This artist’s concept depicts a Trans-Neptunian
Object, a small, faint, icy body orbiting the Sun beyond the orbit of Neptune.
These objects are so small that even with NASA’s Hubble and Webb space
telescopes, they appear only as tiny points of light.
Artwork: NASA, ESA, Leah Hustak (STScI)
For the first time,
scientists used the joint power of NASA’s Hubble and James Webb Space Telescopes to study some of
the most far-flung bodies in our solar system, Trans-Neptunian Objects (TNOs).
Some of these are the smallest and faintest ever directly seen. The researchers
unexpectedly found fewer small TNOs than they expected, and that the colors of
these bodies followed the same relationships as their larger family members.
These objects are typically small,
faint, icy bodies orbiting the Sun beyond the orbit of Neptune. Most are more than 100 million times dimmer than objects visible to
the unaided eye. In two complementary papers published Tuesday in The
Astronomical Journal, teams analyzed the color, composition, and size
distribution of 27 newly discovered tiny, dim TNOs.
This class of small bodies offers the
best view into an early stage of planet-building, when a disk of dust and
pebbles in orbit around the Sun coalesced into city-sized “planetesimals” — the
solid building blocks that clump together to form planets — but had not yet
merged into full-sized worlds. Beyond Neptune, this second stage never
happened, leaving behind a frozen population of planetesimals.
In the deepest TNO survey to date, teams
led by PhD candidates from the University of Victoria in Canada, under the
guidance of the National Research Council of Canada, and Northern Arizona
University in Flagstaff examined a patch of sky simultaneously with Hubble,
observing the TNOs’ visible light, and Webb, observing their infrared light.
The team of researchers measured the objects' colors, which are like a
fingerprint of the surface composition, as well as their sizes and determined
their orbits.
In the coordinated observations, the teams studied two different types of TNOs. The first, dynamically “cold” TNOs, are on their original, relatively circular orbits around the Sun in the plane of the solar system. The second type, dynamically “hot” TNOs, formed between the current locations of Uranus and Neptune but were pushed outward where they are today when the outer gas giants migrated early in the solar system’s history. Today they reside in highly elliptical orbits and move in and out of the plane of our solar system.
NASA's Goddard Space Flight Center; Lead Producer: Paul Morris
Prior to these
observations, astronomers thought that small TNOs from both hot and cold
populations would have undergone many collisions, changing their surfaces
compared to larger TNOs. But that's not what the observations showed. Instead,
the small bodies look like their larger counterparts. This implies that
collisions are not changing the surfaces significantly—perhaps because there
are fewer collisions than expected, or because the TNOs somehow retain their
primordial, pre-collision compositions. The teams are still trying to unravel
this mystery.
“You could imagine a scenario where
getting knocked around and fragmented would change the surface composition, and
then you would see a different surface color for tiny TNOs compared to their
larger siblings. So it's really fascinating to see that the smallest objects
are somehow 'remembering' and preserving the history of how they were made,”
said Northern Arizona University PhD candidate Anastasia Morgan, who led the study of color and composition.
“These dynamically ‘hot’ TNOs retain a
signature of where they were born, even though they’ve been orbitally scrambled
since then,” said co-author David Trilling of Northern Arizona University.
Both the “hot” and “cold” populations
seem to keep the same colors as when they were formed, with little change since
the birth of the solar system.
The Webb data also allowed researchers
to measure the number of objects of each size. They found that the overall size
distributions for both populations were surprisingly similar.
“It's very interesting that the process
of planetesimal formation ends up producing the same distribution of sizes for
both cold and hot populations, despite forming in different regions of the
early solar system. The process seems to be insensitive to disk conditions,
producing similar planetesimal sizes whether the disk is hot or cold, and dense
or fluffy,” said University of Victoria PhD candidate Marielle Eduardo, who led
the study on size distribution.
Researchers also found fewer of these
very small bodies than they expected based on some planet formation models.
Webb discovered 27 new, remarkably dim TNOs, one so faint it is equivalent to
standing on Earth and seeing a small swarm of fireflies on the Moon. The
smallest one they observed has a diameter of about 3 miles (5 kilometers),
which is about five times smaller than what is possible to detect with the most
sensitive ground-based telescopes.
This project would not have been
possible without Hubble and Webb working together to detect and characterize
these TNOs. With Hubble’s sensitivity in visible light and Webb’s in infrared,
the space telescopes provide more insights than either can on its own.
The Hubble Space Telescope has been operating for over three decades and continues to make ground-breaking discoveries that shape our fundamental understanding of the universe. Hubble is a project of international cooperation between NASA and ESA (European Space Agency). NASA’s Goddard Space Flight Center in Greenbelt, Maryland, manages the telescope and mission operations. Lockheed Martin Space, based in Denver, also supports mission operations at Goddard. The Space Telescope Science Institute in Baltimore, which is operated by the Association of Universities for Research in Astronomy, conducts Hubble science operations for NASA.
Source: NASA’s Hubble, Webb Find Far-out Solar System Objects ‘Remember’ Past - NASA Science

