The Webb Deep-Sky Society

An international society of amateur and professional astronomers specialising in the observation of double stars and 'deep sky' objects founded in 1967. Membership is open to anyone who shares the interests of the Society.

  • About Us
  • Membership
  • Deep-Sky News
  • Galaxies
  • Nebulae and Clusters
  • Double Stars
  • Publications
  • The DSO
  • August 2015 - Double Star of the Month

    Lambda Cygni (20 47 24.563 +36 29 26.7) is easily found. Just move 3 degrees due north from epsilon Cygni, the left-hand star in the cross. One of Otto Struve's discoveries from Pulkova the seeing needs to be good to get a measure of the companion. The stars are magnitudes 4.7 and 6.3 but have always been separated by less than 1" although the angular distance between the stars is now roughly double that at discovery. Since 1990 the writer has observed the pair in 12 seasons and in that time the position angle has decreased by about 10 degrees. The current orbit has a period of 391 years but this is complicated by the fact that Hal McAlister and colleagues found the primary to be an interferometric binary with a period of 11 years and maximum separation of 0".05. There is some evidence that one of the three stars is also a single-lined spectroscopic binary. Lambda Cyg has a spectral type of B5Ve and is a rapid rotator surrounded by a circumstellar disk. Sir James South adds a faint companion, mag 9.7, at 106° and 83".

    The sprawling constellation of Capricornus sits near the meridian on a northern summer night but locating stars in it apart from the third magnitude alpha and beta needs the help of a star atlas. However, starting with the brightest star of all, beta, by moving 3 degrees south and slightly east a trio of stars is encountered, all enclosed by a 1 degree field. Each of these is a visual double star and the subject of this column is omicron Cap = SHJ 324 (20 29 53.91 -18 34 59.4) the most southerly of the three. Smyth calls it omicron2 and notes that both components are to be found in Piazzi's catalogue. The WDS gives magnitudes of 5.9 and 6.7 and the separation is currently 21".9, down from 25" when found by William Herschel with a small decrease in the position angle, currently 238°. The Hipparcos catalogue gives the distance as 216 light years but with a formal error of 27% this is an indicator that there could possibly be another star nestling in the system.

    Smyth calls both stars bluish, and whilst Sissy Haas regards them as almost equal, the report by Hartung notes that they are an 'unequal white pair'.

    Bob Argyle - Double Star Section Director

  • About the Webb Society

    • Back top of this page
    • Go to our home page
    • About us
    • News
    • Our Annual Meeting
    • Galaxy Section
    • Nebulae and Clusters Section
    • Double Star Section
    • Join the Webb Deep-Sky Society
    • Links to members' websites
    • Useful astronomy links
    • Contact Us
  • Deep-Sky Objects and Observations

    • Observations home page
    • Object of the Season
    • Double Star Circulars
    • Double Star of the Month archive
    • Double Star of the Month RSSRSS feed icon
    • Galaxy of the Month archive
    • Galaxy of the Month RSSRSS feed icon
    • Picture of the Month archive
    • Picture of the Month RSSRSS feed icon
    • Nebula and Cluster of the Month archive
  • The Deep-Sky Observer

    • DSO digital subscriber login
    • Webb Society Journal archive
  • Publications

    • Handbooks, Guides and Atlases
    • Alvin Huey's Observer's Guides
    • Willman-Bell Publications
    • Free Observing Guide Downloads
  • Featured Articles

    • Where to get reliable NGC/IC data
    • Rediscovering the Bedford Catalogue
    • An Averted Vision Scale

If you have any comments or problems with this page or any other Webb Deep-Sky webpage then please contact the Website Administrator

The Webb Society is registered under The Charities Act 1960 - Registered Charity No. 288384 © 2025 Webb Society except where stated.

The information contained in this website is for general information purposes only. The information is provided by The Webb Deep-Sky Society and while we endeavour to keep the information up to date and correct, we make no representations or warranties of any kind, express or implied, about the completeness, accuracy, reliability, suitability or availability with respect to the website or the information, products, services, or related graphics contained on the website for any purpose. Any reliance you place on such information is therefore strictly at your own risk. In no event will we be liable for any loss or damage including without limitation, indirect or consequential loss or damage, or any loss or damage whatsoever arising from loss of data or profits arising out of, or in connection with, the use of this website. Through this website you are able to link to other websites which are not under the control of The Webb Deep-Sky Society. We have no control over the nature, content and availability of those sites. The inclusion of any links does not necessarily imply a recommendation or endorse the views expressed within them. Every effort is made to keep the website up and running smoothly. However, The Webb Deep-Sky Society takes no responsibility for, and will not be liable for, the website being temporarily unavailable due to technical issues beyond our control.