𝔖 Bobbio Scriptorium
✦   LIBER   ✦

The Near-Earth Objects Follow-Up Program

✍ Scribed by P. Pravec; M. Wolf; L. Šarounová; S. Mottola; A. Erickson; G. Hahn; A.W. Harris; A.W. Harris; J.W. Young


Publisher
Elsevier Science
Year
1997
Tongue
English
Weight
381 KB
Volume
130
Category
Article
ISSN
0019-1035

No coin nor oath required. For personal study only.


📜 SIMILAR VOLUMES


The Near-Earth Objects Follow-up Program
✍ Yu.N. Krugly; I.N. Belskaya; V.G. Shevchenko; V.G. Chiorny; F.P. Velichko; S. Mo 📂 Article 📅 2002 🏛 Elsevier Science 🌐 English ⚖ 247 KB

Lightcurve observations of 16 near-Earth objects (NEOs) and 2 Mars-crossers in 1996-1999 from three observational sites are presented. Eight objects were observed shortly after their discovery within the follow-up program of NEO observations. We were able to determine rotation periods for 14 asteroi

The Near-Earth Object Population
✍ Brett Gladman; Patrick Michel; Christiane Froeschlé 📂 Article 📅 2000 🏛 Elsevier Science 🌐 English ⚖ 344 KB

We examine the dynamics of a sample of 117 near-Earth objects (NEOs) over a time scale of 60 Myr. We find that while 10-20% end their lifetimes by striking a terrestrial planet (usually Venus or Earth), more than half end their lives in a Sun-grazing state, and about 15% are ejected from the Solar S

Debiased Orbital and Absolute Magnitude
✍ William F. Bottke Jr.; Alessandro Morbidelli; Robert Jedicke; Jean-Marc Petit; H 📂 Article 📅 2002 🏛 Elsevier Science 🌐 English ⚖ 946 KB

The orbital and absolute magnitude distribution of the near-Earth objects (NEOs) is difficult to compute, partly because only a modest fraction of the entire NEO population has been discovered so far, but also because the known NEOs are biased by complicated observational selection effects. To circu

From Magnitudes to Diameters: The Albedo
✍ A. Morbidelli; R. Jedicke; W.F. Bottke; P. Michel; E.F. Tedesco 📂 Article 📅 2002 🏛 Elsevier Science 🌐 English ⚖ 287 KB

A recently published model of the Near Earth Object (NEO) orbital-magnitude distribution (Bottke et al., 2002, Icarus 156, 399-433.) relies on five intermediate sources for the NEO population: the ν 6 resonance, the 3 : 1 resonance, the outer portion of the main belt (i.e., 2.8-3.5 AU), the Mars-cro