Jupiter |
The Position of Jupiter in the Night Sky:
2025 to 2029
by Martin J. Powell
The path of Jupiter against the background stars of Gemini, Cancer, Leo and Virgo from August 2025 to October 2029, with positions marked on the 1st of each month (click on the thumbnail for the full-size image). Periods when the planet is unobservable (i.e. when it is too close to the Sun, or passes behind it) are indicated by a dashed line; hence the planet becomes lost from view (in the evening sky) in early July 2026 and becomes visible again (in the morning sky) in mid-August of that year. The chart shows the changing shape of a planet's apparent looping formation as it moves through the zodiac: Jupiter describes a zig-zag formation in Gemini in the 2025-26 observing period, followed by a 'hybrid' loop (half loop, half zig-zag) in western Leo in the 2026-27 period, transforming into Northward-facing loops in both 2027-28 and 2028-29.
The star map applies to observers in the Northern hemisphere (i.e. North is up); for the Southern hemisphere view, click here. The faintest stars on the map have an apparent magnitude of about +4.8. Printer-friendly versions of this chart are available for Northern and Southern hemisphere views. Astronomical co-ordinates of Right Ascension (longitude, measured Eastwards in hrs:mins from the First Point of Aries) and Declination (latitude, measured in degrees North or South of the celestial equator) are marked around the border of the chart. Click here to see a 'clean' star map of the area (i.e. without planet path); observers may wish to use the 'clean' star map as an aid to plotting the planet's position on a specific night - in which case, a printable version can be found here. Night sky photographs of the region, together with dates of the planet's passage of the brighter stars, can be seen below.
The three star names shown in yellow-green were officially adopted by the International Astronomical Union (IAU) in 2017 and 2018, derived from Persian, Coptic and Chinese mythology (for more details see the IAU's Working Group on Star Names pages).
Having spent the
entire
2024-25
apparition within
the constellation of Taurus,
the Bull, Jupiter
heads out of view in the dusk twilight in early June of 2025, crossing
into Gemini,
the Twins, soon afterwards. The planet is then unobservable from Earth for several weeks, reaching its most Northerly point of the zodiac (declination
= +23° 16' or +23°.28
in decimal form) in mid-June
and
passing through
superior
conjunction
(positioned behind the Sun
as seen from the Earth) in the third week of that month.
Jupiter
with its moon Ganymede in transit,
imaged by Michael
Wong (Hong Kong, China)
at the planet's opposition
in November 2023 (click on the thumbnail
for a larger version). Ganymede took an hour to complete the transit,
whilst casting its shadow upon the Jovian disk. Wong used a 14-inch (356 mm) Schmidt-Cassegrain
reflector telescope fitted with a planetary camera (Image: Michael
Wong
/ ALPO-Japan)
Jupiter emerges in the dawn sky - rising
shortly before the Sun
- in mid-July 2025, marking the
start of the planet's 2025-26 apparition.
The planet is moving direct (West
to East) at this time, positioned in Western Gemini,
a few degrees South-west of the star Mebsuta (
Gem or Epsilon Geminorum, apparent
magnitude +3.0).
In early August 2025 Jupiter
appears to
form an isosceles triangle with the constellation's brightest stars Castor (
Gem or Alpha Geminorum,
mag. +1.6) and Pollux (
Gem or Beta Geminorum, mag.
+1.1) to its ENE, the long sides of the triangle measuring 13°
(the apparent distance between Castor and
Pollux is 4°.5). In
early September Jupiter makes
a close pass of
the star Wasat
(
Gem
or Delta Geminorum,
mag. +3.5) then in mid-September it crosses
to the North of the ecliptic (the
apparent path of the Sun through
the zodiac, which the Moon and
planets follow closely).
In mid-November the planet reaches
its Eastern stationary point before turning retrograde
(moving East to West) and describing its 2025-26 'zig-zag' pattern against
the stars of Eastern Gemini.
Jupiter reaches opposition (its
closest and brightest orbital position in relation to the Earth for that year)
in the second week of January 2026, positioned several degrees to the South
and SSW of Castor and Pollux
respectively. Moving retrograde, the planet makes another close pass
of
Wasat around mid-January. Now in the evening sky, Jupiter continues its Westward motion and reaches its Western stationary point in mid-March, positioned several
degrees to the South-west and WSW of Castor and Pollux,
respectively (the three forming a near-isosceles triangle). Jupiter
then resumes
direct motion, making a third and final pass of
Wasat at the end of April and
moving into Cancer,
the Crab, in the third week of June. A few days later Castor and Pollux
appear to 'point the way' to Jupiter,
the three celestial bodies forming a line 12°.5 long,
pointing SSE towards the head of Hydra,
the Water Snake, some 19° to the SSE of the planet. As Jupiter
heads towards
central Cancer
in the second week of July the planet becomes lost from view in the dusk twilight,
bringing the 2025-26 apparition to a close.
