Zobrazeno 1 - 10
of 135
pro vyhledávání: '"Brian D, Warner"'
Autor:
Marina Brozović, Lance A. M. Benner, Shantanu P. Naidu, Nicholas Moskovitz, Jon D. Giorgini, Anne K. Virkki, Sean E. Marshall, Lord R. Dover, Agata Rożek, Stephen C. Lowry, Brian D. Warner, Patrick A. Taylor, Edgard G. Rivera-Valentin, Timothy A. Lister, Joseph P. Chatelain, Michael W. Busch, Christopher Magri, Joseph S. Jao, Lawrence G. Snedeker, Kenneth J. Lawrence
Publikováno v:
The Planetary Science Journal, Vol 5, Iss 5, p 123 (2024)
We report radar, photometric, and visible-wavelength spectrophotometry observations of NEA 2018 EB obtained in 2018. The radar campaign started at Goldstone (8560 MHz, 3.5 cm) on April 7, and it was followed by more extensive observations from Octobe
Externí odkaz:
https://doaj.org/article/7e03b22d7c0e49b3a7984d46681d32ff
Autor:
Brian D, Warner
Publikováno v:
Minor Planet Bull
Lightcurves for 40 main-belt asteroids were obtained at the Center for Solar System Studies-Palmer Divide Station (CS3-PDS) from 2014 January through March. The majority of the objects were members of the Hungaria group/family. In many cases, the obs
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=pmid________::de35a97eaf2b8fb82f73a3a3d5fedd16
https://pubmed.ncbi.nlm.nih.gov/32549049
https://pubmed.ncbi.nlm.nih.gov/32549049
Autor:
Brian D, Warner
Publikováno v:
Minor Planet Bull
Lightcurves for 13 main-belt asteroids were obtained at the Center for Solar System Studies-Palmer Divide Station (CS3-PDS) from 2014 December through 2015 March. All but two were members of the Hungaria orbital group or collisional family and observ
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=pmid________::96609ccf4a9e963417b5c9699dd9b2f4
https://pubmed.ncbi.nlm.nih.gov/32549044
https://pubmed.ncbi.nlm.nih.gov/32549044
Autor:
Brian D, Warner
Publikováno v:
Minor Planet Bull
Lightcurves for 41 asteroids were obtained at the Palmer Divide Observatory (PDO) from 2013 January through March: 785 Zwetana, 1509 Esclangona, 1599 Giomus, 1925 Franklin-Adams, 2048 Dwornik, 2491 Tvashtri, 3007 Reaves, 3720 Hokkaido, 4719 Burnaby,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=pmid________::2afbf8cea3ec39f28532e4c6657dfc57
https://pubmed.ncbi.nlm.nih.gov/32494785
https://pubmed.ncbi.nlm.nih.gov/32494785
Publikováno v:
Minor Planet Bull
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 via lightcurve inversi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=pmid________::0ab1e3989c2e333a93aa7f12c9cc8660
https://pubmed.ncbi.nlm.nih.gov/32494789
https://pubmed.ncbi.nlm.nih.gov/32494789
Autor:
Brian D, Warner
Publikováno v:
Minor Planet Bull
Lightcurves for 40 asteroids were obtained at the Palmer Divide Observatory (PDO) from 2012 September to 2013 January: 495 Eulalia, 1694 Kaiser, 2001 Einstein, 3086 Kalbaugh, 3635 Kreutz, 5806 Archieroy, 6310 Jankonke, 6447 Terrycole, 6744 Komoda, 70
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=pmid________::c316b90e9c043615869beb5db1164791
https://pubmed.ncbi.nlm.nih.gov/32494783
https://pubmed.ncbi.nlm.nih.gov/32494783
Autor:
Brian D, Warner
Publikováno v:
Minor Planet Bull
The very wide binary asteroids (VWBA) are a subgroup of binary asteroids that exhibit very long primary periods and, mostly, short secondary periods that are similar to those of the primary of “normal” small binary asteroids. It is unlikely that
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=pmid________::ddf95444f810525eae0d5c2e1bc839cb
https://pubmed.ncbi.nlm.nih.gov/32455385
https://pubmed.ncbi.nlm.nih.gov/32455385
Autor:
Brian D, Warner
Publikováno v:
Minor Planet Bull
Three Hungaria asteroids observed at the Center for Solar System Studies-Palmer Divide Station (CS3-PDS) in 2015 January-March showed unusual characteristics. 2449 Kenos, a probable member of the Hungaria collisional family, is likely to be a binary
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=pmid________::35351082d70c8d4d5f0c800758fcc9e7
https://pubmed.ncbi.nlm.nih.gov/32455356
https://pubmed.ncbi.nlm.nih.gov/32455356
Autor:
Brian D, Warner, Amadeo Aznar, Macías
Publikováno v:
Minor Planet Bull
Analysis of CCD photometric observations in late 2015 of the Hungaria asteroid 6384 Kervin indicates that it may be a binary asteroid with a primary lightcurve of P(1) = 3.6194 ± 0.0001 h, A(1) = 0.06 ± 0.01 mag. The secondary lightcurve parameters
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=pmid________::2f014099693649b2f595420c143e1389
https://pubmed.ncbi.nlm.nih.gov/32455378
https://pubmed.ncbi.nlm.nih.gov/32455378
Autor:
Brian D, Warner, Robert D, Stephens
Publikováno v:
Minor Planet Bull
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=pmid________::ac53b7349e2a825e5864d69e6b71f91d
https://pubmed.ncbi.nlm.nih.gov/32455411
https://pubmed.ncbi.nlm.nih.gov/32455411