C/2007 W1 (Boattini) is a non-periodic comet discovered on 20 November 2007, by Andrea Boattini at the Mt. Lemmon Survey. At the peak the comet had an apparent magnitude around 5.
Observational history On 3 April 2008, when C/2007 W1 was from the Earth and 1.7AU from the Sun, the coma (expanding tenuous dust atmosphere) of the comet was estimated to be as large as 10 arcminutes. This made the coma roughly in diameter.
On 30 April 2008, Alexandre Amorim reported that the comet was a magnitude 7.3 object as seen in 10 × 50 binoculars. By 8 May 2008, David Seargent noted that it brightened up to magnitude 6.4 in the naked eye. It was located within the constellation Pyxis on 20 May 2008.
Physical characteristics Spectroscopic observations in May 2008 reveal a dust production rate of approximately () mol/sec−1, corresponding to a ratio of HCN relative to water by () %. This is nearly compatible to the HCN ratio measured at Hale–Bopp in 1997. In addition, emissions of OH, , and CN were detected.
The nucleus is estimated to have an effective radius of , with a total mass nearly 4.6 kg.
Orbit On 12 June 2008, the comet passed within about of the Earth. The comet came to perihelion on 24 June 2008 at a distance of .
The comet has an observation arc of 597 days allowing a good estimate of the orbit. Using JPL Horizons, the barycentric orbital elements for epoch 2020-Jan-01 generate a semi-major axis of 1,582 AU, an apoapsis distance of 3,163 AU, and a period of approximately 63,000 years.
A 2022 study calculated that it hats a minimum orbit intersection distance of around and with 55637 Uni and respectively.
Before entering the planetary region, C/2007 W1 had a nearly hyperbolic trajectory, which indicated that it was a dynamically new comet originating from the outer Oort cloud, with a loosely bound chaotic orbit that was easily perturbed by passing stars.
Meteor shower A meteor shower known as the Daytime Craterids has been associated with C/2007 W1, thus becoming the first hyperbolic comet associated with a meteor shower. The meteor shower produced daytime outbursts in 2003 and 2009, with a Zenithal Hourly Rate of over 30 meteors per hour observed with radar.
Notes
References
External links
Reconstructing the Morphology of an Evolving Coronal Mass Ejection (1 June 2008)