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During its departure from Pluto, New Horizons used its LORRI camera to image a portion of Pluto's southern hemisphere that was in a decades-long seasonal winter darkness, but still very faintly illuminated by sunlight reflected by Charon.…

In 2015, the New Horizons spacecraft flew past Pluto and its moon Charon, providing the first clear look at the surface of Charon. New Horizons images revealed an ancient surface, a large, intricate canyon system, and many fractures, among…

Chapter 17 in High-Luminosity Large Hadron Collider (HL-LHC) : Preliminary Design Report. The Large Hadron Collider (LHC) is one of the largest scientific instruments ever built. Since opening up a new energy frontier for exploration in…

加速器物理 · 物理学 2017-05-29 C. Adorisio , I. Bejar Alonso , J. C. Gascon , T. Otto , S. Roesler

The CuPID CubeSat Observatory was a 6U cubesat launched into low-Earth orbit with a ride-share opportunity in Fall 2021. The mission was supported by NASA's Heliophysics division and motivated scientifically with the objective to image…

空间物理 · 物理学 2023-04-11 Emil A. Atz , Brian M. Walsh , Connor J. O'Brien

Chapter 14 in High-Luminosity Large Hadron Collider (HL-LHC) : Preliminary Design Report. The Large Hadron Collider (LHC) is one of the largest scientific instruments ever built. Since opening up a new energy frontier for exploration in…

加速器物理 · 物理学 2017-05-29 B. Goddard , A. Lechner , J. Uythoven

Chapter 16 in High-Luminosity Large Hadron Collider (HL-LHC) : Preliminary Design Report. The Large Hadron Collider (LHC) is one of the largest scientific instruments ever built. Since opening up a new energy frontier for exploration in…

加速器物理 · 物理学 2017-05-29 M. Lamont , M. Pojer , J. M. Jowett

Recently discovered asteroid 2024 YR$_4$ has an orbital period of almost exactly 4 years, a descending node located almost exactly 1 au from the Sun, with a perihelion slightly less than that. Its combination of semi-major axis and…

地球与行星天体物理 · 物理学 2025-02-27 Adam Hibberd , Thomas Marshall Eubanks

The Lucy Mission accomplishes its science during a series of five flyby encounters with seven Trojan asteroid targets. This mission architecture drives a concept of operations design that maximizes science return, provides redundancy in…

Indian Centre for Space Physics has taken a novel strategy to study low energy cosmic rays and astrophysical X-ray sources which involve very light weight payloads up to about five kilograms on board a single or multiple balloons which are…

天体物理仪器与方法 · 物理学 2017-07-04 Sandip K. Chakrabarti , Ritabrata Sarkar , Debashis Bhowmick , Arnab Bhattacharya

The Solar System Odyssey mission uses modern-day high-precision experimental techniques to test the laws of fundamental physics which determine dynamics in the solar system. It could lead to major discoveries by using demonstrated…

The ANTARES Collaboration is completing the deployment of a 12 lines underwater detector, 2500m deep in the Mediterranean Sea, dedicated to high energy neutrino astronomy. Starting with the first line in 2006, 10 lines were continuously…

天体物理学 · 物理学 2019-08-13 Thierry Pradier

We present two large cosmological N-body simulations, called Horizon Run 2 (HR2) and Horizon Run 3 (HR3), made using 6000^3 = 216 billions and 7210^3 = 374 billion particles, spanning a volume of (7.200 Gpc/h)^3 and (10.815 Gpc/h)^3,…

宇宙学与河外天体物理 · 物理学 2012-01-12 Juhan Kim , Changbom Park , Graziano Rossi , Sang Min Lee , J. Richard Gott

Voyager 3 is a concept mission that sends a space telescope to the interstellar medium in a reasonable amount of time. Voyager 3 would take a direct image of an exoplanet using the solar gravitational lensing at the distance of 550…

The Extreme Universe Space Observatory on a Super Pressure Balloon 1 (EUSO-SPB1) was launched in 2017 April from Wanaka, New Zealand. The plan of this mission of opportunity on a NASA super pressure balloon test flight was to circle the…

