Contents

  1. 1. Discovery
  2. 2. Approach
  3. 3. Orbital Period
  4. 4. Composition
  1. 5. Current State
  2. 6. Future Predictions
  3. 7. Video Gallery
Comet Hale-Bopp in April 1997Comet Hale-Bopp in April 1997 / sternwarte.at

One of the most exciting moments in human history was the appearance of the brightest comet in our solar system Hale-Bopp. Many aspects of this comet were both unique as well as the events that surrounded it. Appearing at about the time that the internet was in full swing, Hale-Bopp was the most widely covered and talked about comet in the world.

Discovery

Hale-Bopp was discovered by two different observers independently at the same time, Alan Hale and Thomas Bopp, in 1995. It was located in near Messier 70, a globular cluster, in the Sagittarius constellation. Once both astronomers checked their maps and saw that there were no other comets within that area, they contacted the Central Bureau of Astronomical Telegrams of the comet's coordinates. Research into the comet has revealed that the comet may have been sighted during Pharaoh Pepi I sometime around 2332-2283 BC. Hieroglyph's on Pepi's pyramid point to this theory.

Approach

Hale-Bopp: The Great Comet of 1997Hale-Bopp: The Great Comet of 1997 / nasa.gov

During the time of its discovery, Hale-Bopp was approximately the distance of Jupiter and Saturn from the sun and was at a high magnitude of 10.5. What was unusual is that at this distance, most comets are still very faint but Hale-Bopp's coma was very visible even to amateur telescopes. There was even an image from 1993 when Hale-Bopp was still at a distance where comets were unable to be seen but Hale-Bopp was very much visible.

Hale-Bopp could be seen by the naked eye from Earth in May 1996 and was visible for 18 months before it left the inner solar system. It remained very bright during this time and even developed a second tail as it drew closer to the sun. The first tail, 40 to 45 degrees, had a blue hue and was primarily made of gasses whereas the second tail was more yellow and contained mostly dust.

Orbital Period

Hale-Bopp at perihelion on April 1, 1997Hale-Bopp at perihelion on April 1, 1997 / wikipedia.org

It is believed that it was previously in the inner solar system approximately 4,200 years ago but tidal forces may have sped up its orbit to approximately 2,533 years. Hale-Bopp is anticipated to return to the inner system sometime around 4,385.

Composition

Hale-Bopp had a third tail. This third tail was very faint and was only able to be seen with very powerful equipment. It primarily consisted of sodium and neutral atoms rather than ions and was approximately 50 million km (31 million miles) in length. From observations, it appeared that the sodium derived from the coma of the comet but it has not been determined as to how they were there.

Hubble Sees Material Ejected From Comet Hale-BoppHubble Sees Material Ejected From Comet Hale-Bopp / nasa.gov

A chemical inert and highly volatile, noble gas argon, was also detected on Hale-Bopp but was not seen on other comets. This could aid in helping scientist to determine the different temperature history of a comet's ice. Each of these responds in a different aspect during certain temperature ranges. The presence of this gas has led scientist to believe that Hale-Bopp formed in the Kuiper Belt area and then moved into the Oort Cloud.

Another unusual aspect of Hale-Bopp is it has a satellite. A hypothesis suggested that Hale-Bopp may have a binary nucleus and images were taken by Hubble Space Telescope which confirmed this theory. A binary nucleus is basically two orbiting around one another as if one. Never before has any comet had a stable binary nucleus aspect to them.

Current State

Hale-Bopp is still being imaged by the Herschel Space Observatory and is showing that it is covered in a fresh frost layer. It is believed that the comet will be observable until 2020 and its brightness will diminish to being unseeable at that point.

Future Predictions

Hale-Bopp at a distance of 2 billion km from the SunHale-Bopp at a distance of 2 billion km from the Sun / eso.org

Hale-Bopp is expected to become a sungrazing (extreme close encounter with the sun) comet in time. This is due to it having a high inclination and the effect of the gravitational pull of the planets that it passes along the way. It is estimated at having a 15% chance of this occurring. There is also a possibility that Hale-Bopp may have had a close encounter with Jupiter sometime around 2,215 BC that almost ended in a collision. It is probable that Hale-Bopp's orbit was changed as a result of this.

Although Hale-Bopp had come close to Earth in its passing, it is highly doubtful that it would ever impact with Earth. However, if it were to do so, the impact would be catastrophic as its 60 km (37.3 miles) diameter would decimate the Earth and all its inhabitants.

See also: Comets, Objects