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
(66391) 1999 KW4	16.6	1 - 3 km	16.2	40.7 LD	25 May 2019	13.5 LD	12.8	27 May 2019	12.6
(214088) 2004 JN13	15.3	2 - 5 km	17.6	366.9 LD	26 Jul 2019	74.3 LD	14.2	18 Jul 2019	14.0
(66146) 1998 TU3	14.6	3 - 7 km	15.6	611.9 LD	25 Aug 2019	28.8 LD	12.6	31 Aug 2019	11.9
(1620) Geographos	15.6	2 - 5 km	17.5	312.0 LD	31 Aug 2019	53.5 LD	14.2	7 Sep 2019	13.9
(237805) 2002 CF26	17.3	920 - 2060 m	20.2	450.5 LD	5 Sep 2019	39.4 LD	13.8	4 Sep 2019	13.8
(2100) Ra-Shalom	16.1	2 - 4 km	18.8	187.1 LD	21 Sep 2019	69.9 LD	13.4	18 Sep 2019	13.3
(162082) 1998 HL1	18.9	440 - 985 m	19.1	160.9 LD	25 Oct 2019	16.1 LD	12.9	27 Oct 2019	12.4
(481394) 2006 SF6	20.0	265 - 595 m	21.8	293.5 LD	21 Nov 2019	10.3 LD	14.4	15 Nov 2019	13.7
(52768) 1998 OR2	15.9	2 - 4 km	21.5	1570.5 LD	26 Apr 2020	12.8 LD	10.4	28 Apr 2020	10.3

The current positions of these NEO 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 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.