Abell 370 Parallel Field with Asteroids

Esahubble_opo1733a_1024

esahubble_opo1733a May 6th, 2022

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

Some asteroids from within our Solar System have photobombed deep images of the Universe taken by the NASA/ESA Hubble Space Telescope. These asteroids reside, on average, only about 260 million kilometres from Earth — right around the corner in astronomical terms. Yet they've horned their way into this picture of thousands of galaxies scattered across space and time at inconceivably farther distances. This Hubble photo of a random patch of sky is part of the Frontier Fields survey. The colourful image contains thousands of galaxies, including massive yellowish ellipticals and majestic blue spirals. Much smaller, fragmentary blue galaxies are sprinkled throughout the field. The reddest objects are most likely the farthest galaxies, whose light has been stretched into the red part of the spectrum by the expansion of space. Intruding across the picture are asteroid trails that appear as curved or S-shaped streaks. Rather than leaving one long trail, the asteroids appear in multiple Hubble exposures that have been combined into one image. Of the 20 total asteroid sightings for this field, seven are unique objects. Of these seven asteroids, only two were earlier identified. The others were too faint to be seen previously. The 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. 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 picture is of the parallel field for the galaxy cluster Abell 370. It was assembled from images 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 Asteroids in Hubble Frontier Field Abell 370 Asteroids in Frontier Fields - Abell 370 Parallel (video) Asteroids in Frontier Fields - Galaxy Cluster 370 (video)

Provider: Hubble Space Telescope | ESA

Image Source: https://esahubble.org/images/opo1733a/

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
Abell 370
Subject - Solar System
Interplanetary Body > Asteroid
Galaxy
Esahubble_opo1733a_128
 

Position Details Position Details

Position (ICRS)
RA = 2h 40m 13.4s
DEC = -1° 37’ 32.8”
Orientation
North is 27.9° CW
Field of View
1.0 x 1.2 arcminutes
Constellation
Cetus

Color Mapping Details Color Mapping

  Telescope Spectral Band Wavelength
Blue Hubble (ACS) Optical (B) 435.0 nm
Blue Hubble (ACS) Optical (V) 606.0 nm
Green Hubble (ACS) Optical (I) 814.0 nm
Red Hubble (WFC3) Infrared (H) 1.6 µm
Green Hubble (WFC3) Infrared (Z) 1.1 µm
Red Hubble (WFC3) Infrared (J) 1.3 µm
Red Hubble (WFC3) Infrared (J/H) 1.4 µm
Spectrum_base
Blue
Blue
Green
Red
Green
Red
Red
Esahubble_opo1733a_1280
×
ID
opo1733a
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
2022-05-06T09:00:00
Lightyears
Redshift
Reference Url
https://esahubble.org/images/opo1733a/
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
ACS, ACS, ACS, WFC3, WFC3, WFC3, WFC3
Color Assignment
Blue, Blue, Green, Red, Green, Red, Red
Band
Optical, Optical, Optical, Infrared, Infrared, Infrared, Infrared
Bandpass
B, V, I, H, Z, J, J/H
Central Wavelength
435, 606, 814, 1600, 1050, 1250, 1400
Start Time
Integration Time
Dataset ID
Notes
Coordinate Frame
ICRS
Equinox
J2000
Reference Value
40.0558333, -1.6257778
Reference Dimension
2146.0, 2400.0
Reference Pixel
2249.76952078, -2550.46640712
Scale
-8.04978e-06, 8.04978e-06
Rotation
-27.93500490491
Coordinate System Projection:
TAN
Quality
Full
FITS Header
Notes
Creator (Curator)
ESA/Hubble
URL
https://esahubble.org
Name
Space Telescope Science Institute Office of Public Outreach
Email
outreach@stsci.edu
Telephone
410-338-4444
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
opo1733a
Metadata Date
2017-11-01T12:59:16-04:00
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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