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:

Minor Planet Bulletin
c/o Melissa Hayes-Gehrke
UMD Astronomy Department
1113 PSC Bldg 415
College Park, MD 20742


Authors Guide and Word Templates   (v.2.9: updated 2019 November 14)
The ZIP file contains the Authors Guide PDF as well as a "starter" paper in Word 97 (DOT) and Word 2007+ (DOTX).
Please read this updated guide since there are a number of changes from previous guides.
  • The Pts column is no longer required and has been removed from the template for the standard table
    to allow more room for the other columns.
  • The phase column should have only two values: for the first and last date in the range.
    If the phase reaches an extrema between those dates, put an asterisk before the first value. For example,
       *7.2,13.7.
  • Use semicolons to separate names in the references section. For example:
       Smith, J.J.; Jones, A.A. (2019).
    This also applies if using several references to the same author in the text. For example:
    "This asteroid was observed at three previous apparitions (Jones, 2015; 2017; 2018)..."

Cumulative Index to Volumes 1-45
Cumulative Asteroid Lightcurve Index (Volumes 1 through 50-1)

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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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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 51 (2024)
    

Volume 50 (2023)

Volume 49 (2022)

Volume 48 (2021)

Volume 47 (2020)

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 51-1 (2024 Jan-Mar)
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Show abstracts

Space-Rocky Road to Observatory Automation and Lightcurves
Pages 1-3
Fekete, Paula; Porter, Jaxon J.; Willis, Jacob P.

We report six lightcurve analyses based on observations obtained at the West Point Observatory over the interval 2021 September through 2023 February. One notable result is finding a previously unreported rotation period for 4482 Frèrebasile; P = 3.043 ± 0.001 hours with an amplitude of 0.12 magnitudes. Since these are the first asteroid photometry results reported from our Observatory, we also detail some aspects in developing our program and some unique challenges for meshing astronomical projects with the cadet lifestyle.

Lightcurves and Rotation Periods of 1292 Luce, 1340 Yvette, 2738 Viracocha, 2841 Puijo, 4362 Carlisle, and 9911 Quantz
Pages 3-5
Stone, Geoffrey

Lightcurves and rotation periods were found for six asteroids observed from 2021 April to May.

Lightcurves and Derived Results for Koronis Family Member (5139) Rumoi, Including a Discussion of Measurements for Epochs Analysis
Pages 6-10
Slivan, Stephen M.; Barrera, Kaylee; Colclasure, Abigail M.; Cusson, Erin M.; Larsen, Skylar S.; McLellan-Cassivi, Claire J.; Moulder, Summer A.; Nair, Prajna R.; Namphy, Paola D.; Neto, Orisvaldo S.; Noto, Maurielle I.; Redden, Maya S.; Rhodes, Spencer J.; Youssef, Sandra A.

Lightcurves of (5139) Rumoi recorded during three apparitions are presented, with derived results for synodic rotation period, solar phase coefficients, color index, and absolute magnitude, along with an analysis for spin direction and sidereal rotation period in combination with previously published data. An approach for measuring lightcurves for epochs analyses also is described.

Lightcurve Analysis of 5780 Lafontaine
Pages 10-11
Farfán, Rafael González; de la Cuesta, Faustino García; Carballo, Juan-Luis González; Fernández, José María; Fernández, Javier Ruiz; Reina, Esteban; Podlewska-Gaca, Edyta; de Elias, Javier Cantalapiedra

CCD photometric observations of minor planet 5780 Lafontaine were made in 2023 July and August by a group of observers from Spain and Poland. Analysis of the data could not find a definitive solution for a synodic rotation period.

Lightcurves and Rotation Period Determination of Seven Main-Belt Asteroids Observed from Malta and Slovakia
Pages 12-15
Brincat, Stephen M.; Bucek, Marek; Galdies, Charles; Mifsud, Martin; Grech, Winston

We present the results of our photometric observations of seven main-belt asteroids from five observatories in Malta and Slovakia. We have managed to derive the lightcurves for the following asteroids that can assist future analysis of these objects at different oppositions: (1400) Tirela; (1850) Kohoutek; (2591) Dworetsky; (5163) Vollmayr-Lee; (5606) Muramatsu; (23080) 1999 XH100 and (66875) 1999 VY52.

