.

 

Although Danjon devised the scale to fit every lunar eclipse, it is rare

for an eclipse to match one of his descriptions exactly. Instead, most

seem to fall somewhere between two values - therefore, so should your

estimate. For example, at mid-eclipse, if the Moon appears a muddy-clay

color highlighted with a bright, almost yellow rim, then the Danjon

luminosity value would fall somewhere between 2.0 and 3.0. After carefully

examining the Moon's appearance, judge which description it most resembles,

then prorate the value accordingly. In this case, a luminosity value of

2.4 or 2.5 would seem most appropriate. Astronomical magazines always

encourage readers to send in their observations and reports, but to be of

real value, always include your time, location, instrument used, if any,

and a description of the sky conditions.

 

A less-often quoted rating system was introduced in 1924 by Willard J.

Fischer. The Fischer scale uses a three-point strategy based not on color,

but instead, on the amount of surface detail visible through various

instruments. Table 4.2 offers a summary.

 

Table 4.2

Fischer Lunar Eclipse Scale

 

Grade Description

2 The naked eye sees "spots" on the eclipsed Moon, and the seas and

other detail can be seen with hand instruments (small binoculars and field

glasses)

 

1 Instruments of 5 cm (2 inches) up to 15 cm (6 inches) are necessary

to show detail on the eclipsed surface.

 

0 Apertures greater than 15 cm (6 inches) are needed to see surface detail.

 

Phil Harrington

Author: Eclipse!

http://www.philharrington.homepage.com

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Send in your lunar eclipse darkness rating (according to the scale above and we will list them here.

Send to Dr. Eric Flescher (KCStarguy@aol.com)

Your name: ______________________________

Screen name:___________________

Place observing from: City :_____________________ State:_____________________

Your rating number for the eclipse at mid totality

Danjon) 0 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0

the reason for your rating-explain (colors, brightness etc) : ________________________________________

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Lunar Eclipse photography exposures with 35 mm

Choose what you want to shoot and set you aperature and speed to these settings

no filter required. Tripod recommended

These recommendations modified from Astrophotgraphy Basics by Kodak (P-150)

 

If you wold like to try to photograph the eclipse

try

http://www.mreclipse.com/LEgallery/LEphoto.html

stage of eclipse

asa fim speeds

higher ASA faster it is but more grain

faster film

25-32

64-80

100-125

200

400

full moon

1/250

at f/5.6

1/250

at f/8

1/250

at f/11

1/250

at f/22

1/250

at f/22

up to first contact

1/60

at f/5.6

1/60

at f/8

1/60

at f/11

1/60

at f/16

1/125

at f/16

2nd 3rd contact

2

at f/2

1

at f/2

2

at f/2.8

2

at f/4

1/4

at f/2.8

mid totality

8

at f/2

4

at f/2

2

at f/2.8

1

at f/2.8

1

at f/2.8

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