| Minorplanet: | yes |
| (5496) 1973 NA | |
| Background: |
|
| Discovered: | 4 July 1973 |
| Mpc Name: | (5496) 1973 NA |
| Alt Names: | 1973 NA1992 OA |
| Epoch: | 4 September 2017 (JD 2458000.5) |
| Uncertainty: | 0 |
| Observation Arc: | 41.30 yr (15,086 days) |
| Perihelion: | 0.8865 AU |
| Semimajor: | 2.4351 AU |
| Eccentricity: | 0.6360 |
| Period: | 3.80 yr (1,388 days) |
| Mean Motion: | / day |
| Inclination: | 68.006° |
| Asc Node: | 101.04° |
| Arg Peri: | 118.02° |
| Moid: | 0.0904 AU |
| Mean Diameter: | 1.88 km |
| Albedo: | 0.20 |
| Abs Magnitude: | 16.0 |
(5496) 1973 NA, is a very eccentric and heavily tilted asteroid, classified as near-Earth object of the Apollo group, approximately 2 kilometers in diameter. It was discovered on 4 July 1973, by American astronomer Eleanor Helin at the U.S. Palomar Observatory in California. At the time of its discovery, it was the most highly inclined minor planet known to exist. It may be the parent body of the Quadrantids.
is a possible parent body of the Quadrantids, a major meteor shower that occurs every January. It may also be just a fragment of the parent or the dormant remains of the parent. Other possible parent bodies are and comet 96P/Machholz, as well as .
The asteroid orbits the Sun at a distance of 0.9–4.0 AU once every 3 years and 10 months (1,388 days). Its orbit has an eccentricity of 0.64 and an inclination of 68° with respect to the ecliptic. No precoveries were taken. The asteroid's observation arc even begins 2 days after its discovery.
The body was also one of the first known near-Earth asteroids. Its discovery happened just two days after it had passed 0.07984AU from Earth on one of its closest approaches ever computed. It was then tracked for more than a month, but was not seen again until its next close approach in 1992, when it was recovered by the Siding Spring Observatory in Australia. Its minimum orbit intersection distance with Earth is now 0.0904abbr=onNaNabbr=on.
The stony S-type asteroid is also classified as a transitional C/X-type according to observations by the NASA IRTF telescope. A rotational lightcurve for this asteroid was obtained by American astronomer Brian Skiff from photometric observations made in June 2011. Lightcurve analysis gave a well-defined rotation period of hours with a brightness variation of 0.15 magnitude . The Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 1.88 kilometers with an absolute magnitude of 16.0.