Zobrazeno 1 - 10
of 2 101
pro vyhledávání: '"Asteroid belt"'
Autor:
Pitjeva, E. V.1 evp@iaaras.ru, Pitjev, N. P.1,2
Publikováno v:
Astronomy Letters. Aug2018, Vol. 44 Issue 8/9, p554-566. 13p.
Autor:
Snodgrass, Colin1 colin.snodgrass@open.ac.uk, Agarwal, Jessica2, Combi, Michael3, Fitzsimmons, Alan4, Guilbert-Lepoutre, Aurelie5, Hsieh, Henry, Hui, Man-To6, Jehin, Emmanuel7, Kelley, Michael8, Knight, Matthew8, Opitom, Cyrielle9, Orosei, Roberto10, Val-Borro, Miguel11, Yang, Bin9
Publikováno v:
Astronomy & Astrophysics Review. 11/14/2017, Vol. 25 Issue 1, p1-59. 59p.
Autor:
Kazantsev, A.1 ankaz@observ.univ.kiev.ua, Kazantseva, L.1
Publikováno v:
Solar System Research. Nov2017, Vol. 51 Issue 6, p527-534. 8p.
Autor:
Abraham Loeb
Publikováno v:
The Astrophysical Journal Letters, Vol 968, Iss 2, p L27 (2024)
Recently, pulsar timing arrays (PTAs) reported a signal at nanohertz frequencies consistent with a stochastic gravitational-wave background. Here, I show that the Brownian motion of the Sun as a result of its random gravitational interactions with th
Externí odkaz:
https://doaj.org/article/4d61f3d644854af3b3f875b827e6be35
Autor:
van den Berg, Hugo A.
Publikováno v:
Science Progress. Jun2016, Vol. 99 Issue 2, p220-224. 5p.
Autor:
Thomas H. Burbine, Iman Khanani, Deepika Kumawat, Ahlay Hussain, Sydney M. Wallace, M. Darby Dyar
Publikováno v:
The Planetary Science Journal, Vol 5, Iss 9, p 194 (2024)
The most widely used method to spectrally classify asteroids is the Bus–DeMeo taxonomy. To test how well the Bus–DeMeo taxonomy groups asteroids on the basis of their mineralogy, we have classified ∼1500 meteorite spectra using this Bus–DeMeo
Externí odkaz:
https://doaj.org/article/c4cb24bbd4df48fd9f3e209c9da61765
Autor:
Rogerio Deienno, David Nesvorný, Matthew S. Clement, William F. Bottke, André Izidoro, Kevin J. Walsh
Publikováno v:
The Planetary Science Journal, Vol 5, Iss 5, p 110 (2024)
The main asteroid belt (MAB) is known to be primarily composed of objects from two distinct taxonomic classes, generically defined here as S- and C-complex. The former probably originated from the inner solar system (interior to Jupiter’s orbit), w
Externí odkaz:
https://doaj.org/article/f6c86c4e955c4859b0ab19445cfa1654
Publikováno v:
The Planetary Science Journal, Vol 5, Iss 3, p 80 (2024)
Red ( S > 10%/0.1 μ m) spectral slopes are common among Centaurs and trans-Neptunian objects (TNOs) in the outer solar system. Interior to and co-orbital with Jupiter, the red ( S ∼ 10%/0.1 μ m) slopes of D-type main-belt and Jupiter Trojan aster
Externí odkaz:
https://doaj.org/article/55c0f5ddb4b644eba873bde12a557f16