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We report spectropolarimetric and broadband polarimetric observations of the near-Earth asteroid 2025 FA22 during its close approach of 18 September 2025 (about two Moon distances). With a diameter estimated between 130 and 290 m, 2025 FA22…

We report new observations of the active asteroid P/2010 A2 taken when it made its closest approach to the Earth (1.06 au in 2017 January) after its first discovery in 2010. Despite a crucial role of the rotational period in clarifying its…

地球与行星天体物理 · 物理学 2017-06-28 Yoonyoung Kim , Masateru Ishiguro , Myung Gyoon Lee

The Solar Probe Plus (SPP) mission will explore the Sun's corona and innermost solar wind starting in 2018. The spacecraft will also come close to a number of Mercury-crossing asteroids with perihelia less than 0.3 AU. At small heliocentric…

地球与行星天体物理 · 物理学 2016-06-22 Steven R. Cranmer

The Large Synoptic Survey Telescope (LSST) will be a ground-based, optical, all-sky, rapid cadence survey project with tremendous potential for discovering and characterizing asteroids. With LSST's large 6.5m diameter primary mirror, a wide…

天体物理仪器与方法 · 物理学 2016-03-16 R. Lynne Jones , Mario Juric , Zeljko Ivezic

The population of near-Earth asteroids (NEAs) shows a large variety of objects in terms of physical and dynamical properties. They are subject to planetary encounters and to strong solar wind and radiation effects. Their study is also…

We present visible spectroscopic observations of a near-earth object (NEO) 2012 DA14. The asteroid 2012 DA14 came close to the surface of the Earth on February 15, 2013 at a distance of 27,700 km. Its estimated diameter is around 45 m. The…

地球与行星天体物理 · 物理学 2015-06-16 Seitaro Urakawa , Mitsugu Fujii , Hidekazu Hanayama , Jun Takahashi , Tsuyoshi Terai , Osamu Oshima

We describe systematic ranging, an orbit determination technique especially suitable to assess the near-term Earth impact hazard posed by newly discovered asteroids. For these late warning cases, the time interval covered by the…

地球与行星天体物理 · 物理学 2015-07-15 D. Farnocchia , S. R. Chesley , M. Micheli

In order to avoid collisions with space debris, the near Earth orbit must be continuously scanned by either ground- or spaced-based facilities. For the low Earth orbit, radar telescopes are the workhorse for this task, especially due to…

天体物理仪器与方法 · 物理学 2015-01-26 Daniel Hampf , Paul Wagner , Wolfgang Riede

We present deep imaging observations of activated asteroid P/2016 G1 (PANSTARRS) using the 10.4m Gran Telescopio Canarias (GTC) from late April to early June 2016. The images are best interpreted as the result of a relatively short-duration…

地球与行星天体物理 · 物理学 2016-08-03 Fernando Moreno , Javier Licandro , Antonio Cabrera-Lavers , Francisco J. Pozuelos

The Euclid Ecliptic Survey was conducted during the calibration phase of the mission, 23-31 December 2023, as a campaign to study Solar System objects. We used data from this survey to analyse more than 23 000 appeareances of 2321 known…

