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.

Important: If the ADS bibcode and "Download PDF" links are missing for the latest issue, it is because the ADS has not processed the files. The links will be made available after the ADS processes the files.
If the "Download PDF" link is visible and there is no PDF available, clicking the link will download an arbitrary page. We are working with ADS to make sure all papers are available and, if not, being able to diasable the link. The "Download Full Issue" link does retrieve the correct file.

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 23-4 (1996 Oct-Dec)
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Show abstracts

CCD Photometry of 523 Ada
Pages 41-42
Georgilas, S. A.; Wetterer, C. J.
1996MPBu...23...41G    Download PDF

The asteroid 523 Ada was observed on 4 different nights in 1996 February and March. The best synodic period derived from all these observations is 9.800 ± 0.002 hours with an instrumental V magnitude amplitude of 0.65 -0.70.

The Lightcurve and Period of the Minor Planet 193 Ambrosia
Pages 42
De Young, J. A.; Schmidt, R. E.
1996MPBu...23...42D    Download PDF

The minor planet 193 Ambrosia is found to have a photometric rotation period of 0.27420 ±0.00025 days (6.5807 ± 0.006 hours) and an amplitude in the Kron-Cousins I­ band of 0.532 ± 0.013 mag.

Photometric Observations of Minor Planet 212 Medea
Pages 43
Holliday, B.
1996MPBu...23...43H    Download PDF

CCD photometry of asteroid 212 Medea was performed in April 1996 to determine its rotational period and lightcurve amplitude. The period was found to be 10.25 ± 0.07 hours and the amplitude was 0.11 magnitudes.

The Lightcurve and Period of the C-type Minor Planet 38 Leda
Pages 44
De Young, J. A.; Schmidt, R. E.
1996MPBu...23...44D    Download PDF

The minor planet 38 Leda is found to have a photometric (rotation) period of 0.5349 ± 0.0018 days (12.84 ± 0.04 hours) and an amplitude in the Kron-Cousins I-band of 0.155 ± 0.024 magn.

Asteroid News Notes
Pages 45-46
Tholen, D. J.
1996MPBu...23...45T    Download PDF

Through the July 30 batch of Minor Planet Circulars, 258 asteroids were newly numbered, breaking the 7000 level, and bringing the numbered total to 7100.

Asteroid Photometry Opportunities: November-January
Pages 47
Harris, A. W.; Zappalá, V.
1996MPBu...23...47H    Download PDF

The table below lists asteroids that come to opposition during the months of November through January that represent useful targets for photoelectric or CCD photometry observations. Observations are typically needed because the asteroid has either an unknown or ambiguous rotational period. The table gives (in order of opposition dates) the asteroid number and name, opposition date, opposition V magnitude, the rotational period (in hours), the estimated lightcurve amplitude (in magnitudes), and the designation PER if observations are needed to determine the rotational period. AMB implies that previous period determinations have given ambiguous results and these alternate periods are listed in the table. RAD indicates the asteroid is a planned radar target, and MOD denotes an asteroid at a critical longitude for shape and pole modeling. Question marks are used to denote uncertain or unknown values.


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