Dark Nebulae Observing Program Coordinator:
4845 N Smalley Ave.
Kansas City, MO 64119
Dark nebulae were once thought to be holes in the Milky Way. This viewpoint changed as astronomers such as E.E. Barnard started serious study of the dark areas and photography was developed as a useful tool to study the heavens. These pioneers discovered that dark nebulae were not holes in the Milky Way but obscuring interstellar dust clouds blocking our view. These dust clouds may be small, dusty star forming regions, or may be portions of larger dark lanes of galactic dust. Other dusty spiral galaxies clearly show similar dark lanes and patches.
Observing the Objects
Dark nebulae are among the most difficult objects for an observer to search out. Although many are large enough to be naked eye or binocular objects, they may be difficult because transparent skies away from city lights are needed. The dark nebulae “holes” are not visible unless the Milky Way itself is clearly present. Identification is sometimes challenging. Some large dark nebulae include smaller, darker patches with separate ID’s which may cause confusion. Log only the objects that you can distinguish as separate areas. For example, the Stem of the Pipe Nebula has four Barnard dark nebulae within its area. Only log the darker concentrations of the individual Barnard objects if you can distinguish them as separate darker patches. It is very possible that on some nights you will see the whole, but not the parts or vice versa.
The objects on this list will require equipment ranging from naked eye to a telescope. Tripod-mounted binoculars or a small (4-6”) rich field telescope will be ideal for finding many dark nebulae. Some of the smaller dark nebulae may require the smaller field and light gathering of an 8” or larger telescope. Larger telescopes may be needed to see some of the more difficult optional dark nebulae. You do not need a telescope larger than 8” to complete this observing project if your skies are dark and transparent and you choose your targets carefully. You may need to use more than one source to locate and identify the nebulae.
The list includes objects from Barnard (B), Lynds Dark Nebula (LDN), and other catalogs. The definitive identification of the Barnard objects is E.E. Barnard’s Photographic Atlas of the Milky Way. The Georgia Institute of Technology has made this valuable resource available on-line. This web site is at: http://www.library.gatech.edu/search/digital_collections/barnard/intro.html .
Not all the Barnard objects are in the Barnard Photographic Atlas; a few, such as B33 (the Horsehead), are not.
Dark nebulae vary in how much they obscure the background stars. Many dark nebulae have a Lynds opacity number associated with them. The Lynds opacity scale is based on Palomar blue and red photographic plates rather than visible light, but does provide a method of describing the apparent density of dark nebulae. In this 1-6 scale, the most opaque dark nebulae are classed as opacity 6, and the least opaque as opacity 1. For example, on the Lynds opacity scale: B92 is classed as an opacity 6, B86 is a 5, B361 is a 4, B111 is a 3, B138 is a 2, and B144 is a 1. In this project, you are to estimate the opacity of the dark nebulae you observe. Use an opacity scale of 1-6, with 6 being the darkest. Estimating the opacity of various dark nebulae will give you an additional way to describe and compare them.
- You must be a member of the Astronomical League either as a member of an affiliated club or as a Member-at-Large.
- You must image 70 dark nebulae. There are 35 required objects on this list that you must image. Choose 35 others from the list for a total of 70 to receive your pin/certificate. Please see the link to the lists below.
- Use of publicly available “remote” telescopes controlled via an internet connection is not allowed. Delegation of image acquisition is not acceptable.
- "Go-to" telescopes are allowed.
- Imaged dark nebulae must be identified by means of an overlay, companion sketch or other method to clearly identify the dark nebulae on the image(s). This is particularly important in cases where the dark nebula may be difficult to clearly identify on the image or more than one dark nebula is present.
- Keep a log recording your imaging including:
- Object name and number
- Date and time of the imaging (local or UT)
- Latitude and longitude of your imaging location
- Seeing and transparency
- Filters used (if any)
- Telescope/optics used including aperture and focal ratio
- The camera/CCD used, exposure times, film types, image software, number of stacked images, and other information relevant to the image production must also be provided
Combined Visual and Imaging:
Observers may combine imaging and visual observations provided that the logging requirements for each type of activity meet the individual requirements above.
Please check with the Dark Nebulae Observing Program Coordinator if you have any questions about the requirements.
Submitting for Certification
To receive your Dark Nebulae Program certificate and pin, send copies of your observations/images along with the completed Submission Form (or equivalent) to the Dark Nebulae Observing Program Coordinator.
Be sure to include: your name, mailing address, email, phone number, society affiliation, and to whom the certification should be sent.
Send only COPIES of your observations or images in case they get lost in the mail. Please avoid sending prints or slides unless you do not require them back. Images or observations in electronic format may be forwarded by any convenient means. This may include mailing of a storage device such as a CD or 'posting' on the web. Please check with the Program Coordinator if you have any questions on how to transfer your images or observations for review. Material sent for review will not be returned unless return postage is included.
Upon verification, your certificate and pin will be sent directly to you or to your Club’s award coordinator for presentation.
Dark Nebulae Program Chair:
4845 N Smalley Ave.
Kansas City, MO 64119