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Atransit of Deimos across the Sun as seen fromMars occurs whenDeimos passes directly between the Sun and a point on the surface of Mars, obscuring a small part of the Sun's disc for an observer on Mars. During atransit, Deimos can be seen from Mars as a small dark spot rapidly moving across the Sun's face.[1][2]
The event could also be referred to as a partialeclipse of the Sun by Deimos. However, since theangular diameter of Deimos is only about 1/10 of the angular diameter of the Sun as seen from Mars, it is more natural to refer to it as a transit. The angular diameter of Deimos is only 2½ times the angular diameter ofVenus as seen from Earth during atransit of Venus from Earth.
A transit of Deimos from Mars lasts a maximum of about two minutes, due to its relatively rapidorbital period of about 30.3 hours.
Because they orbit Mars in low-inclination equatorial orbits, the shadows ofPhobos or Deimos projected onto the surface of Mars exhibit a seasonal variation in latitude. At any given geographical location on the surface of Mars, there are two intervals in a Martian year when the shadows of Phobos or Deimos are passing through its latitude. During each such interval, no or one transit of Deimos can be seen by observers at that geographical location (compared to about half a dozentransits of Phobos).
The shadow always falls on the "winter hemisphere", except when it crosses the equator during theMarch andSeptember equinoxes. Thus transits of Deimos happen during Martian autumn and winter in the northern hemisphere and the southern hemisphere, roughly symmetrically around thewinter solstice. Close to the equator they happen around the March and September equinoxes; farther from the equator they happen closer to the winter solstice.
Because it orbits relatively close to Mars, Deimos cannot be seen north of 82.7°N or south of 82.7°S; such latitudes will obviously not see transits either.
On 4 March 2004, a transit was photographed by Mars RoverOpportunity, while on 13 March 2004, a transit was photographed by Mars RoverSpirit. In the captions below, the first row shows Earth timeUTC and the second row showsMartian local solar time.
 |  |  |  |
| 03:03:43 10:28:17 | 03:03:53 10:28:27 | 03:04:03 10:28:36 | 03:04:13 10:28:46 |
 |  |  |  |  |  |  |  |
| 00:04:27 13:54:11 | 00:04:37 13:54:20 | 00:04:47 13:54:30 | 00:04:57 13:54:40 | 00:05:07 13:54:50 | 00:05:17 13:54:59 | 00:05:27 13:55:09 | 00:05:37 13:55:19 |
 |  |  |  |  |  |  |  |  |  |  |
| 15:58:19 | 15:58:29 | 15:58:39 | 15:58:49 | 15:58:59 | 15:59:09 | 15:59:19 | 15:59:29 | 15:59:39 | 15:59:49 | 15:59:59 |
The data in the tables below is generated usingJPL Horizons. There is some discrepancy of a minute or two with the times reported for the series of images above. This may be due to imprecision in the ephemeris data used by JPL Horizons; also the JPL Horizons data gives local apparent solar time while the times reported above are probably some form of mean solar time (and therefore some of the discrepancy would be due to the Martian equivalent of theequation of time).
Note: the data below is valid for the original landing sites. To the extent that the rovers have moved around on the surface, the parameters of the transits as actually observed may be slightly different.
Near misses are in italics.
| Transits of Deimos from the MarsSpirit rover landing site | |||||
|---|---|---|---|---|---|
| Duration Earth time (UTC) | Duration (Local Solar time) | Minim. separ. | Deimos ang. diam. | Sun ang. diam. | Sun alt. |
| 24 April 2003 03:05:36 | 10 12 59 | 888.8" | 151.0" | 1296.4" | 58.3° |
| 25 April 2003 (10:22:29 – 10:24:25) | 16 39 46 – 16 41 39 | 248.4" | 139.6" | 1297.8" | 18.5° |
| 13 March 2004 (00:05:06 – 00:06:35) | 13 56 12 – 13 57 39 | 458.6" | 150.6" | 1225.0" | 56.8° |
| 9 March 2005 (15:54:16 – 15:56:14) | 14 49 07 – 14 51 02 | 261.4" | 147.6" | 1294.5" | 44.3° |
| 26 January 2006 05:28:45 | 11 57 05 | 1509.5" | 153.4" | 1227.9" | 74.0° |
| 22 January 2007 21:19:39 | 12 52 10 | 982.8" | 152.6" | 1291.6" | 67.8° |
| 12 December 2007 18:10:49 | 16 26 33 | 850.0" | 140.9" | 1229.2" | 22.3° |
| Transits of Deimos from the MarsOpportunity rover landing site | |||||
|---|---|---|---|---|---|
| Duration Earth time (UTC) | Duration (Local Solar time) | Minim. separ. | Deimos ang. diam. | Sun ang. diam. | Sun alt. |
| 30 May 2003 (00:06:57 – 00:09:04) | 13 28 59 – 13 31 02 | 95.8" | 152.5" | 1306.3" | 67.3° |
| 4 March 2004 (03:03:52 – 03:05:06) | 10 30 14 – 10 31 25 | 550.0" | 152.6" | 1233.6" | 67.6° |
| 5 March 2004 10:21:52 | 16 58 21 | 1041.5" | 138.6" | 1232.3" | 15.4° |
| 17 March 2005 05:28:44 | 11 28 40 | 1041.8" | 154.0" | 1303.0" | 81.6° |
| 18 March 2005 (12:36:42 – 12:38:43) | 17 46 46 – 17 48 43 | 89.6" | 134.3" | 1304.4" | 3.0° |
| 18 January 2006 (15:54:26 – 15:56:21) | 15 08 00 – 15 09 52 | 198.4" | 147.2" | 1235.3" | 42.7° |
| 31 January 2007 18:15:01 | 16 02 28 | 824.8" | 143.2" | 1301.4" | 29.3° |
| 3 December 2007 21:20:36 | 13 11 25 | 739.0" | 153.1" | 1238.0" | 72.1° |
March 5, 2024: NASA released images of transits of the moon Deimos, the moonPhobos and the planetMercury as viewed by thePerseverance rover on the planet Mars.
A transit lightcurve of Deimos was obtained[3] in 2020 using the solar array currents measured by theInSight lander. The light drop was about 0.9% (possibly less than the predicted geometric obstruction of 1% due to light scattering by atmospheric dust outside the shadow). The transit lasted between 116 and 124 seconds.
