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Dynamical evolution of the early solar system
D Nesvorný - Annual Review of Astronomy and Astrophysics, 2018 - annualreviews.org
Several properties of the Solar System, including the wide radial spacing of the giant
planets, can be explained if planets radially migrated by exchanging orbital energy and …
planets, can be explained if planets radially migrated by exchanging orbital energy and …
Transneptunian space
We provide a nonspecialist overview of the current state of understanding of the structure
and origin of our Solar System's transneptunian region (often called the Kuiper Belt) …
and origin of our Solar System's transneptunian region (often called the Kuiper Belt) …
A Sedna-like body with a perihelion of 80 astronomical units
CA Trujillo, SS Sheppard - Nature, 2014 - nature.com
Abstract The observable Solar System can be divided into three distinct regions: the rocky
terrestrial planets including the asteroids at 0.39 to 4.2 astronomical units (au) from the Sun …
terrestrial planets including the asteroids at 0.39 to 4.2 astronomical units (au) from the Sun …
Science with the 2.5-meter wide field survey telescope (WFST)
Abstract The Wide Field Survey Telescope (WFST) is a dedicated photometric surveying
facility being built jointly by University of Science and Technology of China (USTC) and the …
facility being built jointly by University of Science and Technology of China (USTC) and the …
Tuning the legacy survey of space and time (LSST) observing strategy for solar system science
Abstract The Vera C. Rubin Observatory is expected to start the Legacy Survey of Space and
Time (LSST) in early to mid-2025. This multiband wide-field synoptic survey will transform …
Time (LSST) in early to mid-2025. This multiband wide-field synoptic survey will transform …
The absolute magnitude distribution of Kuiper belt objects
Here we measure the absolute magnitude distributions (H-distribution) of the dynamically
excited and quiescent (hot and cold) Kuiper Belt objects (KBOs), and test if they share the …
excited and quiescent (hot and cold) Kuiper Belt objects (KBOs), and test if they share the …
The evolution of dust disk sizes from a homogeneous analysis of 1–10 Myr old stars
We utilize ALMA archival data to estimate the dust disk size of 152 protoplanetary disks in
Lupus (1–3 Myr), Chamaeleon I (2–3 Myr), and Upper-Sco (5–11 Myr). We combine our …
Lupus (1–3 Myr), Chamaeleon I (2–3 Myr), and Upper-Sco (5–11 Myr). We combine our …
OSSOS. VII. 800+ trans-Neptunian objects—the complete data release
Abstract The Outer Solar System Origins Survey (OSSOS), a wide-field imaging program in
2013–2017 with the Canada–France–Hawaii Telescope, surveyed 155 deg 2 of sky to …
2013–2017 with the Canada–France–Hawaii Telescope, surveyed 155 deg 2 of sky to …
Origin and evolution of the cometary reservoirs
L Dones, R Brasser, N Kaib, H Rickman - Space Science Reviews, 2015 - Springer
Comets have three known reservoirs: the roughly spherical Oort Cloud (for long-period
comets), the flattened Kuiper Belt (for ecliptic comets), and, surprisingly, the asteroid belt (for …
comets), the flattened Kuiper Belt (for ecliptic comets), and, surprisingly, the asteroid belt (for …
A search of the full six years of the Dark Energy Survey for outer solar system objects
We present a search for outer solar system objects in the 6 yr of data from the Dark Energy
Survey (DES). The DES covered a contiguous 5000 deg 2 of the southern sky with≈ 80,000 …
Survey (DES). The DES covered a contiguous 5000 deg 2 of the southern sky with≈ 80,000 …