Two’s company

Esahubble_potw2414a_1024

esahubble_potw2414a April 1st, 2024

Credit: ESA/Hubble & NASA, L. Galbany, J. Dalcanton, Dark Energy Survey/DOE/FNAL/DECam/CTIO/NOIRLab/NSF/AURA

This image features Arp 72, a very selective galaxy group that only includes two interacting galaxies: NGC 5996 (the large spiral galaxy) and NGC 5994 (its smaller companion, in the lower left of the image). Both galaxies lie approximately 160 million light-years from Earth, and their cores are separated from each other by a distance of around 67 thousand light-years. Moreover, the distance between the galaxies at their closest points is even smaller, closer to 40 thousand light-years. Whilst this might still sound vast, in galactic separation terms it is really very cosy! For comparison, the distance between the Milky Way and its nearest independent galactic neighbour Andromeda is around 2.5 million light-years. Alternatively, the distance between the Milky Way and its largest and brightest satellite galaxy, the Large Magellanic Cloud (satellite galaxies are galaxies that are bound in orbit around another galaxy), is about 162 thousand light-years.  Given this, coupled with the fact that NGC 5996 is roughly comparable in size to the Milky Way, it is not surprising that NGC 5996 and NGC 5994 — apparently separated by only 40 thousand light-years or so — are interacting with one another. In fact, the interaction might be what has caused the spiral shape of NGC 5996 to distort and apparently be drawn in the direction of NGC 5994. It also prompted the formation of the very long and faint tail of stars and gas curving away from NGC 5996, up to the top right of the image. This ‘tidal tail’ is a common phenomenon that appears when galaxies get in close together, as can be seen in several Hubble images. [Image Description: A large spiral galaxy with a smaller neighbouring galaxy. The spiral galaxy is wide and distorted, with colourful dust. Its companion lies close by it at the end of a spiral arm, to the lower left. A long, faint tail of stars reaches up from the right side of the spiral galaxy to the top of the image. Several small, distant galaxies can be seen in the background, as well as one bright star in the foreground.]Links Pan video: Arp 72

Provider: Hubble Space Telescope | ESA

Image Source: https://esahubble.org/images/potw2414a/

Curator: ESA/Hubble, Baltimore, MD, United States

Image Use Policy: Creative Commons Attribution 4.0 International License

Image Details Image Details

Image Type
Observation
Object Name
Arp 72
Esahubble_potw2414a_128
 

Position Details Position Details

Position (ICRS)
RA = 15h 46m 58.7s
DEC = 17° 52’ 48.3”
Orientation
North is 124.3° CW
Field of View
3.2 x 2.6 arcminutes
Constellation
Serpens

Color Mapping Details Color Mapping

  Telescope Spectral Band Wavelength
Blue Blanco-4m (DECam) Optical (G) 474.0 nm
Green Blanco-4m (DECam) Optical (R) 644.0 nm
Red Blanco-4m (DECam) Optical (Z) 919.0 nm
Luminosity Hubble (ACS) Optical (V) 606.0 nm
Purple Hubble (WFC3) Ultraviolet (UV) 275.0 nm
Spectrum_base
Blue
Green
Red
Luminosity
Purple
Esahubble_potw2414a_1280
×
ID
potw2414a
Subject Category
Subject Name
Arp 72
Credits
ESA/Hubble & NASA, L. Galbany, J. Dalcanton, Dark Energy Survey/DOE/FNAL/DECam/CTIO/NOIRLab/NSF/AURA
Release Date
2024-04-01T06:00:00
Lightyears
Redshift
Reference Url
https://esahubble.org/images/potw2414a/
Type
Observation
Image Quality
Distance Notes
Facility
Víctor M. Blanco 4-meter Telescope, Víctor M. Blanco 4-meter Telescope, Víctor M. Blanco 4-meter Telescope, Hubble Space Telescope, Hubble Space Telescope
Instrument
DECam, DECam, DECam, ACS, WFC3
Color Assignment
Blue, Green, Red, Luminosity, Purple
Band
Optical, Optical, Optical, Optical, Ultraviolet
Bandpass
G, R, Z, V, UV
Central Wavelength
474, 644, 919, 606, 275
Start Time
Integration Time
Dataset ID
None, None, None, None, None
Notes
Coordinate Frame
ICRS
Equinox
J2000
Reference Value
236.7447503327549, 17.880089233474347
Reference Dimension
3884.0, 3107.0
Reference Pixel
1942.0, 1553.5
Scale
-1.3890859611487946e-05, 1.3890859611487946e-05
Rotation
-124.30000000000008
Coordinate System Projection:
TAN
Quality
Full
FITS Header
Notes
Creator (Curator)
ESA/Hubble
URL
https://esahubble.org
Name
Email
Telephone
Address
ESA Office, Space Telescope Science Institute, 3700 San Martin Dr
City
Baltimore
State/Province
MD
Postal Code
21218
Country
United States
Rights
Creative Commons Attribution 4.0 International License
Publisher
ESA/Hubble
Publisher ID
esahubble
Resource ID
potw2414a
Metadata Date
2024-03-25T12:35:04+01:00
Metadata Version
1.1
×

 

Detailed color mapping information coming soon...

×

There is no distance meta data in this image.

 

Providers | Sign In