50 recent changes in Main Web retrieved at 12:41 (GMT)

Arecibo
4337 Arecibo occultations on June/July/August 2021 (4337) Arecibo is a main belt asteroid with a diameter estimation of approximately 20 km. Recently, in work s...
Campaigns
Targeted campaigns Apophis March 2021 Didymos April 2021 Arecibo June/July/August 2021 Main.PaoloTanga 26 Feb 2021
Didymos_1
65803 Didymos occultation on April 9, 2021 Didymos is an Earth crossing asteroid target of the NASA/DART and ESA/Hera mission. The April 9th occultation et 22:3...
OccultationAstrometry
Stellar occultations for asteroid astrometry Motivations The high quality astrometry of Gaia offers unique opportunities for solar system science. Apart from t...
Apophis
Targeted campaigns Apophis 2021 99942 Apophis is a Near Earth Asteroid discovered on June 19, 2004, that temporarily reached the highest level of impact risk ...
EditorGroup
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WikiUsers
List of Asteroid observations users Below is a list of users with accounts. If you want to edit topics or see protected areas of the site then you can get added t...
WebHome
Asteroid observations Laboratoire Lagrange Observatoire de la Côte d'Azur * Stellar occultations for asteroid astrometry * Photometry * Shape...
WebLeftBar
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SitePreferences %MAKETEXT{ "Foswiki's default preferences are located in _1 , however settings defined here have override priority and should be used for local ...
WikiGuest
The WikiGuest User A guest of this web, not unlike yourself. You can leave your trace behind you, just add your name in UserRegistration and create your own page....
OccultationScience
Occultation astrometry major goals The power of Gaia based predictions was demonstrated by the successful observation of a MU69/Arrokoth occultation (New Horizo...
GroupViewTemplate
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WikiGroups
Wiki groups dashboard Showing all known groups that can be used to define access controls in Asteroid observations. %TWISTY{ link=" " mode="div" }% ...
Ltypes
The poorly known L type asteroids and the intriguing Barbarians We investigate the poorly known L type asteroids as some of them (known as "Barbarians") are known...
HaythamAli
#x634; #x631; #x643; #x629; #x643; #x634; #x641; #x62A; #x633; #x631; #x628; #x627; #x62A; #x627; #x644; #x645; #x64A; #x627; #x647; #x628; #x627; #x644; #x63...
AdminGroup
How to add the first administrator If you haven't previously set up an administrator, follow these steps: * Note: This help text will disappear once you have ...
TargetList
Observational opportunities until the end of year 2016 for all asteroids with accurate mass estimates (compiled from the literature), and for which shape models h...
StellarOccultations
Stellar occultations, preparing the Gaia era The technique of observation relies upon fast photometry and accurate absolute timing of the observations (by appropr...
ThermalModeling
Thermal modeling The most frequent method to determine the size (and volume) of an asteroid is fitting the thermal data observations (typically from IRAS, WISE, a...
ShapeModeling
Shape determination Orbital parameters are currently known for more than 500 000 asteroids. On the other hand, rotational states and shapes were determined only f...
MethodsPhotometry
Photometry One of the most important sources of information about asteroid physical parameters is photometry typical kilometer sized asteroids (up to diameters ...
ProjectDensities
Densities of asteroids: convex shape models and Gaia masses This project focus on the volume determination by scaling the convex shape models in size. To determin...
Photometry
Densities of asteroids: convex shape models and Gaia masses This project focus on the volume determination by scaling the convex shape models in size. To determin...
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GEARGroup
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Topic revision: r1 - 08 Sep 2009, ProjectContributor
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