天体物理仪器与方法 · 物理学 2024-01-15 EUSO Collaboration , G. Abdellaoui , S. Abe , J. H. Adams. , D. Allard , G. Alonso , L. Anchordoqui , A. Anzalone , E. Arnone , K. Asano , R. Attallah , H. Attoui , M. Ave Pernas , R. Bachmann , S. Bacholle , M. Bagheri , M. Bakiri , J. Baláz , D. Barghini , S. Bartocci , M. Battisti , J. Bayer , B. Beldjilali , T. Belenguer , N. Belkhalfa , R. Bellotti , A. A. Belov , K. Benmessai , M. Bertaina , P. F. Bertone , P. L. Biermann , F. Bisconti , C. Blaksley , N. Blanc , S. Blin-Bondil , P. Bobik , M. Bogomilov , K. Bolmgren , E. Bozzo , S. Briz , A. Bruno , K. S. Caballero , F. Cafagna , G. Cambié , D. Campana , J. N. Capdevielle , F. Capel , A. Caramete , L. Caramete , R. Caruso , M. Casolino , C. Cassardo , A. Castellina , O. Catalano , A. Cellino , K. Černý , M. Chikawa , G. Chiritoi , M. J. Christl , R. Colalillo , L. Conti , G. Cotto , H. J. Crawford , R. Cremonini , A. Creusot , A. Cummings , A. de Castro Gónzalez , C. de la Taille , L. del Peral , J. Desiato , A. Diaz Damian , R. Diesing , P. Dinaucourt , A. Djakonow , T. Djemil , A. Ebersoldt , T. Ebisuzaki , J. Eser , F. Fenu , S. Fernández-González , S. Ferrarese , G. Filippatos , W. Finch , C. Fornaro , M. Fouka , A. Franceschi , S. Franchini , C. Fuglesang , T. Fujii , M. Fukushima , P. Galeotti , E. García-Ortega , D. Gardiol , G. K. Garipov , E. Gascón , E. Gazda , J. Genci , A. Golzio , P. Gorodetzky , R. Gregg , A. Green , F. Guarino , C. Guépin , A. Guzmán , Y. Hachisu , A. Haungs , T. Heigbes , J. Hernández Carretero , L. Hulett , D. Ikeda , N. Inoue , S. Inoue , F. Isgrò , Y. Itow , T. Jammer , S. Jeong , J. Jochum , E. Joven , E. G. Judd , A. Jung , F. Kajino , T. Kajino , S. Kalli , I. Kaneko , M. Kasztelan , K. Katahira , K. Kawai , Y. Kawasaki , A. Kedadra , H. Khales , B. A. Khrenov , Jeong-Sook Kim , Soon-Wook Kim , M. Kleifges , P. A. Klimov , I. Kreykenbohm , J. F. Krizmanic , K. Królik , V. Kungel , Y. Kurihara , A. Kusenko , E. Kuznetsov , H. Lahmar , F. Lakhdari , J. Licandro , L. López Campano , F. López Martínez , S. Mackovjak , M. Mahdi , D. Mandát , M. Manfrin , L. Marcelli , J. L. Marcos , W. Marszał , Y. Martín , O. Martinez , K. Mase , M. Mastafa , J. N. Matthews , N. Mebarki , G. Medina-Tanco , A. Menshikov , A. Merino , M. Mese , J. Meseguer , S. S. Meyer , J. Mimouni , H. Miyamoto , Y. Mizumoto , A. Monaco , J. A. Morales de los Ríos , J. M. Nachtman , S. Nagataki , S. Naitamor , T. Napolitano , A. Neronov , K. Nomoto , T. Nonaka , T. Ogawa , S. Ogio , H. Ohmori , A. V. Olinto , Y. Onel , G. Osteria , A. N. Otte , A. Pagliaro , W. Painter , M. I. Panasyuk , B. Panico , E. Parizot , I. H. Park , B. Pastircak , T. Paul , M. Pech , I. Pérez-Grande , F. Perfetto , T. Peter , P. Picozza , S. Pindado , L. W. Piotrowski , S. Piraino , Z. Plebaniak , A. Pollini , E. M. Popescu , R. Prevete , G. Prévôt , H. Prieto , M. Przybylak , G. Puehlhofer , M. Putis , P. Reardon , M. H. Reno , M. Reyes , M. Ricci , M. D. Rodríguez Frías , O. F. Romero Matamala , F. Ronga , M. D. Sabau , G. Saccá , H. Sagawa , Z. Sahnoune , A. Saito , N. Sakaki , H. Salazar , J. L. Sánchez , J. C. Sanchez Balanzar , A. Santangelo , A. Sanz-Andrés , O. A. Saprykin , F. Sarazin , M. Sato , A. Scagliola , T. Schanz , H. Schieler , P. Schovánek , V. Scotti , M. Serra , S. A. Sharakin , H. M. Shimizu , K. Shinozaki , J. F. Soriano , A. Sotgiu , I. Stan , I. Strharský , N. Sugiyama , D. Supanitsky , M. Suzuki , J. Szabelski , N. Tajima , T. Tajima , Y. Takahashi , M. Takeda , Y. Takizawa , M. C. Talai , Y. Tameda , C. Tenzer , S. B. Thomas , O. Tibolla , L. G. Tkachev , T. Tomida , N. Tone , S. Toscano , M. Traïche , Y. Tsunesada , K. Tsuno , S. Turriziani , Y. Uchihori , J. F. Valdés-Galicia , P. Vallania , L. Valore , G. Vankova-Kirilova , T. M. Venters , C. Vigorito , L. Villaseñor , B. Vlcek , P. von Ballmoos , M. Vrabel , S. Wada , J. Watanabe , J. Watts. , R. Weigand Muñoz , A. Weindl , L. Wiencke , M. Wille , J. Wilms , T. Yamamoto , J. Yang , H. Yano , I. V. Yashin , D. Yonetoku , S. Yoshida , R. Young , I. S. Zgura , M. Yu. Zotov , A. Zuccaro Marchi

RT-2 Experiment (RT - Roentgen Telescope) is a low energy gamma-ray instrument which is designed and developed as a part of Indo-Russian collaborative project of CORONAS-PHOTON Mission to study the Solar flares in wide energy band of…

We report on the first extra-solar planet discovered with the brand new HARPS instrument. The planet is a typical 'hot Jupiter' with m2sini = 0.62 MJup and an orbital period of 3.39 days, but from the photometric follow-up of its parent…

Context. During the last 30 years the surface of Pluto has been characterized, and its variability has been monitored, through continuous near-infrared spectroscopic observations. But in the visible range only few data are available. Aims.…

地球与行星天体物理 · 物理学 2016-01-13 V. Lorenzi , N. Pinilla-Alonso , J. Licandro , D. P. Cruikshank , W. M. Grundy , R. P. Binzel , J. P. Emery

The upcoming launch of the James Webb Space Telescope (JWST) in less than three years is certain to bring a revolution in our understanding of many area of astrophysics, with one of the key goals being galaxy evolution. As the first…

天体物理仪器与方法 · 物理学 2015-12-16 Steven L. Finkelstein , James Dunlop , Olivier Le Fevre , Stephen Wilkins

On July 14th 2015, NASA's New Horizons mission gave us an unprecedented detailed view of the Pluto system. The complex compositional diversity of Pluto's encounter hemisphere was revealed by the Ralph/LEISA infrared spectrometer on board of…