Jupiter
passes through superior
conjunction in late July 2026, re-appearing in the dawn sky in central Cancer
in
mid-August, heralding the start of its 2026-27 apparition. The planet enters
Leo,
the Lion, in the third week of September, passing to the South of the Sickle
asterism
(star pattern),
at the Western end of the constellation,
in early November. Jupiter
reaches its Eastern stationary
point in mid-December, located within the confines of the Sickle
and 3°.3 to the WNW of
Leo's
brightest star Regulus (
Leo or Alpha Leonis,
mag. +1.4). The planet turns retrograde and heads away from the Sickle in
the third week of January 2027, reaching opposition in mid-February 2027, some
8°.3 to the WNW of Regulus.
Jupiter
describes most of its 2026-27 'hybrid loop' pattern against the stars of Western
Leo,
just to the West of the Sickle;
the remainder of the loop takes place in Cancer,
which the planet re-enters in mid-March. Here it reaches its Western stationary point in
mid-April, positioned only 1° from the constellation's border with Leo.
The planet resumes direct motion and re-enters Leo
in the second week of May, again passing South of the Sickle from
late June to early August whilst passing a short distance North of Regulus in
late July. Soon afterwards Jupiter heads
out of view in the dusk twilight, bringing the 2026-27 apparition to a close.
The planet remains
out of view for the next six weeks, passing through superior conjunction at
the end of August 2027 before emerging into the dawn sky by the third week of
September, at the
start of its 2027-28 apparition. Jupiter begins the apparition in central
Southern Leo,
located just beneath the Lion's belly, but steadily heads ESEwards, entering
Virgo,
the Maiden, in the third week of November. Jupiter reaches
its Eastern stationary point in mid-January 2028, located a short distance North
of the star Zavijava ( Vir or
Beta Virginis, mag. +3.6), at the Western end of the constellation. Part of
the planet's Northward-facing loop is described in Western Virgo
but it is mostly described in South-eastern Leo,
which Jupiter re-enters
whilst moving retrograde in early March. The planet reaches opposition to the
Sun in
mid-March, positioned about 10° South of Leo's
rump and less than 1° West of that constellation's boundary with Virgo.
Moving retrograde, Jupiter
makes a close pass of the star
Leo (Sigma Leonis,
mag. +4.0), at the foot of the Lion's rear leg, in the second week of April,
reaching its Western stationary point in mid-May, a short distance West of that
star. The planet then turns direct, passing close to
Leo again in mid-June and re-entering Virgo in
the third week of July. Jupiter
passes close to Zavijava for
a third time during the second week of August, crossing
to the South of the celestial equator - where the declination
of a celestial body is 0° (
= 0°) - in early September. The
planet becomes
lost from view in the Western sky at dusk soon afterwards, thereby ending the
2027-28 apparition.
Jupiter
passes through superior
conjunction at the end of September 2028, rising in the Eastern sky at dawn
sky by
the third week of October, located near
the star Porrima ( Vir or
Gamma Virginis, mag. +3.5). Moving direct, the planet makes a close pass
of the star
Vir (Theta
Virginis, mag. +4.4) in the third week of November, reaching its Eastern
stationary point in the second week of February 2029, located 4°.7
to the ENE of the constellation's brightest star Spica (
Vir or
Alpha Virginis, mag. +1.0). The planet's open, Northward-facing loop
is described entirely amongst the stars of South-eastern Virgo.
Jupiter
turns retrograde,
reaching opposition in mid-April,
positioned some 4°
North of Spica; it is the planet's most distant and dimmest opposition since 2017.
Continuing its motion to the WNW, the planet makes a second close pass of
Vir in
mid-May, reaching its Western stationary point in mid-June, 1°.2
West of that star. Resuming direct motion towards the ESE, Jupiter passes
close to
Vir for
a third and final time in mid-July, passing to the North of Spica again
in mid-August. The planet ends its 2028-29 apparition during the second
week of October, as it heads into the dusk twilight in South-eastern Virgo.
