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Sky-Tonight.com / Asteroids / 7 Iris
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Observation Settings

Or select it on the map:
This Earth map fragment is intended to illustrate celestial motion across the sky, emphasizing both bearing and elevational perspectives. The map's center point corresponds to the transit, showcasing celestial objects at their highest point, while elevation gradually decreases towards the map edges. This dynamic representation offers insights into the changing positions of celestial bodies with a focus on their bearing and elevational trajectories.
Your location: Santa Clara, United States
Timezone:
Latitude:
37.3541
Longitude:
-121.955

Asteroid 7 Iris Observation Details

Iris

Iris Daily Motion


7 Iris will be visible until June, 18, when it will move too close to the Sun. During this time, its proximity to the Sun will cause it to disappear from the night sky, making it unobservable for a while.

Iris Visibility Timetable on January 10

Iris Rise and Set Timetable

TimeElevation
Astrosession begin16:40-37°
Iris rise19:54
Moon Rise, 53.2% illuminated22:1327°
Iris transit01:4951°
Astrosession end03:4942°
Civil sunrise04:5332°
Sunrise05:2327°
Iris set07:43
Moon Set09:26-20°

Track Iris Position Throughout the Night

← Sat, 10 January 2026 →

Elevation (degrees)
Time
Altitude
Azimuth
Shift the map to change the time and observe Iris changing position in the night sky.

Iris Description

Iris, designated as 7 Iris, is a main-belt asteroid, located between Mars and Jupiter in the solar system. With a diameter of 200 km, 7 Iris completes its orbit around the Sun in 3.7 years. At the moment, 7 Iris is 1.697 AU (253,867,587 km) from Earth, and it is located in the constellation Leo.

Current position of Iris in Solar System

Earth Iris
DateSat, 10 January 2026
Distance from Earth to Iris1.697 AU (253,867,587km)
Elongation122°
Angular diameter"
Magnitude9.71
This section provides an interactive projection of the solar system, illustrating the relative positions of Iris, Earth, and the Sun throughout the year. By sliding the image left or right, you can change the day of the year, observing how the positions of Iris and Earth shift in their orbits around the Sun.

Finder Chart for Iris

Double-click to unlock the map.
Object name7 Iris
Field of view
Limiting magnitude
7 Iris coordinates11.027032634674, -1.4708802473673
Center coordinates11.027032634674, -1.4708802473673

Annual motion of Iris

Time
DateSun, 11 January 2026
Twighlight start16:41
Twighlight end03:47
Twighlight duration11h 6m
Rise19:50
Set07:39
Elevation at transit51°
Transit time01:45
Equatorial coordinatesRA: 11h 01m 31s", Dec: -1° 31' 18s
Magnitude10
ConstellationLeo
The graph illustrates the annual visibility pattern of a Iris, providing a comprehensive overview of its daily appearances and transit times throughout the year.
The graph is structured with the vertical axis showing the hours of the day, ranging from 12 AM to 12 AM the next day, while the horizontal axis spans each day of the year.
The reddish shaded area indicates the periods when the Iris is above the horizon, visible to observers. The white line marks the times when the celestial object reaches its highest point in the sky each day, known as the transit.

Astrometric & Physical Parameters of 7 Iris

Coordinates & Visibility

Right Ascension11.027032634674°
Declination-1.4708802473673°
Magnitude9.71
ConstellationLeo
Elevation-43.8°
Azimuth-46.7°

Physical properties

Mean radius in kilometres100
Boby mass in kg8.4E+18
Body density in g.cm31

Orbital Parameters

Sideral orbital time for body around another one (the Sun or a planet) in earth day1346.628

Data Acknowledgment

Our solar system data—including planetary physical and orbital parameters—comes from the Solar System OpenData API , maintained by Le Système Solaire. We thank Christophe and the contributors for making this open data available.

Acknowledgments

We acknowledge NASA's Jet Propulsion Laboratory (JPL) for providing essential data on asteroids and comets through their Small-Body Database (SBDB) and Center for Near-Earth Object Studies (CNEOS). Their continuous efforts in tracking and cataloging these celestial bodies make it possible to offer accurate and up-to-date information on their positions, orbits, and physical characteristics.