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Literature DB >> 32455368

ASTEROID LIGHTCURVE ANALYSIS AT CS3-PALMER DIVIDE STATION: 2015 JUNE-SEPTEMBER.

Abstract

Lightcurves for 29 main-belt asteroids were obtained at the Center for Solar System Studies-Palmer Divide Station (CS3-PDS) from 2015 June-September. Hungaria members 1876 Napolitania and (47141) 1999 HB3 are suspected binary asteroids.

Entities: Chemical

Year: 2016 PMID： 32455368 PMCID： PMC7244003

Source DB: PubMed Journal: Minor Planet Bull

8 in total

1. Formation of asteroid pairs by rotational fission.

Authors: P Pravec; D Vokrouhlický; D Polishook; D J Scheeres; A W Harris; A Galád; O Vaduvescu; F Pozo; A Barr; P Longa; F Vachier; F Colas; D P Pray; J Pollock; D Reichart; K Ivarsen; J Haislip; A Lacluyze; P Kusnirák; T Henych; F Marchis; B Macomber; S A Jacobson; Yu N Krugly; A V Sergeev; A Leroy
Journal: Nature Date: 2010-08-26 Impact factor: 49.962

18 in total

ASTEROID LIGHTCURVE ANALYSIS AT CS3-PALMER DIVIDE STATION: 2015 JUNE-SEPTEMBER.

1. Formation of asteroid pairs by rotational fission.

2. ASTEROID LIGHTCURVE ANALYSIS AT CS3-PALMER DIVIDE STATION: 2013 SEPTEMBER-DECEMBER.

3. ASTEROID LIGHTCURVE ANALYSIS AT CS3-PALMER DIVIDE STATION: 2014 JANUARY-MARCH.

4. ASTEROID LIGHTCURVE ANALYSIS AT THE PALMER DIVIDE OBSERVATORY: 2012 JUNE - SEPTEMBER.

5. ASTEROID LIGHTCURVE ANALYSIS AT CS3-PALMER DIVIDE STATION: 2014 MARCH-JUNE.

6. ROUNDING UP THE UNUSUAL SUSPECTS.

7. ASTEROID LIGHTCURVE ANALYSIS AT THE PALMER DIVIDE OBSERVATORY: 2012 SEPTEMBER - 2013 JANUARY.

8. ASTEROID LIGHTCURVE ANALYSIS AT THE PALMER DIVIDE OBSERVATORY: 2013 JANUARY - MARCH.

1. ASTEROID LIGHTCURVE ANALYSIS AT CS3-PALMER DIVIDE STATION: 2013 SEPTEMBER-DECEMBER.

2. ASTEROID LIGHTCURVE ANALYSIS AT CS3-PALMER DIVIDE STATION: 2014 JANUARY-MARCH.

3. MAIN-BELT ASTEROIDS OBSERVED FROM CS3: 2019 JULY TO SEPTEMBER.

4. ANOTHER TRIO OF POSSIBLE VERY WIDE BINARY ASTEROIDS.

5. NEAR-EARTH ASTEROID LIGHTCURVE ANALYSIS AT CS3-PALMER DIVIDE STATION: 2016 JANUARY-APRIL.

6. ASTEROID LIGHTCURVE ANALYSIS AT CS3-PALMER DIVIDE STATION: 2014 OCTOBER-DECEMBER.

7. A SEXTET OF MAIN-BELT BINARY ASTEROID CANDIDATES.

8. ASTEROID LIGHTCURVE ANALYSIS AT THE PALMER DIVIDE OBSERVATORY: 2013 FEBRUARY-MARCH. THE FINAL REPORT.

9. TWO NEW BINARIES AND CONTINUING OBSERVATIONS OF HUNGARIA GROUP ASTEROIDS.

10. A TRIO OF BINARY ASTEROIDS.