Results 21 to 30 of about 4,911 (246)
ATLAS Photometry of Interstellar Object 3I/ATLAS
We present calibrated Asteroid Terrestrial-impact Last Alert System (ATLAS) photometry of the interstellar comet 3I/ATLAS (C/2025 N1) from March 28 through 2025 August 29, obtained with the five-site, robotic ATLAS network in the c (420–650 nm), o (560 ...
John L. Tonry +9 more
doaj +4 more sources
Interstellar dust within the life cycle of the interstellar medium [PDF]
Cosmic dust is omnipresent in the Universe. Its presence influences the evolution of the astronomical objects which in turn modify its physical and chemical properties.
Demyk K.
doaj +2 more sources
Interstellar objects in a galactic context [PDF]
Interstellar objects (ISOs) form a vast Galaxy-spanning population with an number density ∼ 1015 pc−3 in the Solar neighbourhood. Though only two members of this population have been observed, 1I/‘Oumuamua and 2I/Borisov, the Vera C. Rubin’s Legacy Survey of Space and Time (LSST) which begins later this year is expected to increase our sample of known ...
Hopkins, Matthew
openaire +3 more sources
He Awa Whiria: The Tidal Streams of Interstellar Objects [PDF]
Upcoming surveys are likely to discover a new sample of interstellar objects (ISOs) within the solar system, but questions remain about the origin and distribution of this population within the Galaxy.
John C. Forbes +7 more
doaj +3 more sources
Strength Ratios of Diffuse Interstellar Bands in Slightly Reddened Objects [PDF]
The disk of the Milky Way fills the interstellar medium in the form of discrete clouds, many (∼30) light-years across. The average density of this medium is 1 hydrogen atom per cm3 (Oort limit), in the clouds—several dozen atoms, and between the clouds ...
Jacek Krełowski, Arkadii Bondar
doaj +2 more sources
Identifying Interstellar Object Impact Craters
Abstract The discoveries of two interstellar objects (ISOs) in recent years have generated significant interest in constraining their physical properties and the mechanisms behind their formation. However, their ephemeral passages through our solar system permitted only incomplete characterization.
Samuel H. C. Cabot, Gregory Laughlin
openalex +3 more sources
Predicting Interstellar Object Chemodynamics with Gaia
The interstellar object (ISO) population of the Milky Way is a product of its stars. However, what is in fact a complex structure in the solar neighborhood has traditionally in ISO studies been described as smoothly distributed.
Matthew J. Hopkins +2 more
doaj +3 more sources
Interstellar Object Accessibility and Mission Design
IEEE Aerospace Conference, Preprint Version, Accepted: November ...
Donitz, Benjamin P. S. +8 more
openaire +3 more sources
Candidate Captured Interstellar Objects in the Solar System [PDF]
Interstellar objects (ISOs) can become gravitationally bound to the solar system, enabling multiple observations. If these bound ISOs exist, they provide valuable opportunities to generalize models of planetesimal formation, composition, and ejection beyond our solar system.
Rainer Marquardt-Demen +2 more
openalex +3 more sources
Radio seti observations of the interstellar object 'oumuamua [PDF]
10 pages, 5 figures, submitted to Astrophysical ...
G. R. Harp
openalex +4 more sources

