323P/SOHO
From Wikipedia, the free encyclopedia
 Comet 323P SOHO by Hubble Space Telescope in March 2021 | |
| Discovery[1] | |
|---|---|
| Discovered by | SOHO |
| Discovery date | 12 March 2004 |
| Designations | |
| P/1999 X3, P/2004 E2, P/2008 K10, P/2012 Q2 | |
| Orbital characteristics[2] | |
| Epoch | 12 February 2021 |
| Earliest precovery date | 12 December 1999 |
| Aphelion | 5.125 AU |
| Perihelion | 0.039 AU |
| Semi-major axis | 2.582 AU |
| Eccentricity | 0.9848 |
| Orbital period | 4.15 years |
| Inclination | 5.37° |
| 324.23° | |
| Argument of periapsis | 353.17° |
| Last perihelion | 14 March 2025 17 January 2021 |
| Next perihelion | 12 February 2029 (Yoshida) 17 June 2029 (JPL)[3] |
| Earth MOID | 0.022 AU |
| Jupiter MOID | 0.221 AU |
| Physical characteristics[2][4][5] | |
Mean diameter | 172±6 m |
| 0.522 hours | |
| (V–R) = 0.13±0.09 | |
| Comet total magnitude (M1) | 23.6 |
323P/SOHO is a periodic comet with an orbital period of 4.15 years discovered in images obtained by the Solar and Heliospheric Observatory (SOHO). It is considered to be a sungrazing comet due to its perihelion being very close to the Sun.[6] 323P/SOHO has the smallest perihelion of all numbered comets.[7] It should next come to perihelion around Feb–June of 2029.
The comet was first noticed by Rainer Kracht in images obtained on 12 March 2004, getting the name C/2004 E2.[1][8] In 2006 it was published that a very faint comet was visible in SOHO images obtained on 12 December 1999.[9][8] R. Kracht identified these two objects as being the same comet that had been observed by SOHO on 30 May 2008, a link subsequently confirmed by Brian G. Marsden.[8]
In late December 2020, the object was recovered at Subaru showing no cometary features on its way to perihelion. However, in postperihelion observations, it developed a long narrow tail mimicking a disintegrated comet. The ejecta, composed of at least millimeter-sized dust with a power law size distribution index of 3.2 ± 0.2, was impulsively produced shortly after the perihelion passage, during which ≳0.1%–10% of the nucleus mass was shed due to excessive thermal stress and rotational disruption. Two fragments of ~20 m in radius (assuming a geometric albedo of 0.15) were seen in Hubble Space Telescope observations from early March 2021.[4]
Physical characteristics
The comet has a convex shaped nucleus, based on its light curve, with approximate axis ratios of R2/R1 ≈ 0.8 and R3/R1 ≈ 0.7 and an equivalent radius of 86 ± 3 m (assuming a geometric albedo of 0.15).[4] The comet has a rotation period of 0.522 hours, which is the shortest for known comets in the Solar System. The next fastest rotating comet is 322P/SOHO, with a period of 2.8 hours.[4] The spin axis is oriented toward the southern ecliptic hemisphere.[4]
On 13 February 2021, the g − r color turned redder as the aperture radius grew, suggesting that the dust ejecta was redder than the nucleus. However, on March 3, the trend became the opposite, which means that the nucleus was bluer than the dust ejecta. As for the r − i color, no strong spatial variation in the color measurements was noticed, indicative of similar colors between the dust ejecta and the nucleus, which is also consistent with the annular aperture measurements.[4] The change of the color was possibly related to the mass loss around perihelion and intense solar heating.[4]
.png)