Jupiter passes through superior conjunction at the end of October 2029, entering Libra, the Balance, on the same day. The planet re-emerges in the morning sky by the third week of November, positioned in the Western half of that constellation.
[Terms in yellow italics are explained in greater detail in an associated article describing planetary movements in the night sky.]
Jupiter in Aries, the Ram photographed by the writer a few days after the planet's opposition in November 2023. In the full-size picture stars are visible down to about magnitude +6.2 (click here for an annotated version and click on the thumbnail for the full-size photo).
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Jupiter Opposition Data, 2026 to 2029
Jupiter reaches opposition to the Sun (when it is closest to the Earth and brightest in the sky for any given apparition) every 398.9 days on average, i.e. about 33½ days later in each successive year. For the period covered by the above star map, oppositions take place on January 10th 2026, February 11th 2027, March 12th 2028 and April 12th 2029. Around opposition, the planet is due South at local midnight in the Northern hemisphere (due North at local midnight in the Southern hemisphere).
Data relating to Jupiter's oppositions from 2026 to 2029 are provided in the table below.
Jupiter opposition data for the period 2026 to 2029 (click on the thumbnail for the full-size table). The Declination is the angle of the planet to the North (+) or South (-) of the celestial equator; on the star chart, it represents the planet's angular distance above or below the blue line. The angular diameter (or apparent size) of the planet as seen from Earth is given in arcseconds (where 1 arcsecond = 1/3600th of a degree).
Jupiter reached a maximum angular diameter at the 2022 opposition, after it passed perihelion - its closest orbital point to the Sun - in early 2023. Since then its angular diameter has reduced slightly at each successive opposition as its distance from Earth has increased. This is reflected in the planet's apparent magnitude, which has faded since its peak at the 2022 opposition and continues to fade over the period, through to its next most distant opposition in April 2029 (the planet passes aphelion - its most distant orbital point from the Sun - in December 2028). The Tilt (the inclination of Jupiter's rotational axis relative to the Earth's orbital plane) is positive (+) when Jupiter's Northern hemisphere is tipped towards the Earth and negative (-) when its Southern hemisphere is tipped towards the Earth; the maximum value it can attain is ±3°.4. The Tilt values were obtained from the SETI Institute's JUICE/Jupiter Ephemeris Generator 3.0. All other data were obtained from 'Redshift' and 'SkyGazer Ephemeris' software. The Jupiter images were obtained from NASA's Solar System Simulator.
Superior conjunction takes place when Jupiter passes behind the Sun as seen from the Earth; the planet is not visible from Earth for about two weeks on either side of this date. At superior conjunction the planet's apparent brightness fades to -1.9 (in 2026) and -1.7 (in 2027, 2028 and 2029) whilst its apparent diameter shrinks to 31".3 (in 2026), 30".8 (in 2027), 30".6 (in 2028) and 30".7 (in 2029).
Jupiter Conjunctions with other Planets,
2025
Viewed from the orbiting Earth, whenever two planets appear to pass each other in the night sky (a line-of-sight effect) the event is known as a planetary conjunction or appulse. Not all planetary conjunctions will be visible from the Earth, however, because many of them take place too close to the Sun. Furthermore, not all of them will be seen from across the world since the observers' latitude will affect the altitude (angle above the horizon) at which the two planets are seen at the time of the event, and the local season will affect the sky brightness at that particular time. A flat, unobstructed horizon will normally be required to observe most of them.
A
conjunction of Jupiter and Mars in
the morning sky in August 2024, photographed by the writer using
a telephoto lens. Note the subtly differing colours of the two planets, also four
of Jupiter's moons.
Conjunctions between
Jupiter and
Venus are
perhaps the most spectacular to view and the most photogenic. A morning conjunction
between these two planets
takes place on August 12th 2025 in central Gemini, the pair
being separated by 0°.8. They contrast
nicely with the much wider (and much dimmer) stellar pair of Castor (
Gem or Alpha Geminorum,
mag. +1.6) and Pollux (
Gem or Beta Geminorum, mag.
+1.1), the brightest stars in the constellation, positioned 12°
to their North-east (Castor and Pollux
themselves
point South-eastwards towards Mercury,
of magnitude
+1.5, which is just beginning a morning apparition). At latitude
50°
North Jupiter
and Venus reach around 25°
high in the East as Jupiter fades
from view in the dawn sky, whilst at 30°
North the pair are around 32°
high, also in the East. At
mid-Southern latitudes the
pair stand around 12°
to 18° high in the North-east when Jupiter disappears
in the twilight. The
pair rise in darkness between latitudes of about 55°
North and 40°
South.
