2025A&A...699A.110F


Query : 2025A&A...699A.110F

2025A&A...699A.110F - Astronomy and Astrophysics, volume 699A110 (2025/7-1)

Alkali phenoxides in comets.

FULLE M., MOLARO P., ROTUNDI A., TONIETTI L., ALETTI A., BUZZI L. and VALISA P.

Abstract (from CDS):

Context. Potassium was first detected in spectra of the sungrazer comet C/1965 S1 Ikeya-Seki at the heliocentric distance rh = 0.15 au and, 48 years later, in comets C/2011 L4 PanSTARRS and C/2012 S1 ISON at rh = 0.46 au. The alkali tail photoionization model provides a Na/K ratio close to the solar value in comets C/1965 S1 and C/2011 L4. No lithium was detected in any comet: the lower limit of the Na/Li ratio was almost one order of magnitude greater than the solar ratio.
Aims. Here we searched for the emissions of the alkali NaI, KI, and LiI in Comets C/2020 F3 NEOWISE and C/2024 G3 ATLAS.
Methods. High-resolution spectra of the comets were taken with the 0.84 m telescope at the Schiaparelli Observatory at rh = 0.36 and rh = 0.15 au, respectively, the observations closest to the Sun since C/1965 S1. To model the data, we assumed that alkali phenoxides are present in the aromatic fraction of organic dust at the nucleus surface where they react with carbon dioxide ejecting alkali atoms. Results. NaI and KI were detected in emission lines of exceptional intensity in both comets, with no evidence of LiI emission. The NaI/KI ratios were determined: 31 ± 5 and 26 ± 8 in comets C/2020 F3 and C/2024 G3, respectively, whereas solar Na/K ≈ 15. This excess and its observed trend with the heliocentric distance are consistent with chemistry between CO2 and alkali phenoxides at the nucleus surface. The Li upper limit for comet C/2020 F3 is very stringent at Na/Li > 3.4 × 104, a factor of 34 greater than the solar value. This Li depletion is consistent with the reaction rate of lithium phenoxides, which is a factor of 104 slower than sodium phenoxides.
Conclusions. The widespread chemistry of carbon dioxide with organic dust may provide a significant energy and mass sink of carbon dioxide in all comets also at rh > 1 au, reconciling recent models of cometary activity with Rosetta CO2 measurements. At rh < 0.5 au potassium was observed in all comets, so that we predict the formation of a KI tail spatially resolved from the NaI tail.

Abstract Copyright: © The Authors 2025

Journal keyword(s): molecular processes - techniques: spectroscopic - comets: general - comets: individual: Comet C/2024 G3 ATLAS - comets: individual: Comet C/2020 F3 NEOWISE

Simbad objects: 1

goto Full paper

goto View the references in ADS

Number of rows : 1
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 HD 31069 PM* 04 54 51.2429233200 +44 03 39.103253064   6.022 6.058     A0V 60 0

Query : 2025A&A...699A.110F

Basic data :
HD 31069 -- High Proper Motion Star
Other object types:
otypes_help
* (2019AJ,HD,...), UV (CEL,TD1), PM* (2016A&A), NIR (2MASS)
ICRS coord. (ep=J2000) :
04 54 51.2429233200 +44 03 39.103253064 (Optical) [ 0.0404 0.0294 90 ] A 2020yCat.1350....0G
FK4 coord. (ep=B1950 eq=1950) :
04 51 15.5733465561 +43 58 53.334869031 [ 0.0404 0.0294 90 ]
Gal coord. (ep=J2000) :
161.8069206066634 +00.3219344905998 [ 0.0404 0.0294 90 ]
Proper motions mas/yr :
21.778 -55.423 [0.068 0.052 90] A 2020yCat.1350....0G
Radial velocity / Redshift / cz :
V(km/s) 5.50 [2.8] / z(~) 0.000018 [0.000009] / cz 5.50 [2.80]
   C 2006AstL...32..759G
Parallaxes (mas):
10.1205 [0.0530] A 2020yCat.1350....0G
Spectral type:
A0V C ~
Fluxes (6) :
B 6.022 [0.014] D 2000A&A...355L..27H
V 6.058 [0.010] D 2000A&A...355L..27H
G 6.052764 [0.002791] C 2022yCat.1355....0G
J 6.048 [0.034] C 2003yCat.2246....0C
H 6.103 [0.038] C 2003yCat.2246....0C
K 6.107 [0.021] C 2003yCat.2246....0C
SIMBAD within arcmin
Overlay Simbad points in this preview
Back
All CDSPortal (CDSPortal)

Send to sendBySAMP sendBySAMP

sedIcon
within arcsec sed-help-icon

Hierarchy : number of linked objects
whatever the membership probability is (see description here ) :

: 1 : 6921 Display criteria :

Identifiers (28) :
An access of full data is available using the icon Vizier near the identifier of the catalogue

HD 31069 GEN# +1.00031069 ROT 687 UBV M 10408
AG+43 523 GSC 02906-02736 SAO 39851 uvby98 100031069
BD+43 1116 HIC 22842 SKY# 7662 WEB 4423
BSD 24-380 HIP 22842 TD1 3657 YPAC 361
CEL 481 HR 1558 TIC 367787291 Gaia DR2 205334041305995648
GC 5969 2MASS J04545124+4403391 TYC 2906-2736-1 Gaia DR3 205334041305995648
GCRV 2887 PPM 47482 UBV 4690 Gaia DR1 205334037007792896

References (60 between 1850 and 2026) (Total 60)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
Follow new references on this object
                Reference summaries :

                from: to:

                 or select by : (not exhaustive, explanation here)


Collections of Measurements Description of Measurements

Velocities : 7    Distance : 3    Rot : 1    Plx : 6    PM : 4    SpT : 4   

   


External archives :

Archive data at HEASARC - High-Energy Astrophysics Science Archive Research Center

Link by name to the catalogue in VizieR :

HD 31069 AG+43 523 BD+43 1116 CEL 481 GSC 02906-02736
HIC 22842 HIP 22842 HR 1558 2MASS J04545124+4403391 PPM 47482
SAO 39851 TD1 3657 TYC 2906-2736-1 uvby98 100031069 Gaia DR2 205334041305995648
Gaia DR3 205334041305995648 Gaia DR1 205334037007792896

Search by coordinates in Vizier (radius: 5 arcsec)


Annotations :
Annotations allow a user to add a note or report an error concerning the astronomical object and its data. It requires registration to post a note. See description .
Please, have a look at Best practices. The list of all annotations to SIMBAD objects can be found here .

The annotation server is currently not available. Sorry for any inconvenience


To bookmark this query, right click on this link: simbad:objects in 2025A&A...699A.110F and select 'bookmark this link' or equivalent in the popup menu