These three photographs taken with NASA's Hubble Space Telescope chronicle a violent outburst in the life of comet LINEAR, also known as C/1999 S4. The orbiting observatory's Space Telescope Imaging Spectrograph tracked the streaking comet for two days, July 5 to 7, capturing a dramatic leap in its brightness [left image]; followed by seeing a wave of newly created dust from the outburst flowing into the coma, a shell of dust surrounding the core [middle image]; and culminating in the discovery of a castoff chunk of material from the nucleus sailing along its tail [the bright dot trailing behind the comet in the picture at right]. The white region represents the brightest part of the coma. The nucleus cannot be seen in these images because it is about a mile or so across, which is too small for the Hubble telescope to see.
When the Hubble telescope snapped these visible-light images, comet LINEAR was 74 million miles (120 million km) from Earth. At 6:32 p.m. EDT July 5 [left image], Hubble watched as the light within a 50-mile-wide region surrounding the core brightened by about 50 percent in less than four hours. By 5:20 p.m. EDT the next day [middle image], that region was a third less luminous than at its peak the previous day, as the dust expelled from the core during the outburst moved farther out in the coma. By 7:04 p.m. EDT on the final day [right image], the comet's brightness was back to normal – about one-seventh less luminous than at peak level.
The chunk of material seen in the final picture is roughly 290 miles (470 km) from the nucleus and appears to be moving down the tail at about 6 miles per hour. The fragment's slow pace indicates that it could be quite large (possibly house-size), but accurate estimates for the sizes of the chunk and of the core require further analyses of the Hubble images and data from other observatories.
Credits
NASA, H. Weaver and P. Feldman (Johns Hopkins University), M. A'Hearn (University of Maryland), C. Arpigny (Liege University), M. Combi (University of Michigan), M. Festou (Observatoire Midi-Pyrenees), and G.-P. Tozzi (Arcetri Observatory)| About The Object | |
|---|---|
| Object Name | Comet LINEAR (Lincoln Laboratory Near-Earth Asteroid Research); C/1999 S4 |
| Object Description | Comet |
| Distance | On July 5, 2000 the comet was at a distance of 74 million miles (120 million km) from Earth. |
| About The Data | |
| Data Description | Principal Astronomers: Comet LINEAR investigation team: H. Weaver and P. Feldman (JHU), M. A'Hearn (Univ. of Maryland), C. Arpigny (Liege Univ.), J. Bauer (Univ. of Hawaii), M. Combi (Univ. of Michigan), J. Davies (Joint Astronomy Centre), M. Festou (Observatoire Midi-Pyrenees), M. Keesey (JPL), P. Lamy (Laboratoire d'Astronomie Spatiale), C. Lisse (STScI), B. Marsden (SAO), K. Meech (Univ. of Hawaii), Z. Sekanina (JPL) , I. Toth (Konkoly Observatory) , G.-P. Tozzi (Arcetri Observatory), D. Yeomans (JPL). |
| Instrument | HST>STIS |
| Exposure Dates | July 5 - 7, 2000 |
| Filters | F28X50LP |
| About The Object | |
|---|---|
| Object Name | A name or catalog number that astronomers use to identify an astronomical object. |
| Object Description | The type of astronomical object. |
| R.A. Position | Right ascension – analogous to longitude – is one component of an object's position. |
| Dec. Position | Declination – analogous to latitude – is one component of an object's position. |
| Constellation | One of 88 recognized regions of the celestial sphere in which the object appears. |
| Distance | The physical distance from Earth to the astronomical object. Distances within our solar system are usually measured in Astronomical Units (AU). Distances between stars are usually measured in light-years. Interstellar distances can also be measured in parsecs. |
| Dimensions | The physical size of the object or the apparent angle it subtends on the sky. |
| About The Data | |
| Data Description |
|
| Instrument | The science instrument used to produce the data. |
| Exposure Dates | The date(s) that the telescope made its observations and the total exposure time. |
| Filters | The camera filters that were used in the science observations. |
| About The Image | |
| Image Credit | The primary individuals and institutions responsible for the content. |
| Publication Date | The date and time the release content became public. |
| Color Info | A brief description of the methods used to convert telescope data into the color image being presented. |
| Orientation | The rotation of the image on the sky with respect to the north pole of the celestial sphere. |