Photometric Observations of Main-Belt Asteroids 784 Pickeringia, 1465 Autonoma, 1477 Bonsdorffia, 3057 Malaren, 5708 Melancholia, and 8548 Sumizihara
Pages 16-19
Galdies, Charles; Brincat, Stephen M.; Bucek, Marek; Mifsud, Martin

Photometric observations of selected asteroids were done from Znith Observatory, Flarestar Observatory (MPC-171), Luckystar Observatory (MPC-M55), and Manikata Observatory in 2023. The observations were made during a favorable apparition for each asteroid. Some of these targets were never studied in the past and thus their rotation periods were unknown.

Lightcurves and Rotation Periods Of 903 Nealley, 1051 Merope, and 1187 Afra
Pages 19-21
Pilcher, Frederick

Synodic rotation periods and amplitudes at their year 2023 oppositions are found for 903 Nealley 29.063 ± 0.006 hours, 0.06 ± 0.01 magnitudes with one maximum and minimum per rotational cycle; 1051 Merope 13.712 ± 0.001 hours, 0.17 ± 0.01 magnitudes with one maximum and minimum per rotational cycle; 1187 Afra 14.071 ± 0.001 hours, 0.68 ± 0.05 magnitudes.

Asteroid Lightcurve Analysis at the Center for Solar System Studies Palmer Divide Station: 2023 July-October
Pages 22-30
Warner, Brian D.

CCD photometric observations of 22 asteroids were made at the Center for Solar System Studies Palmer Divide Station during 2023 July to October. Data analysis found four likely binary asteroids: 7187 Isobe, 20037 Duke, 21149 Kenmitchell, and (53453) 1999 XX135. A review of data from 2018 for 17405 McAdams found a period somewhat near half that found using 2023 data. As standalone solutions, both would seem to be valid.

Asteroid Photometry from the Dunwurkin Observatory
Pages 31-32
Clark, Maurice

Asteroid period and amplitude results obtained at the Dunwurkin Observatory in Koorda Western Australia during May and July 2023 are presented.

Lightcurve Analysis for Twelve Main-Belt and One PHA Asteroids
Pages 33-38
Fornas, Gonzalo; Huet, Fernando; Barberá, Rafael; Fornas, Álvaro; Mas, Vicente

Photometric observations of twelve main-belt asteroids and one PHA were obtained between 2023/1/11 - 2023/7/17. We derived the following rotational synodic periods: 489 Comacina, 9.0250 ± 0.0012 h; 600 Musa, 5.88647 ± 0.00064 h; 716 Berkeley, 15.580657 ± 0.00048 h; 907 Rhoda, 22.4700 ± 0.0008 h; 1354 Botha, 8.3776 ± 0.0007 h; 3210 Lupishko, 14.247 ± 0.002 h; 3286 Anatoliya, 5.8103 ± 0.0009 h; 3379 Oishi, 19.2199 ± 0.019 h; 11736 Viktorfischl, 9.78407 ± 0.0012 h; 13653 Priscus, 6.7498 ± 0.0022 h; (23552) 1994 NB, 3.63175 ± 0.00052; (37638) 1993 VB, 3.529 ± 0.001 h; (76644) 2000 HY24, 9.6625 ± 0.012 h. And the following sidereal periods: 716 Berkeley, 15.57505 ± 0.00007 h; 11736 Victorfischl, 9.78218 ± 0.00003 h; (23552) 1994 NB, 3.628683 ± 0.000004; (76644) 2000 HY24, 9.702441± 0.00005 h.

