Asteroids in Hubble Frontier Field Abell 370

Esahubble_opo1733b_1024

esahubble_opo1733b November 6th, 2017

Credit: NASA, ESA, and B. Sunnquist and J. Mack (STScI) Acknowledgment: NASA, ESA, and J. Lotz (STScI) and the HFF Team

As if this Hubble Space Telescope picture isn't cluttered enough with myriad galaxies, nearby asteroids photobomb the image, their trails sometimes mimicking background astronomical phenomena. The stunningly beautiful galaxy cluster Abell 370 contains an astounding assortment of several hundred galaxies tied together by the mutual pull of gravity. Located approximately 4 billion light-years away in the constellation Cetus, the Sea Monster, this immense cluster is a rich mix of a variety of galaxy shapes. Entangled among the galaxies are thin, white trails that look like curved or S-shaped streaks. These are trails from asteroids that reside, on average, only about 260 million kilometres from Earth right around the corner in astronomical terms. The trails appear in multiple Hubble exposures that have been combined into one image. Of the 22 total asteroid sightings for this field, five are unique objects. These asteroids are so faint that they were not previously identified. The asteroid trails look curved due to an observational effect called parallax. As Hubble orbits around Earth, an asteroid will appear to move along an arc with respect to the vastly more distant background stars and galaxies. The motion of Earth around the Sun, and the motion of the asteroids along their orbits, are other contributing factors to the apparent skewing of asteroid paths. All the asteroids were found manually, the majority by "blinking" consecutive exposures to capture apparent asteroid motion. Astronomers found a unique asteroid for every 10 to 20 hours of exposure time. These asteroid trails should not be confused with the mysterious-looking arcs of blue light that are actually distorted images of distant galaxies behind the cluster. Many of these far-flung galaxies are too faint for Hubble to see directly. Instead, in a dramatic example of "gravitational lensing," the cluster functions as a natural telescope, warping space and affecting light traveling through the cluster toward Earth. The Frontier Fields program is a collaboration among several space telescopes and ground-based observatories to study six massive galaxy clusters and their effects. Using a different camera, pointing in a slightly different direction, Hubble photographed six so-called "parallel fields" at the same time it photographed the massive galaxy clusters. This maximised Hubble's observational efficiency in doing deep space exposures. These parallel fields are similar in depth to the famous Hubble Deep Field, and include galaxies about four-billion times fainter than can be seen by the human eye. This image was assembled from several exposures taken in visible and infrared light. The field's position on the sky is near the ecliptic, the plane of our Solar System. This is the zone in which most asteroids reside, which is why Hubble astronomers saw so many crossings. Hubble deep-sky observations taken along a line-of-sight near the plane of our Solar System commonly record asteroid trails. Links: NASA Press Release Abell 370 Parallel Field with Asteroids Asteroids in Frontier Fields - Abell 370 Parallel (video) Asteroids in Frontier Fields - Galaxy Cluster 370 (video)

Provider: Hubble Space Telescope | ESA

Image Source: https://www.spacetelescope.org/images/opo1733b/

Curator: ESA/Hubble, Garching bei München, Germany

Image Use Policy: Creative Commons Attribution 4.0 International License

Image Details Image Details

Image Type
Observation
Object Name
Abell 370
Subject - Solar System
Interplanetary Body > Asteroid
Galaxy
Esahubble_opo1733b_128
 

Position Details Position Details

Position (ICRS)
RA = 2h 39m 54.3s
DEC = -1° 34’ 58.5”
Orientation
North is 27.9° CW
Field of View
2.1 x 2.3 arcminutes
Constellation
Cetus

Color Mapping Details Color Mapping

  Telescope Spectral Band Wavelength
Red Hubble (WFC3) Infrared (H) 1.6 µm
Red Hubble (WFC3) Infrared (J/H) 1.4 µm
Red Hubble (WFC3) Infrared (J) 1.3 µm
Green Hubble (WFC3) Infrared (Z) 1.1 µm
Green Hubble (ACS) Optical (I) 814.0 nm
Blue Hubble (ACS) Optical (V) 606.0 nm
Blue Hubble (ACS) Optical (B) 435.0 nm
Spectrum_base
Red
Red
Red
Green
Green
Blue
Blue
Esahubble_opo1733b_1280
×
ID
opo1733b
Subject Category
A.2.3   D.5  
Subject Name
Abell 370
Credits
NASA, ESA, and B. Sunnquist and J. Mack (STScI) Acknowledgment: NASA, ESA, and J. Lotz (STScI) and the HFF Team
Release Date
2017-11-06T11:20:07
Lightyears
Redshift
Reference Url
https://www.spacetelescope.org/images/opo1733b/
Type
Observation
Image Quality
Good
Distance Notes
Distance to Abell 370
Facility
Hubble Space Telescope, Hubble Space Telescope, Hubble Space Telescope, Hubble Space Telescope, Hubble Space Telescope, Hubble Space Telescope, Hubble Space Telescope
Instrument
WFC3, WFC3, WFC3, WFC3, ACS, ACS, ACS
Color Assignment
Red, Red, Red, Green, Green, Blue, Blue
Band
Infrared, Infrared, Infrared, Infrared, Optical, Optical, Optical
Bandpass
H, J/H, J, Z, I, V, B
Central Wavelength
1600, 1400, 1250, 1050, 814, 606, 435
Start Time
Integration Time
Dataset ID
Notes
Coordinate Frame
ICRS
Equinox
J2000
Reference Value
39.9762101306, -1.58291092604
Reference Dimension
2081.0, 2317.0
Reference Pixel
550.034867518, 1002.98028312
Scale
-1.66756e-05, 1.66756e-05
Rotation
-27.91791169821
Coordinate System Projection:
TAN
Quality
Full
FITS Header
Notes
Creator (Curator)
ESA/Hubble
URL
http://www.spacetelescope.org
Name
Space Telescope Science Institute Office of Public Outreach
Email
outreach@stsci.edu
Telephone
410-338-4444
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
ESA/Hubble
Publisher ID
esahubble
Resource ID
opo1733b
Metadata Date
2017-11-01T12:59:17-04:00
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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