地球与行星天体物理 · 物理学 2026-04-29 B. Y. Irureta-Goyena , B. Altieri , J. -P. Kneib , M. Pöntinen , O. R. Hainaut , M. R. Alarcon , M. Granvik , A. A. Nucita , B. Carry , M. Devogele , M. Mahlke , R. Vavrek , T. Müller , E. Vilenius , C. Snodgrass , R. Kohley , C. Lemon , P. Gómez-Alvarez , G. Verdoes Kleijn , J. Licandro , S. Kruk , L. Conversi , A. Franco , G. Buenadicha , P. Mas-Buitrago , K. Kuijken , S. Andreon , C. Baccigalupi , M. Baldi , A. Balestra , P. Battaglia , A. Biviano , E. Branchini , M. Brescia , S. Camera , V. Capobianco , C. Carbone , J. Carretero , R. Casas , M. Castellano , G. Castignani , S. Cavuoti , K. C. Chambers , A. Cimatti , C. Colodro-Conde , G. Congedo , C. J. Conselice , Y. Copin , F. Courbin , H. M. Courtois , M. Cropper , H. Degaudenzi , G. De Lucia , C. Dolding , H. Dole , F. Dubath , X. Dupac , M. Farina , R. Farinelli , S. Ferriol , M. Frailis , M. Fumana , S. Galeotta , K. George , B. Gillis , C. Giocoli , J. Gracia-Carpio , A. Grazian , F. Grupp , S. V. H. Haugan , H. Hoekstra , W. Holmes , I. M. Hook , F. Hormuth , A. Hornstrup , K. Jahnke , M. Jhabvala , A. Kiessling , B. Kubik , M. Kümmel , M. Kunz , H. Kurki-Suonio , A. M. C. Le Brun , S. Ligori , P. B. Lilje , V. Lindholm , I. Lloro , G. Mainetti , O. Mansutti , O. Marggraf , M. Martinelli , N. Martinet , F. Marulli , R. J. Massey , E. Medinaceli , S. Mei , E. Merlin , G. Meylan , A. Mora , L. Moscardini , R. Nakajima , C. Neissner , S. -M. Niemi , C. Padilla , S. Paltani , F. Pasian , K. Pedersen , W. J. Percival , V. Pettorino , G. Polenta , L. A. Popa , F. Raison , R. Rebolo , A. Renzi , J. Rhodes , G. Riccio , E. Romelli , M. Roncarelli , R. Saglia , Z. Sakr , D. Sapone , M. Schirmer , P. Schneider , A. Secroun , E. Sihvola , P. Simon , C. Sirignano , G. Sirri , L. Stanco , P. Tallada-Crespí , I. Tereno , S. Toft , R. Toledo-Moreo , F. Torradeflot , I. Tutusaus , J. Valiviita , T. Vassallo , Y. Wang , J. Weller , F. M. Zerbi , J. García-Bellido , J. Martín-Fleitas , V. Scottez , G. Helou , D. Scott

Phase curves of asteroids are typically considered to depend solely on the scattering properties of airless particulate surfaces and the size of the object being studied. In this study, we demonstrate the additional dependence of phase…

地球与行星天体物理 · 物理学 2022-04-27 Samuel L. Jackson , Benjamin Rozitis , Lord R. Dover , Simon F. Green , Ulrich C. Kolb , Allison E. Andrews , Stephen C. Lowry

This paper presents synthetic observations of long-lived, coorbiting asteroids of Mercury, Venus, the Earth and Mars. Our sample is constructed by taking the limiting semimajor axes, differential longitudes and inclinations for long-lived…

天体物理学 · 物理学 2009-10-31 N. W. Evans , S. A. Tabachnik

Context. Near-Earth objects (NEOs) on an impact course with Earth can move at high angular speed. Understanding their properties, including rotation state, is crucial for assessing impact risks and mitigation strategies. Traditional…

Asteroid 2009 FD could impact Earth between 2185 and 2196. The long term propagation to the possible impacts and the intervening planetary encounters make 2009 FD one of the most challenging asteroids in terms of hazard assessment. To…

地球与行星天体物理 · 物理学 2015-06-22 F. Spoto , A. Milani , D. Farnocchia , S. R. Chesley , M. Micheli , G. B. Valsecchi , D. Perna , O. Hainaut

Deflecting an asteroid from an Earth impact trajectory requires only small velocity changes, typically of the order of microns per second, if done many years ahead of time. For this, a highly precise method of determining the need,…

空间物理 · 物理学 2008-09-17 Bernhard W. Adams

Accurate measurements of osculating orbital elements are essential in order to understand and model the complex dynamic behavior of Near Earth Asteroids (NEAs). ESA's Gaia mission promises to have great potential in this respect. In this…

地球与行星天体物理 · 物理学 2014-09-19 Siegfried Eggl , Hadrien Devillepoix

At the end of its discovery apparition, the $\sim$60 m near-Earth object 2024 YR4 was associated with a non-zero probability of lunar impact during its 2032 December 22 close approach. While posing no threat to Earth, a lunar impact of this…

We study the time evolution of the impact probability for synthetic but realistic impacting and close approaching asteroids detected in a simulated all-sky survey. We use the impact probability to calculate the impact warning time as the…

地球与行星天体物理 · 物理学 2015-08-26 Peter Vereš , Davide Farnocchia , Robert Jedicke , Federica Spoto

The DART spacecraft is planned to impact the secondary of the binary asteroid (65803) Didymos in 2022, to assess deflection strategies for planetary defense. The impact will create a crater and release asteroidal material, some of which…

地球与行星天体物理 · 物理学 2020-03-05 Paul Wiegert

The Gaia satellite will survey the entire celestial sphere down to 20th magnitude, obtaining astrometry, photometry, and low resolution spectrophotometry on one billion astronomical sources, plus radial velocities for over one hundred…