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The near-earth object camera (NEOCam) is a proposed infrared space mission designed to discover and characterize most of the potentially hazardous asteroids larger than 140 m in diameter that orbit near the Earth. NASA has funded technology…

The Near-Earth Object (NEO) Surveyor mission is a NASA observatory designed to discover and characterize near-Earth asteroids and comets. The mission's primary objective is to find the majority of objects large enough to cause severe…

Assess the joint capabilities of emerging telescopes for near-Earth objects (NEOs) survey and characterization, and what they will add to the current capabilities or replace. NASA telescopes in prime mission, in development, or under study,…

天体物理仪器与方法 · 物理学 2019-07-23 S. N. Milam , H. B. Hammel , J. Bauer , M. Brozovic , T. Grav , B. J. Holler , C. Lisse , A. Mainzer , V. Reddy , M. E. Schwamb , T. Spahr , C. A. Thomas , D. Woods

Increasing our knowledge of the orbits and compositions of Near-Earth Objects (NEOs) is important for a better understanding of the evolution of the Solar System and of life. The detection of serendipitous NEO appearances among the millions…

NASA's Nancy Grace Roman Space Telescope, slated to launch in October 2026, will serve a critical role in the characterization and threat assessment of near-Earth Objects (NEOs), thus contributing to national and international planetary…

The \emph{Wide-field Infrared Survey Explorer} has surveyed the entire sky at four infrared wavelengths with greatly improved sensitivity and spatial resolution compared to its predecessors, the \emph{Infrared Astronomical Satellite} and…

e-ASTROGAM (`enhanced ASTROGAM') is a breakthrough Observatory mission dedicated to the study of the non-thermal Universe in the photon energy range from 0.3 MeV to 3 GeV. The mission is based on an advanced space-proven detector…

The outer solar system provides a unique, quiet vantage point from which to observe the universe around us, where measurements could enable several niche astrophysical science cases that are too difficult to perform near Earth. NASA's New…

NASA's Wide-field Infrared Survey Explorer (WISE) spacecraft has been brought out of hibernation and has resumed surveying the sky at 3.4 and 4.6 um. The scientific objectives of the NEOWISE reactivation mission are to detect, track, and…

The survey of the nearby space and continuous monitoring of the Near Earth Objects (NEOs) and especially Near Earth Asteroids (NEAs) are essential for the future of our planet and should represent a priority for our solar system research…

newASTROGAM is a breakthrough mission concept for the study of the non-thermal Universe from space with gamma rays in the energy range from 15 keV to 3 GeV. It is based on advanced space-proven detector technologies, which will achieve…

天体物理仪器与方法 · 物理学 2025-07-14 D. Berge , M. N. Mazziotta , M. Tavani , V. Tatischeff , U. Oberlack

Near Earth Asteroids (NEAs) and dead comets comprise the vast majority of the population of Near Earth Objects (NEOs) detected to date. Less is known of their physical properties than of the much larger population of main-belt asteroids.…

天体物理仪器与方法 · 物理学 2010-12-14 Mark Trueblood , Larry Lebofsky , Robert Crawford

Ground-based telescopes coupled with adaptive optics (AO) have been playing a leading role in exoplanet direct imaging science and technological development for the past two decades and will continue to have an indispensable role for the…

Near Earth Objects (NEOs) are small Solar System bodies whose orbits bring them close to the Earth's orbit. We are carrying out a Warm Spitzer Cycle 11 Exploration Science program entitled NEOSurvey --- a fast and efficient flux-limited…

e-ASTROGAM (enhanced ASTROGAM) is a breakthrough Observatory space mission, with a detector composed by a Silicon tracker, a calorimeter, and an anticoincidence system, dedicated to the study of the non-thermal Universe in the photon energy…

