In this article, we will explore and analyze in detail the topic of 2018 CL, which has been the subject of interest and research over the years. 2018 CL is a topic that has sparked debate in various areas and fields, from science to politics, including culture and society in general. Over the decades, 2018 CL has evolved and taken on new dimensions, prompting continued interest in understanding its implications and consequences. In this sense, it is crucial to critically examine the various perspectives and approaches related to 2018 CL, in order to deepen our understanding and generate a constructive debate around this topic.
| Discovery[1][2] | |
|---|---|
| Discovered by | Zwicky Transient Facility |
| Discovery site | Palomar Obs. |
| Discovery date | 5 February 2018 |
| Designations | |
| 2018 CL | |
| NEO · Aten[1][3] | |
| Orbital characteristics[3] | |
| Epoch 23 March 2018 (JD 2458200.5) | |
| Uncertainty parameter 6 | |
| Observation arc | 2 days |
| Aphelion | 1.0606 AU |
| Perihelion | 0.6484 AU |
| 0.8545 AU | |
| Eccentricity | 0.2412 |
| 0.79 yr (289 days) | |
| 294.91° | |
| 1° 14m 52.08s / day | |
| Inclination | 11.847° |
| 136.30° | |
| 141.70° | |
| Earth MOID | 0.0046 AU (1.8 LD) |
| Physical characteristics | |
| 50 m (160 ft)[2] | |
| 25.5–15 (at closest approach)[2] | |
| 25.525[3] | |
2018 CL is a small asteroid and a near-Earth object of the Aten group, approximately 50 metres (160 feet) in diameter. It was the first confirmed finding, detected on 5 February 2018, announced on 8 February 2018, of the Zwicky Transient Facility project, located at Palomar Observatory, California, in the United States.[2][4]