Bright NEO

The below near-earth objects are expected to become brighter than magnitude 14.0 in the coming 12 months. If a NEO is currently brighter than magnitude 14 it will be highlighted in yellow. For more information about one of these near-earth objects, click on its designation.

NEO Today Closest Approach Brightest
designation Hₒ diameter est. magn delta (LD) date delta (LD) magn date magn
(481394) 2006 SF619.9280 - 620 m13.817.0 LD21 Nov 201911.3 LD14.411 Nov 201913.8
(2062) Aten16.81 - 3 km19.3573.0 LD12 Jan 202050.0 LD13.58 Jan 202013.3
(52768) 1998 OR215.82 - 4 km19.2542.2 LD29 Apr 202016.2 LD10.91 May 202010.8
(388945) 2008 TZ320.4220 - 495 m24.5734.8 LD10 May 20207.2 LD14.18 May 202013.8
(85275) 1994 LY16.12 - 4 km21.31274.6 LD24 Aug 202045.0 LD13.621 Aug 202013.6
(1981) Midas15.22 - 5 km20.4952.6 LD10 Sep 202067.9 LD13.915 Sep 202013.7
(159402) 1999 AP1016.12 - 4 km22.11570.7 LD17 Oct 202029.6 LD12.511 Oct 202012.3


The current positions of these NEOs are plotted in the below all-sky chart:





    Terminology:
            
    diameter est.:  Estimated diameter based on Hₒ and an albedo between 0.25 and 0.05 (So sizes may be over-estimated for icy objects)
    delta:          Distance between dwarf planet and earth in AU    
    magn:           Magnitude (brightness) estimate    
    LD:             Lunar distance (~0.0257 AU)
    AU:             Astronomical Unit (mean distance between earth and sun: 149597870.7 km    
    Hₒ:             Absolute magnitude (magnitude from a distance of 1 AU) 
    

Orbital elements provided by the MPC (Minor Planet Center).
UCAC4 star catalog via VizieR as provided by the Strasbourg astronomical Data Center.
Calculations by a modified version of AAPlus, a C# implementation of the AA+ project by PJ Naughter from the algorithms presented in the book "Astronomical Algorithms" by Jean Meeus.