Full details of the only planetary conjunction involving Jupiter during 2025 are provided in the table below.
Jupiter conjunctions with other planets in 2025 (click on thumbnail for full-size table). The column headed 'UT' is the Universal Time (equivalent to GMT) of the conjunction (in hrs : mins). The separation (column 'Sep') is the angular distance between the two planets, measured relative to Jupiter, hence on 2025 Aug 12 Venus is positioned 0°.8 South of Jupiter at the time shown. The 'Favourable Hemisphere' column shows the Hemisphere in which the conjunction is best observed. The expression 'Not high NHem' indicates that observers at latitudes further North than about 45°N will find the conjunction difficult or impossible to observe because of low altitude and/or bright twilight.
To find the direction in which the conjunction is seen, note down the constellation in which the planets are located ('Con' column) and find the constellation's rising direction for your particular latitude in the Rise-Set direction table.
Although any given conjunction takes place at a particular instant in time, it is worth pointing out that, because of the planets' relatively slow daily motions, such events are interesting to observe for several days both before and after the actual conjunction date.
There are in fact two methods of defining a planetary conjunction date: one is measured in Right Ascension (i.e. perpendicular to the celestial equator) and the other is measured along the ecliptic, which is inclined at 23½° to the Earth's equatorial plane (this is due to the tilt of the Earth's axis in space). An animation showing how conjunction dates are determined by each method can be found on the Jupiter-Uranus 2010-11 triple conjunction page. Although conjunctions measured along the ecliptic can be significantly closer, the Right Ascension method is the more commonly used, and it is the one which is adopted here.
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Constellations of the Zodiac: Photographs
Leo, Virgo & Coma Berenices |
Cancer & Northern Hydra |
Gemini, Orion, et al |
Gemini, Cancer, Leo and Virgo Three photographs showing the region of the night sky through which Jupiter passes from 2025 to 2029 (click on the thumbnails for their full-size versions). The regions of the star chart which are covered by each photograph are shown on the overlay chart above; dashed lines indicate that the photograph extends beyond the boundaries of the chart. The faintest stars visible in each photo are approximately as follows: Gemini photo (blue border): magnitude +6.5; Cancer photo (green border): mag. +8.2; Leo/Virgo photo (red border): mag. +7.0. Note that the photographs do not have the same scale because of the varying camera lens settings and image resolutions.
Passage of Bright Stars, 2025 to 2029
As it slowly moves along the 'celestial highway' known as the ecliptic (the apparent path of the Sun through the constellations, which the Moon and planets follow closely) Jupiter passes numerous bright stars; these are listed below, in chronological order:
2025
2026
Jupiter
Rising Photographed
by the writer at dusk in early 2015, when the planet was previously
positioned
in Cancer
(click on the thumbnail
for the full-size picture).
2027
2028
2029
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Jupiter Transit Altitudes, 2025 to 2029
Jupiter is the largest of the Solar System planets and it can show considerable detail even through modest-sized telescopes. A major factor determining the likelihood of seeing a clear telescopic image is the altitude (angle above the horizon) of a planet at the time of observation. For the naked-eye observer, apart from the increased likelihood of obstruction from trees and buildings, a planet's low altitude is generally of little consequence, however for the telescopic observer high altitude is essential in order to minimise the effects of turbulence, atmospheric dimming and light pollution (skyglow) which prevails near the horizon. Consequently, telescopic observers consider high altitude transits (when a celestial body crosses the observer's meridian, reaching its highest point in the sky) as more favourable than low altitude transits. As a general rule, telescopic observation is best done when a celestial body's altitude is greater than about 30°; hence observation in the couple of hours after rising or before setting is best avoided, unless there is no other alternative.
Jupiter's meridian transit altitude (as seen from any given point on Earth) varies from one year to the next in the course of its 11.8-year journey through the zodiac constellations. Its most Northerly point is attained in Gemini (around 23½° North of the celestial equator) then - some six years later - its most Southerly point is attained in Sagittarius (around 23½° South of the celestial equator). In the intervening years, the planet lies somewhere between these two extremes.
