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 19-4 (1992 Oct-Dec)
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The 1992 Close Approach by 4179 Toutatis: A Call for Observations
Pages 27
Binzel, R. P.; Harris, A. W.
1992MPBu...19...27B    Download PDF

On 1992 December 8, the near-Earth asteroid 4179 Toutatis will pass within 0.024 AU of the Earth, a distance of less than 10 times that of the Moon. As reported by Sicoli and Cavagna (MPB _li!, No. 2, page 17), Toutatis will not make an encounter closer than this one until 2004. Thus this apparition marks a good chance for observers to see this small minor planet, estimated to be only about 3 km in diameter. During its close approach, observers who locate Toutatis or capture it on film should be able to detect its motion or record a trail within a few minutes.

CCD Photometry of Asteroid 16 Psyche
Pages 28-29
Neely, A. W.
1992MPBu...19...28N    Download PDF

Photometric obsetvations of the asteroid 16 Psyche were made during its 1992 apparition using a CCD detector at the NFI Obsetvatory. The synodic rotational period was 4.196 ± 0.005 hrs. The lightcutve amplitude was 0.19 ± 0.02 magnitudes. These results agree well with previous studies.

Photoelectric Photometry of 10 Hygiea
Pages 29-30
Lagerkvist, C.-I.; Oja, T.; Pohjolainen, S.; Erikson, A.
1992MPBu...19...29L    Download PDF

UBV photometry was performed of 10 Hygiea during nine nights in October, November and December 1992. A composite lightcurve is presented favouring a rotation period of 27.62 hours.

Observing Programs of the Minor Planets Section Circolo Astrofili Di Milano
Pages 31
Foglia, S.
1992MPBu...19...31F    Download PDF

The Minor Planets Section of Circolo Astrofili di Milano was established In November 1991. It promotes observing programs and research activities for amateur astronomers. It also collaborates with the Minor Planets Sections of the Unione Astrofill Italiani (where I coordinate the visual programs) and the Association of Lunar and Planetary Observers. At the moment, our programs include visual astrometry, visual photometry. and photographic astrometry.

CCD Photometry of Asteroid 487 Venetia
Pages 31-32
Neely, A. W.
1992MPBu...19...31N    Download PDF

Photometric observations of the asteroid 487 Venetia were made during its 1992 apparition using a CCD detector at the NFI Observatory. The synodic rotational period, which was previously unknown, was determined to be 12.73 ± 0.12 hrs. The lightcurve amplitude was 0.30 ± 0.02 magnitudes.

CCD Photometry of 141 Lumen
Pages 33
Wetterer, C. J.; Flower, T. F.
1992MPBu...19...32W    Download PDF

CCD photometry of the asteroid 141 Lumen is reported. The observations indicate a rotation period greater than 18 hours with an amplitude of at least 0.2 magnitudes.

Asteroid News Notes
Pages 33-36
Tholen, D. J.
1992MPBu...19...33T    Download PDF

Through the August 13 batch of Minor Planet Circulars, 226 asteroids were newly numbered since the last installment of News Notes, bringing the numbered total to 5297.

Astrometric Positions of Minor Planets
Pages 36
Pryal, J.
1992MPBu...19...36P    Download PDF

The following precise astrometric positions have been measured from photographs obtained by the author. The location of each observing site follows each set. The photographs were measured using the Digitized Stage Microscope, at the University of Washington.

Photoelectric Photometry Opportunities: November-January
Pages 37
Harris, A. W.; Zappalá, V.
1992MPBu...19...37H    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. ObseiVations are needed because the asteroid has either an unknown or ambiguous rotational period or because the asteroid will be obseiVable at a vety low phase angle.


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