| Minorplanet: | yes |
| 1998 Titius | |
| Background: |
|
| Discovered: | 24 February 1938 |
| Mpc Name: | (1998) Titius |
| Alt Names: | 1966 TF |
| Epoch: | 4 September 2017 (JD 2458000.5) |
| Uncertainty: | 0 |
| Observation Arc: | 79.27 yr (28,955 days) |
| Perihelion: | 2.2643 AU |
| Semimajor: | 2.4196 AU |
| Eccentricity: | 0.0642 |
| Period: | 3.76 yr (1,375 days) |
| Mean Motion: | / day |
| Inclination: | 7.6265° |
| Asc Node: | 351.78° |
| Arg Peri: | 246.70° |
| Dimensions: | 10.79 km km km km |
| Albedo: | 0.20 |
| Abs Magnitude: | 12.1012.2 |
1998 Titius, provisional designation, is a metallic–carbonaceous asteroid from the inner regions of the asteroid belt, approximately 14 kilometers in diameter.
It was discovered on 24 February 1938, by German astronomer Alfred Bohrmann at Heidelberg Observatory in southern Germany. On the same night, the body was also observed at the Finnish Turku Observatory. It was later named after astronomer Johann Daniel Titius.
Titius orbits the Sun in the inner main-belt at a distance of 2.3–2.6 AU once every 3 years and 9 months (1,375 days). Its orbit has an eccentricity of 0.06 and an inclination of 8° with respect to the ecliptic. It stays in a 2:1 orbital resonance with the planet Mars. Titius observation arc starts on the night following its official discovery observation.
According to observations carried out by the Japanese Akari and NASA's Wide-field Infrared Survey Explorer (WISE) with its subsequent NEOWISE mission, Titius has an albedo between 0.093 and 0.126, and its diameter measures between 14.2 and 16.0 kilometers. The Collaborative Asteroid Lightcurve Link assumes a standard albedo of 0.20 and calculates a diameter of 10.8 kilometers with an absolute magnitude of 12.2.
Its spectral classification is that of a Xc-type asteroid in the SMASS taxonomy, a transitional spectral type between the two large main groups of metallic X-type and carbonaceous C-type asteroids. Both types are much darker than the stony S-type asteroids, which are also very common in the inner main-belt. In addition, Titius is also classified as a M-type asteroid by WISE.
A rotational lightcurve of Titius was obtained from photometric observations by American astronomer Robert Stephens at the Californian Santana Observatory in March 2002. Lightcurve analysis gave a rotation period of hours, during which its brightness amplitude varies by magnitude .
This minor planet was named after German astronomer Johann Daniel Titius (1729–1796), best known for formulating the Titius-Bode law, which states that each subsequent planet in the Solar System is roughly twice as far from the Sun than the previous one. He is also honored by the lunar crater Titius. The official was published by the Minor Planet Center on 15 October 1977 .