New insights into debris discs

Eso_potw1621a_1024

eso_potw1621a May 23rd, 2016

Credit: ESO/Marino et al.

Using 39 of the 66 antennas of the Atacama Large Millimeter/submillimeter Array (ALMA), located 5000 metres up on the Chajnantor plateau in the Chilean Andes, astronomers have been able to detect carbon monoxide (CO) in the disc of debris around an F-type star. Although carbon monoxide is the second most common molecule in the interstellar medium, after molecular hydrogen, this is the first time that CO has been detected around a star of this type. The star, named HD 181327, is a member of the Beta Pictoris moving group, located almost 170 light-years from Earth. Until now, the presence of CO has been detected only around a few A-type stars, substantially more massive and luminous than HD 181327. Using the superb spatial resolution and sensitivity offered by the ALMA observatory astronomers were now able to capture this stunning ring of smoke and map the density of the CO within the disc. The study of debris discs is one way to characterise planetary systems and the results of planet formation. The CO gas is found to be co-located with the dust grains in the ring of debris and to have been produced recently. Destructive collisions of icy planetesimals in the disc are possible sources for the continuous replenishment of the CO gas. Collisions in debris discs typically require the icy bodies to be gravitationally perturbed by larger objects in order to reach sufficient collisional velocities. Moreover, the derived CO composition of the icy planetesimals in the disc is consistent with the comets in our Solar System. This possible secondary origin for the CO gas suggests that icy comets could be common around stars similar to our Sun which has strong implications for life suitability in terrestrial exoplanets. The results were published in the journal Monthly Notices of the Royal Astronomical Society under the title “Exocometary gas in the HD 181327 debris ring” by S. Marino et al. Link: Paper by Marino et al.

Provider: European Southern Observatory

Image Source: https://www.eso.org/public/images/potw1621a/

Curator: European Southern Observatory, Garching bei München, Germany

Image Use Policy: Creative Commons Attribution 4.0 International License

Image Details Image Details

Image Type
Observation
Object Name
HD 181327
Subject - Milky Way
Star > Circumstellar Material > Disk > Debris
Eso_potw1621a_128
 

Position Details Position Details

Position (ICRS)
RA = 19h 22m 59.0s
DEC = -54° 32’ 18.2”
Orientation
North is up
Field of View
0.1 x 0.1 arcminutes
Constellation
Telescopium

Color Mapping Details Color Mapping

  Telescope Spectral Band Wavelength
Orange ALMA (None) Millimeter (220 GHz) -
Eso_potw1621a_1280
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ID
potw1621a
Subject Category
B.3.7.2.3  
Subject Name
HD 181327
Credits
ESO/Marino et al.
Release Date
2016-05-23T06:00:00
Lightyears
Redshift
Reference Url
https://www.eso.org/public/images/potw1621a/
Type
Observation
Image Quality
Distance Notes
Facility
Atacama Large Millimeter/submillimeter Array
Instrument
None
Color Assignment
Orange
Band
Millimeter
Bandpass
220 GHz
Central Wavelength
Start Time
Integration Time
Dataset ID
Notes
Coordinate Frame
ICRS
Equinox
J2000
Reference Value
290.745805624, -54.538391248
Reference Dimension
2000.0, 2000.0
Reference Pixel
1000.0, 1000.0
Scale
-1.05397609661e-06, 1.05397609661e-06
Rotation
-0
Coordinate System Projection:
TAN
Quality
Full
FITS Header
Notes
Creator (Curator)
European Southern Observatory
URL
http://www.eso.org
Name
Email
Telephone
Address
Karl-Schwarzschild-Strasse 2
City
Garching bei München
State/Province
Postal Code
D-85748
Country
Germany
Rights
Creative Commons Attribution 4.0 International License
Publisher
European Southern Observatory
Publisher ID
eso
Resource ID
potw1621a
Metadata Date
2023-10-11T09:21:20.815018
Metadata Version
1.1
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Detailed color mapping information coming soon...

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There is no distance meta data in this image.

 

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