Estimation of orbit quality

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Kalliope / Linus
22 Kalliope / Linus
Daphne / S2008(41)1

41 Daphne / S2008(41)1

45 Eugenia / Petit-Prince

45 Eugenia / Petit-Prince

45 Eugenia / Petite-Princesse

45 Eugenia / Petite-Princesse

87 Sylvia / Romulus

87 Sylvia / Romulus

87 Sylvia / Remus

87 Sylvia / Remus

93 Minerva / Aegis

93 Minerva / Aegis

93 Minerva / Gorgoneion

93 Minerva / Gorgoneion

107 Camilla / S(2001)107 1

107 Camilla / S(2001)107 1

130 Elektra / S(2003)130 1

130 Elektra / S(2003)130 1

216 Kleopatra / Alexhelios

216 Kleopatra / Alexhelios

216 Kleopatra / Cleoselene

216 Kleopatra / Cleoselene

283 Emma / S(2003)283 1

283 Emma / S(2003)283 1

379 Huenna / S(2003)379 1

379 Huenna / S(2003)379 1

617 Patroclus / Menoetius

617 Patroclus / Menoetius

624 Hektor / S(2006)624 1

624 Hektor / S(2006)624 1

702 Alauda / Pichi Unem

702 Alauda / Pichi_Unem

762 Pulcova / S(2000)762 1

762 Pulcova / S(2000)762 1

3749 Balam / S(2002)3749 1

3749 Balam / S(2002)3749 1

50000 Quaoar / Weywot

50000 Quaoar / Weywot

90482 Orcus / Vanth

Orcus / Vanth

136108 Haumea / Hiiaka

136108 Haumea / Hiiaka

136108 Haumea / Namaka

136108 Haumea / Namaka

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Overview

For each systems we use all orbits inside the 1,2 and 3-σ errors zone to compute them for the date of January 1st 2017. Knowing the orbit direction for the primary at this date, if there are a star occultation for this date, we obtain a limit precision in kilometer.

The aim is to classify, at glance, the quality of prediction found in these pages.