Asteroid Photometry and Lightcurves for Twelve Asteroids – September 2023
Pages 39-41
Milagros Colazo; Fornari, César; Suárez, Néstor; Morales, Mario; Garcí, Alberto; Scotta, Damián; Melia, Raúl; Speranza, Tiago; Stechina, Ariel; Monteleone, Bruno; Cianci, Giuseppe; Wilberge, Aldo; Suligoy, Matías; Ortiz, Axel; Santos, Francisco; Colazo, Carlos

Synodic rotation periods and amplitudes are reported for: 830 Petropolitana, 931 Whittemora, 953 Painleva, 1064 Aethusa, 1199 Geldonia, 1465 Autonoma, 1937 Locarno, 4569 Baerbel.

Lightcurves of Eighteen Asteroids
Pages 42-49
Dose, Eric V.

We present lightcurves and synodic rotation periods for eighteen asteroids observed July through October 2023.

Photometric Results for Ten Minor Planets
Pages 49-53
Polakis, Tom

Photometric measurements were made for 10 main-belt asteroids, based on CCD observations made from 2023 September through 2023 October. Phased lightcurves were created for all ten asteroids, and an orbital period was computed for one binary asteroid. All the data have been submitted to the ALCDEF database.

Lightcurve and Rotation Period Analysis of 4226 Damiaan and (25242) 1998 UH15
Pages 54-55
Hawley, W.; Miles, R.; Wiggins, P.; McCormick, J.; Dawson, M.; Pilcher, F.

Photometric observations of two main-belt asteroids were obtained between 2023 July 7 and 2021 October 3. The following rotational periods were determined: 4226 Damiaan, 32.639 ± 0.005 h; (25242) 1998 UH15, 7.869 ± 0.002 h. Images were obtained from observatories around the globe. Several of the co-authors used their own equipment while others used the Las Cumbres Observatory facilities.

Collaborative Asteroid Photometry from UAI: 2023 July-September
Pages 56-61
Franco, Lorenzo; Scarfi, Giulio; Baj, Giorgio; Iozzi, Marco; Lombardo, Matteo; Marchini, Alessandro; Papini, Riccardo; Falco, Carmelo; Nastasi, Alessandro; Fini, Paolo; Betti, Guido; Arangio, Julie; Bacci, Paolo; Maestripieri, Martina; Montigiani, Nico; Mannucci, Massimiliano; Coffano, Alessandro; Marinello, Wladimiro; Aceti, Pietro; Banfi, Massimo; Galli, Gianni; Ruocco, Nello; Tinelli, Luciano

Photometric observations of nine asteroids were made in order to acquire lightcurves for shape/spin axis modeling. Lightcurves were acquired for 81 Terpsichore, 238 Hypatia, 773 Irmintraud, 862 Franzia, 894 Erda, 914 Palisana, 2763 Jeans, 5766 Carmelofalco, and (458732) 2011 MD5.

Lightcurve Analysis of Asteroids 6108 Glebov, 6991 Chichibu and 10039 Keet Seel
Pages 62-63
Marchini, Alessandro; Papini, Riccardo

Photometric observations of three main-belt asteroids were conducted to determine their synodic rotation periods. We found: for 6108 Glebov, P = 2.832 ± 0.002 h with A = 0.09 ± 0.03 mag; for 6991 Chichibu, P = 9.492 ± 0.001 h with A = 0.18 ± 0.03 mag; for 10039 Keet Seel, P = 36.99 ± 0.02 h with A = 0.16 ± 0.03 mag.

Lightcurve and Rotation Period for Minor Planets 2090 Mizuho (1978 EA) and 4164 Shilov (1969 UR)
Pages 64-65
Foylan, Mike

CCD photometric observations of main-belt asteroids 2090 Mizuho (1978 EA) and 4164 Shilov (1969 UR) were acquired during 2023 September and October and 2016 October and November, respectively. A synodic rotation period of 5.4792 ± 0.0024 h and amplitude of A = 0.22 ± 0.03 mag were determined for 2090 Mizuho and 74.500 ± 0.072 h and amplitude of A = 0.84 ± 0.05 mag were determined for 4164 Shilov.