高能天体物理现象 · 物理学 2018-10-30 A. De Angelis , V. Tatischeff , I. A. Grenier , J. McEnery , M. Mallamaci , M. Tavani , U. Oberlack , L. Hanlon , R. Walter , A. Argan , P. Von Ballmoos , A. Bulgarelli , A. Bykov , M. Hernanz , G. Kanbach , I. Kuvvetli , M. Pearce , A. Zdziarski , J. Conrad , G. Ghisellini , A. Harding , J. Isern , M. Leising , F. Longo , G. Madejski , M. Martinez , M. N. Mazziotta , J. M. Paredes , M. Pohl , R. Rando , M. Razzano , A. Aboudan , M. Ackermann , A. Addazi , M. Ajello , C. Albertus , J. M. Alvarez , G. Ambrosi , S. Anton , L. A. Antonelli , A. Babic , B. Baibussinov , M. Balbo , L. Baldini , S. Balman , C. Bambi , U. Barres de Almeida , J. A. Barrio , R. Bartels , D. Bastieri , W. Bednarek , D. Bernard , E. Bernardini , T. Bernasconi , B. Bertucci , A. Biland , E. Bissaldi , M. Boettcher , V. Bonvicini , V. Bosch Ramon , E. Bottacini , V. Bozhilov , T. Bretz , M. Branchesi , V. Brdar , T. Bringmann , A. Brogna , C. Budtz Jorgensen , G. Busetto , S. Buson , M. Busso , A. Caccianiga , S. Camera , R. Campana , P. Caraveo , M. Cardillo , P. Carlson , S. Celestin , M. Cermeno , A. Chen , C. C Cheung , E. Churazov , S. Ciprini , A. Coc , S. Colafrancesco , A. Coleiro , W. Collmar , P. Coppi , R. Curado da Silva , S. Cutini , F. DAmmando , B. De Lotto , D. de Martino , A. De Rosa , M. Del Santo , L. Delgado , R. Diehl , S. Dietrich , A. D. Dolgov , A. Dominguez , D. Dominis Prester , I. Donnarumma , D. Dorner , M. Doro , M. Dutra , D. Elsaesser , M. Fabrizio , A. FernandezBarral , V. Fioretti , L. Foffano , V. Formato , N. Fornengo , L. Foschini , A. Franceschini , A. Franckowiak , S. Funk , F. Fuschino , D. Gaggero , G. Galanti , F. Gargano , D. Gasparrini , R. Gehrz , P. Giammaria , N. Giglietto , P. Giommi , F. Giordano , M. Giroletti , G. Ghirlanda , N. Godinovic , C. Gouiffes , J. E. Grove , C. Hamadache , D. H. Hartmann , M. Hayashida , A. Hryczuk , P. Jean , T. Johnson , J. Jose , S. Kaufmann , B. Khelifi , J. Kiener , J. Knodlseder , M. Kole , J. Kopp , V. Kozhuharov , C. Labanti , S. Lalkovski , P. Laurent , O. Limousin , M. Linares , E. Lindfors , M. Lindner , J. Liu , S. Lombardi , F. Loparco , R. LopezCoto , M. Lopez Moya , B. Lott , P. Lubrano , D. Malyshev , N. Mankuzhiyil , K. Mannheim , M. J. Marcha , A. Marciano , B. Marcote , M. Mariotti , M. Marisaldi , S. McBreen , S. Mereghetti , A. Merle , R. Mignani , G. Minervini , A. Moiseev , A. Morselli , F. Moura , K. Nakazawa , L. Nava , D. Nieto , M. Orienti , M. Orio , E. Orlando , P. Orleanski , S. Paiano , R. Paoletti , A. Papitto , M. Pasquato , B. Patricelli , M. A. PerezGarcia , M. Persic , G. Piano , A. Pichel , M. Pimenta , C. Pittori , T. Porter , J. Poutanen , E. Prandini , N. Prantzos , N. Produit , S. Profumo , F. S. Queiroz , S. Raino , A. Raklev , M. Regis , I. Reichardt , Y. Rephaeli , J. Rico , W. Rodejohann , G. Rodriguez Fernandez , M. Roncadelli , L. Roso , A. Rovero , R. Ruffini , G. Sala , M. A. SanchezConde , A. Santangelo , P. Saz Parkinson , T. Sbarrato , A. Shearer , R. Shellard , K. Short , T. Siegert , C. Siqueira , P. Spinelli , A. Stamerra , S. Starrfield , A. Strong , I. Strumke , F. Tavecchio , R. Taverna , T. Terzic , D. J. Thompson , O. Tibolla , D. F. Torres , R. Turolla , A. Ulyanov , A. Ursi , A. Vacchi , J. Van den Abeele , G. Vankova Kirilovai , C. Venter , F. Verrecchia , P. Vincent , X. Wang , C. Weniger , X. Wu , G. Zaharijas , L. Zampieri , S. Zane , S. Zimmer , A. Zoglauer , the eASTROGAM collaboration

The Near Earth Object Surveillance Satellite (NEOSSat) is a Canadian-led 15 cm Earth-orbiting telescope originally designed to detect asteroids near the Sun. Its design is however also suitable for the observation of exoplanetary transits…

地球与行星天体物理 · 物理学 2022-09-21 Chris Fox , Paul Wiegert

Large X-ray observatories such as Chandra and XMM-Newton have been delivering scientific breakthroughs in research fields as diverse as our Solar System, the astrophysics of stars, stellar explosions and compact objects, accreting…

The continuing monitoring and surveying of the nearby space to detect Near Earth Objects (NEOs) and Near Earth Asteroids (NEAs) are essential because of the threats that this kind of objects impose on the future of our planet. We need more…

天体物理仪器与方法 · 物理学 2019-01-15 V. Bacu , A. Sabou , T. Stefanut , D. Gorgan , O. Vaduvescu
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