The Minor Planet Bulletin
BULLETIN OF THE MINOR PLANETS SECTION OF THE ASSOCIATION OF LUNAR AND PLANETARY OBSERVERS


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The Minor Planet Bulletin is the journal for almost all amateurs and even some professionals for publishing asteroid photometry results, including lightcurves, H-G parameters, color indexes, and shape/spin axis models. It is considered to be a refereed journal by the SAO/NASA ADS. All MPB papers are indexed in the ADS.

Print subscriptions are no longer available to individuals. Institutions (e.g., college libraries) can still obtain print copies via a special subscription. See details in MPB 37-4 or contact the editor, Richard Binzel.

Annual voluntary contributions of $5.00 or more in support of the publication are welcome.
Please send a check, drawn on a U.S. bank and payable in U.S. funds, to "Minor Planet Bulletin" and send it to:

Derald D. Nye
Minor Planet Bulletin
10385 E. Observatory Drive
Corona de Tucson, AZ 85641-2309


Authors Guide and Word Templates   (v.2.7: updated 2019 March 4)
Please read this updated guide since there are a number of changes from previous guides.
The ZIP file contains the Authors Guide PDF as well as a "starter" paper in Word 97 (DOT) and Word 2007+ (DOTX).

Cumulative Index to Volumes 1-45
Cumulative Asteroid Lightcurve Index (Volumes 1 through 46-2)

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Issues for the upcoming quarter-year are released on about the 21st of March, June, September, and December. Full issues and individual papers from vol 1 (1973) to present are available via links on this page.

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Vol 1-7 run Jul-Jun. Vol 8-present run Jan-Dec. Only papers indexed in the ADS are included. Earlier volumes often contain more papers than listed here. It's recommended to download the full issue in vol 1-9.

Volume 46 (2019)

Volume 45 (2018)

Volume 44 (2017)

Volume 43 (2016)

Volume 42 (2015)

Volume 41 (2014)

Volume 40 (2013)

Volume 39 (2012)

Volume 38 (2011)

Volume 37 (2010)

Volume 36 (2009)

Volume 35 (2008)

Volume 34 (2007)

Volume 33 (2006)

Volume 32 (2005)

Volume 31 (2004)

Volume 30 (2003)

Volume 29 (2002)

Volume 28 (2001)

Volume 27 (2000)

Volume 26 (1999)

Volume 25 (1998)

Volume 24 (1997)

Volume 23 (1996)

Volume 22 (1995)

Volume 21 (1994)

Volume 20 (1993)

Volume 19 (1992)

Volume 18 (1991)
    
    
    
    

Volume 17 (1990)

Volume 16 (1989)

Volume 15 (1988)

Volume 14 (1987)

Volume 13 (1986)

Volume 12 (1985)

Volume 11 (1984)

Volume 10 (1983)

Volume 9 (1982)

Volume 8 (1981)

Volume 7 (1980)

Volumes 6-7 (1979)

Volumes 5-6 (1978)

Volumes 4-5 (1977)

Volumes 3-4 (1976)

Volumes 2-3 (1975)

Volumes 1-2 (1974)

Volume 1 (1973)

  
Issue 18-4 (1991 Oct-Dec)
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Show abstracts

Rotation Period and Lightcurve of Asteroid 338 Budrosa
Pages 37-38
Hutton, R. Gil; Licandro, J.
1991MPBu...18...37H    Download PDF

Photoelectric observations in V and B filters of the asteroid 338 Budrosa were made from Estaci6n de Altura "Dr. Carlos U. Cesco" of Felix Aguilar Observatory during the 1990 apparition. The synodic rotational period, lightcurve amplitude and average B-V color found for 338 Budrosa are: P = 4.6 ± 0.1 hr. Δm = 0.47±0.0l, B-V = 0.680 ± 0.014. This is the first secure period reported.

Photoelectric Photometry of Asteroid 125 Liberatrix
Pages 39-40
Hutton, R. Gil
1991MPBu...18...39H    Download PDF

Photoelectric observations in V and B filters of the asteroid 125 Liberatrix were made from Estaci6n de Altura "Dr. Carlos U. Cesco" of Felix Aguilar Observatory during the 1990 apparition. The 3.97±0.1 hour synodic rotational period, and 0.695±0.014 average B-V color agree with previous determinations. The lightcurve amplitude found is t.m=0.30 ±0.01.

Asteroid News Notes
Pages 41-42
Tholen, D. J.
1991MPBu...18...41T    Download PDF

Through the September 23 batch of Minor Planet Circulars, 238 asteroids were newly numbered since the last installment of News Notes, bringing the numbered total to 4960.

Photoelectric Photometry Opportunities: November-January
Pages 43
Harris, A. W.; Zappalá, V.
1991MPBu...18...43H    Download PDF

The table below lists asteroids which come to opposition during the months of November through January that represent useful targets for photoelectric photometry observations. Observations are needed because the asteroid has either an unknown or ambiguous rotational period or because the asteroid will be observable at a very low phase angle.


copyright©2017 Brian D. Warner. Funding to support this web site is provided by NASA grant NSSC 80NSSC18K0851