Lightcurve Analysis for Six Near-Earth Asteroids Observed in 2009, 2017 and 2023
Pages 66-71
Birtwhistle, Peter

Lightcurves and amplitudes for six small near-Earth asteroids observed from Great Shefford Observatory during close approaches in 2009, 2017, and August to October 2023 are reported. Five have rotation periods less than 20 minutes, two are reliably detected tumblers and another is a possible tumbler.

Photometry and Lightcurve Analysis of Eight Near-Earth Asteroids
Pages 72-76
Pereira, Weslley; Arcoverde, Plícida; Evangelista-Santana, Marçal; Michimani, Jonatan; Rondón, Eduardo; Monteiro, Filipe; Mesquita, Wesley; Côrrea, Tatiane; Souza, Roberto; Rodrigues, Teresinha; Lazzaro, Daniela

Rotational periods of eight near-Earth asteroids (NEAs) were determined from the lightcurve analysis of photometric observations acquired at the Observatório Astronômico do Sertão de Itaparica (MPC Y28, OASI) from 2021 January to 2023 July.

Rotation Periods of Five Near-Earth Asteroids with the Trappist Telescopes: (17188) 1999 WC2, (242450) 2004 QY2, (503871) 2000 SL, 2023 DZ2 And 2023 CM
Pages 76-78
Miftah, Mohamed Amine; Ferrais, Marin; Moulane, Youssef; Jehin, Emmanuël; Jabiri, Abdelhadi; Benkhaldoun, Zouhair

Lightcurves of five near-Earth asteroids were obtained with TRAPPIST-North and TRAPPIST-South from December 2022 to May 2023. For all of them the synodic rotation period and amplitude were found to be: (17188) 1999 WC2, (5.064 ± 0.002 h) and (0.35 ± 0.02 mag); (242450) 2004 QY2, (7.072 h ± 0.001 h) and (0.30 ± 0.01 mag); (503871) 2000 SL, (10.6504 h ± 0.0020 h) and (0.32 ± 0.04 mag); 2023 DZ2, (0.104587 ± 0.000083 h) and (0.58 ± 0.02 mag); 2023 CM, (3.6244 ± 0.0004 h) and (0.24 ± 0.02 mag). All data have been submitted to ALCDEF database.

Minor Planets at Unusually Favorable Elongations in 2024
Pages 79-81
Pilcher, Frederick

A list is presented of minor planets which are much brighter than usual at their 2024 apparitions.

Asteroid-Deepsky Appulses in 2024
Pages 82
Warner, Brian D.

The following list is a very small subset of the results of a search for asteroid-deepsky appulses for 2024, presenting only the highlights for the year based on close approaches of brighter asteroids to brighter DSOs

Lightcurve Photometry Opportunities: 2024 January-March
Pages 83-86
Warner, Brian D.; Harris, Alan W.; Durech, Josef; Benner, Lance A.M.

We present lists of asteroid photometry opportunities for objects reaching a favorable apparition and have no or poorly-defined lightcurve parameters. Additional data on these objects will help with shape and spin axis modeling using lightcurve inversion. We have changed the presentation of the “Radar-Optical Opportunities” section to include a list of potential radar targets as well as some that are in critical need of astrometric data and, if found, might also be targets for radar. These can have ephemeris errors on the order of tens to thousands of arcseconds and, despite the current surveys, have not been observed for several years. This makes them a double challenge: first to be found and, second, to determine astrometric positions and photometric properties.

In This Issue
Pages 87
Warner, Brian D.

This list gives those asteroids in this issue for which physical observations (excluding astrometric only) were made. This includes lightcurves, color index, and H-G determinations, etc. In some cases, no specific results are reported due to a lack of or poor quality data. The page number is for the first page of the paper mentioning the asteroid. EP is the "go to page" value in the electronic version.


copyright©2017-2022 Brian D. Warner. Funding to support this web site was provided by NASA grant NSSC 80NSSC18K0851 prior to 2021 April.