PHOTOMETRY OF COMET С/2009 P1 (GARRADD) BEFORE AND AFTER PERIHELION

Journal Title: Odessa Astronomical Publications - Year 2018, Vol 31, Issue

Abstract

During the period from September 2011 to February 2012, photometric observations of comet C/2009 P1 (Garradd) were performed on the 0.6-m telescope MC AMED at the peak Terskol (North-Caucasus). The paper presents an analysis of photometric observations of Comet C/2009 P1 (Garradd) obtained for heliocentric distances of 2.0-2.1 au before and 1.7-1.8 au after perihelion passage. The measurements of the comet were performed using a CCD camera SiTe003AB with narrow-band comet filters BC (λ4450/67Å), GC(λ5260/56Å), RC(λ7128/58Å) and C2(λ5141/118Å), CN(λ3870/62Å) HB-set (Farnham T., 2000). Observation data were obtained during 11 nights. According to the results of observations, the dust production Afρ (A’Hearn M.F. et al., 1984) of comet, the gas production of comet for molecules C2, CN using the Hazer model (Haser L., 1957), dust-to-gas ratio and color were calculated. The obtained results showed that the physical parameters of the comet are close to the average characteristics typical for dynamically new comets.

Authors and Affiliations

S. F. Velichko, M. V. Andreev

Keywords

Related Articles

PHYSICAL PARAMETERS OF PROTOPLANETARY DISK SURROUNDING IRAS 22150+6109 YOUNG STAR

IRAS 22150+6109 star belongs to L 1188 star forming region in Perseus, according to [1] located at distance of 910 pc from the Sun. Photometric observations in the visible range that were carried out in 1997-1999 have re...

Molybdenum abundance in some open clusters

This paper presents the results of determination of the molybdenum abundances in 13 G, K type stars in the open clusters NGC 2477 and NGC 2506. The abundances of molybdenum were determined using stellar atmosphere models...

Hα AND Hβ PROFILE VARIATIONS IN THE SPECTRA OF THE STAR 55 CYG

We study the variability of the Hα and Hβ lines in the spectra of 55 Cyg based on observations acquired in 2014 on the 2-m telescope of Shamakhy Astrophysical Observatory. In this work line profiles...

”ASYMPTOTIC PARABOLA” FITS FOR SMOOTHING GENERALLY ASYMMETRIC LIGHT CURVES

A computer program is introduced, which allows to determine statistically optimal approximation using the "Asymptotic Parabola" fit, or, in other words, the spline consisting of polynomials of order 1,2,1, or two lines (...

PULSATIONAL ACTIVITY OF THE SMALL–AMPLITUDE CEPHEID POLARIS (α UMi) IN 2016-2017

We present the results of an analysis of 49 spectra of α UMi (Polaris) obtained during August – December 2016 and January – March 2017. Frequency analysis displays an unexpected decrease of the pulsational period up to 1...

Download PDF file
  • EP ID EP603749
  • DOI 10.18524/1810-4215.2018.31.144748
  • Views 74
  • Downloads 0

How To Cite

S. F. Velichko, M. V. Andreev (2018). PHOTOMETRY OF COMET С/2009 P1 (GARRADD) BEFORE AND AFTER PERIHELION. Odessa Astronomical Publications, 31(), 196-198. https://www.europub.co.uk/articles/-A-603749