Astronomical transit

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2003 Transit of Mercury
2003 Transit of Mercury

The term transit or astronomical transit has three meanings in astronomy:

  • A transit is the astronomical event that occurs when one celestial body appears to move across the face of another celestial body, as seen by an observer at some particular vantage point.
  • A transit occurs when a celestial body crosses the meridian due to the Earth's rotation, about halfway between rising and setting. For instance, the Sun transits the meridian at solar noon. Observation of meridian transits was once very important for timekeeping purposes (see transit instrument).
  • The term star transit is used for the passage of a star through the eyepiece of an telescope. Precise observations of elevation or time are carried out to determine star positions or the local vertical (geographic latitude/longitude).
Star transits in a small telescope (FOV ~2°). Two stars passing the vertical thread
Star transits in a small telescope (FOV ~2°). Two stars passing the vertical thread

The rest of this article refers to the first kind of transit.

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[edit] Definition

The word "transit" refers to cases where the nearer object appears considerably smaller in apparent size than the more distant object. Cases where the nearer object appears larger and completely hides the more distant object are known as occultations. Cases where one object moves into the shadow of another are known as eclipses. Each of these three terms are the visible effects of a syzygy.

One example of a transit involves the motion of a planet between a terrestrial observer and the Sun. This can happen only with inferior planets, namely Mercury and Venus (see transit of Mercury and transit of Venus). However, as seen from outer planets such as Mars, the Earth itself transits the Sun on occasion.

Io transits across Jupiter as seen by Cassini spacecraft
Io transits across Jupiter as seen by Cassini spacecraft
Dione transits Titan, as seen by the Cassini probe; in the background, little Prometheus is occulted by the rings of Saturn
Dione transits Titan, as seen by the Cassini probe; in the background, little Prometheus is occulted by the rings of Saturn

The term can also be used to describe the motion of a satellite across its parent planet, for instance one of the Galilean satellites (Io, Europa, Ganymede, Callisto) across Jupiter, as seen from Earth.

A transit requires three bodies to be lined up in a single line. More rare are cases where four bodies are lined up. The one closest to the present occurred on April 27, 1586, when Mercury transited the Sun as seen from Venus at the same time as a transit of Mercury from Saturn and a transit of Venus from Saturn.

In recent years the discovery of extrasolar planets has excited interest in the possibility of detecting their transits across their own stellar primaries. HD 209458b is the first such transiting planet to be discovered.

[edit] Mutual planetary transits and occultations

In rare cases, one planet can transit in front of another. The next time this will happen (as seen from Earth) will be on November 22, 2065 at about 12:43 UTC, when Venus near superior conjunction (with an angular diameter of 10.6") will transit in front of Jupiter (with an angular diameter of 30.9"); however, this will take place only 8° west of the Sun, and will therefore not be visible to the unaided/unprotected eye. When the nearer object has a larger angular diameter than the farther object, thus covering it completely, the event is not a transit but an occultation. Before transiting Jupiter, Venus will occult Jupiter's moon Ganymede at around 11:24 UTC as seen from some southernmost parts of Earth. Parallax will cause actual observed times to vary by a few minutes, depending on the precise location of the observer.

There are only 18 mutual planetary transits and occultations as seen from Earth between 1700 and 2200. Note the long break of events between 1818 and 2065.

A simulation of Venus transiting Jupiter, as it did on January 3, 1818.
A simulation of Venus transiting Jupiter, as it did on January 3, 1818.

The 1737 event was observed by John Bevis at Greenwich Observatory - it is the only detailed account of a mutual planetary occultation. A transit of Mars across Jupiter on 12 Sep 1170 was observed by the monk Gervase at Canterbury, and by Chinese astronomers.

[edit] Contacts

During a transit there are four "contacts", when the circumference of the small circle (small body disk) touches the circumference of the large circle (large body disk) at a single point. The contacts happen in the following order:

  • First contact: the smaller body is entirely outside the larger body, moving inward
  • Second contact: the smaller body is entirely inside the larger body, moving further inward
  • Third contact: the smaller body is entirely inside the larger body, moving outward
  • Fourth contact: the smaller body is entirely outside the larger body, moving outward

[edit] See also

For transit of planets in front of others, see also occultation.

[edit] External references

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Transit visibility from planets superior to the transiting body
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