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Palomar discovery and initial characterization of naked-eye long-period comet C/2022 E3 (ZTF).
- Source :
- Monthly Notices of the Royal Astronomical Society: Letters; Jan2024, Vol. 527 Issue 1, pL42-L46, 5p
- Publication Year :
- 2024
-
Abstract
- Long-period comets are planetesimal remnants constraining the environment and volatiles of the protoplanetary disc. We report the discovery of hyperbolic long-period comet C/2022 E3 Zwicky Transient Facility (ZTF), which has a perihelion ∼1.11 au, an eccentricity ≳1 and an inclination ∼109°, from images taken with the Palomar 48-inch telescope during morning twilight on 2022 March 2. Additionally, we report the characterization of C/2022 E3 (ZTF) from observations taken with the Palomar 200-inch, the Palomar 60-inch, and the NASA Infrared Telescope Facility in early 2023 February to 2023 March when the comet passed within ∼0.28 au of the Earth and reached a visible magnitude of ∼5. We measure g – r = 0.70 ± 0.01, r – i = 0.20 ± 0.01, i – z = 0.06 ± 0.01, z – J = 0.90 ± 0.01, J – H = 0.38 ± 0.01, and H – K = 0.15 ± 0.01 colours for the comet from observations. We measure the A(0°)fρ (0.8 μm) in a 6500 km radius from the nucleus of 1483 ± 40 cm, and CN, C<subscript>3</subscript>, and C<subscript>2</subscript> production of 5.43 ± 0.11 × 10<superscript>25</superscript>, 2.01 ± 0.04 × 10<superscript>24</superscript>, and 3.08 ± 0.5 × 10<superscript>25</superscript> mol s<superscript>−1</superscript>, similar to other long-period comets. We additionally observe the appearance of jet-like structures at a scale of ∼4000 km in wide-field g -band images, which may be caused by the presence of CN gas in the near-nucleus coma. [ABSTRACT FROM AUTHOR]
- Subjects :
- COMETS
PROTOPLANETARY disks
SMALL solar system bodies
TWILIGHT
TELESCOPES
Subjects
Details
- Language :
- English
- ISSN :
- 17453925
- Volume :
- 527
- Issue :
- 1
- Database :
- Complementary Index
- Journal :
- Monthly Notices of the Royal Astronomical Society: Letters
- Publication Type :
- Academic Journal
- Accession number :
- 173856373
- Full Text :
- https://doi.org/10.1093/mnrasl/slad139