PHOTOMETRIC STUDY OF NPA ROTATOR (5247) KRYLOV

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F17%3A10367526" target="_blank" >RIV/00216208:11320/17:10367526 - isvavai.cz</a>

Výsledek na webu

<a href="http://dx.doi.org/10.5303/JKAS.2017.50.3.41" target="_blank" >http://dx.doi.org/10.5303/JKAS.2017.50.3.41</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.5303/JKAS.2017.50.3.41" target="_blank" >10.5303/JKAS.2017.50.3.41</a>

Jazyk výsledku

angličtina

Název v původním jazyce

PHOTOMETRIC STUDY OF NPA ROTATOR (5247) KRYLOV

Popis výsledku v původním jazyce

We conduct BVRI and R band photometric observations of asteroid (5247) Krylov from January 2016 to April 2016 for 51 nights using the Korea Microlensing Telescope Network (KMTNet). The color indices of (5247) Krylov at the light curve maxima are determined as B - V = 0.841 +/- 0.035, V - R = 0.418 +/- 0.031, and V - I = 0.871 +/- 0.031 where the phase angle is 14.1 degrees. They are acquired after the standardization of BVRI instrumental measurements using the ensemble normalization technique. Based on the color indices, (5247) Krylov is classified as a S-type asteroid. Double periods, that is, a primary period P-1 = 82.188 +/- 0.013 h and a secondary period P-2 = 67.13 +/- 0.20 h are identified from period searches of its R band light curve. The light curve phases with P-1 and this indicate that it is a typical Non-Principal Axis (NPA) asteroid. We discuss the possible causes of its NPA rotation.

Název v anglickém jazyce

PHOTOMETRIC STUDY OF NPA ROTATOR (5247) KRYLOV

Popis výsledku anglicky

We conduct BVRI and R band photometric observations of asteroid (5247) Krylov from January 2016 to April 2016 for 51 nights using the Korea Microlensing Telescope Network (KMTNet). The color indices of (5247) Krylov at the light curve maxima are determined as B - V = 0.841 +/- 0.035, V - R = 0.418 +/- 0.031, and V - I = 0.871 +/- 0.031 where the phase angle is 14.1 degrees. They are acquired after the standardization of BVRI instrumental measurements using the ensemble normalization technique. Based on the color indices, (5247) Krylov is classified as a S-type asteroid. Double periods, that is, a primary period P-1 = 82.188 +/- 0.013 h and a secondary period P-2 = 67.13 +/- 0.20 h are identified from period searches of its R band light curve. The light curve phases with P-1 and this indicate that it is a typical Non-Principal Axis (NPA) asteroid. We discuss the possible causes of its NPA rotation.

Druh

J_imp - Článek v periodiku v databázi Web of Science

CEP obor

—

OECD FORD obor

10308 - Astronomy (including astrophysics,space science)

Projekt

<a href="/cs/project/GA15-04816S" target="_blank" >GA15-04816S: Celkový obraz hlavního pásu planetek - fyzikální vlastnosti planetek odvozené inverzí optické a infračervené fotometrie</a><br>

Návaznosti

P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Rok uplatnění

2017

Kód důvěrnosti údajů

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Název periodika

Journal of the Korean Astronomical Society

ISSN

1225-4614

e-ISSN

—

Svazek periodika

50

Číslo periodika v rámci svazku

3

Stát vydavatele periodika

KR - Korejská republika

Počet stran výsledku

9

Strana od-do

41-49

Kód UT WoS článku

000404833900001

EID výsledku v databázi Scopus

—