Color, composition, and thermal environment of Kuiper Belt object (486958) Arrokoth
Earth and Planetary Astrophysics (astro-ph.EP)
CH3OH
550
[SDU.ASTR.EP]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP]
500
[SDU.ASTR.EP] Sciences of the Universe [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP]
surface composition
FOS: Physical sciences
New Horizons spacecraft
01 natural sciences
520
630
color
Kuiper belt
ices
13. Climate action
Arrokoth
0103 physical sciences
2014 MU69
methanol
Astrophysics - Earth and Planetary Astrophysics
DOI:
10.1126/science.aay3705
Publication Date:
2020-02-14T00:05:29Z
AUTHORS (49)
ABSTRACT
Examining Arrokoth
The New Horizons spacecraft flew past the Kuiper Belt object (486958) Arrokoth (also known as 2014 MU
69
) in January 2019. Because of the great distance to the outer Solar System and limited bandwidth, it will take until late 2020 to downlink all the spacecraft's observations back to Earth. Three papers in this issue analyze recently downlinked data, including the highest-resolution images taken during the encounter (see the Perspective by Jewitt). Spencer
et al.
examined Arrokoth's geology and geophysics using stereo imaging, dated the surface using impact craters, and produced a geomorphological map. Grundy
et al.
investigated the composition of the surface using color imaging and spectroscopic data and assessed Arrokoth's thermal emission using microwave radiometry. McKinnon
et al.
used simulations to determine how Arrokoth formed: Two gravitationally bound objects gently spiraled together during the formation of the Solar System. Together, these papers determine the age, composition, and formation process of the most pristine object yet visited by a spacecraft.
Science
, this issue p.
eaay3999
, p.
eaay3705
, p.
eaay6620
; see also p.
980
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