The meridian transit altitude at which an observer sees a planet depends not only upon the constellation in which the planet is positioned at the time, but also upon the observer's latitude. As a result, certain apparitions are more favourable to observers in one hemisphere than to observers in the opposite hemisphere, as demonstrated in the table below:
Transit altitudes of Jupiter at successive oppositions from 2025 to 2029, as seen from a variety of latitudes (click on thumbnail for full-size table). The Declination (Dec.) is the angle of the planet to the North (+) or South (-) of the celestial equator at the time of the planet's opposition. The Altitude Range is the approximate altitude variation over the course of the apparition, e.g. for the 2026/27 apparition at latitude 40° North, the transit altitude of Jupiter ranges from (65°.1 - 3°.4) = 61°.7 to (65°.1 + 3°.4) = 68°.5. The table shows that, over the four apparition periods, Jovian transit altitudes improve significantly for Southern hemisphere observers but worsen for Northern hemisphere observers.
What are the best and worst case scenarios regarding Jupiter's transiting altitude? Southern hemisphere observers witnessed their best case scenario (and Northern hemisphere observers witnessed their worst) in the 2019 and 2020 apparitions, when the planet was positioned in Ophiuchus and Sagittarius, respectively (see table on the 2019-21 page). Jupiter then transited at altitudes of around 70° to 80° at mid-Southern latitudes; the next best observing periods here will be in the early 2030s.
Northern hemisphere observers last saw their best case scenario (and Southern hemisphere observers saw their worst) in the 2024-25 observing period, when Jupiter was positioned close to its most Northerly point in Taurus (see table on the 2022-24 page). Observers at mid-Northern latitudes then saw the planet transit at around 70° high in the sky whilst mid-Southern hemisphere observers saw the planet transiting at only 30° high. The next best viewing time for the Northern hemisphere will be in the observing period which immediately follows (2025-26) when Jupiter is close to its most Northerly point in Gemini (see above table). After 2026 the planet's next high-Northerly position will be in Taurus in 2036.
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Moon near Jupiter Dates, 2025
The Moon is easy to find, and on one or two days in each month, it passes Jupiter in the sky. Use the following table to see on which dates the Moon is in the vicinity of the planet:
The Moon moves relatively quickly against the background stars in an Eastward direction, at about its own angular width (0º.5) each hour (about 12º.2 per day). Because it is relatively close to the Earth, an effect called parallax causes it to appear in a slightly different position (against the background stars) when seen from any two locations on the globe at any given instant; the further apart the locations, the greater the Moon's apparent displacement against the background stars. Therefore, for any given date and time listed in the table, the Moon will appear closer to Jupiter when seen from some locations than from others. For this reason, the dates shown in the table should be used only for general guidance.
Jupiter's Four Brightest Moons
Jupiter's four brightest moons (satellites) - namely Ganymede (magnitude +4.6 at opposition), Io (+5.0), Europa (+5.3) and Callisto (+5.6) - can readily be seen through telescopes or steadily-held binoculars. The moons are seen to change their position in relation to each other, along the planet's equatorial plane, from one night to the next. In fact, their motion can be detected in the space of just a few hours.
Jupiter
and its moons imaged
by Jorge Samaniego in August 2021
(click on the thumbnail
for the full-size picture) (Image:
Jorge Samaniego
/ ALPO-Japan).
Because of their low magnification, binoculars may have some difficulty detecting Io since it is the closest of the four moons to the planet; it never lies more than three Jupiter-diameters away. Europa is easier, but Ganymede is the easiest of the four to see. Callisto moves furthest away from the planet but it is also the faintest of the four.
Due to Jupiter's shallow axial tilt (3º.1 to the plane of its orbit), the Jovian moons appear to present a more-or-less linear motion when seen from the Earth. This is in contrast to, say, Saturn with its relatively high axial tilt (26º.7), which causes its moons to mostly follow apparent elliptical paths around the planet when viewed from the Earth (see Saturn's five brightest moons). Approximately every six years, when the Earth passes through Jupiter's equatorial plane, the Jovian moons are seen to become involved in mutual occultations (where the moons pass in front of each other) and mutual eclipses (where a moon's shadow falls upon another moon). Numerous mutual events (or mutual phenomena) took place in the 2021-22 observing period; the next series of events will occur between May 2026 and August 2027.
According to the Italian amateur astronomer Pierpaolo Ricci, a rare sighting of three satellites on the Jovian disk - namely Io, Europa and Callisto - takes place on December 11th 2026 (two months before the planet's opposition) in an 18-minute period between 2235 UT and 2253 UT. It is one of only 17 occasions during the 21st century when three moons can be seen simultaneously transiting the disk.
The positions of Jupiter's four brightest moons can be found using Sky & Telescope's Jupiter Moons facility.
Jupiter |
Credits
Copyright Martin J Powell December 2024