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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, 19, 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 October 08

Iris Rise and Set Timetable

TimeElevation
Iris transit07:3164°
Iris set14:07
Moon Rise, 98.7% illuminated16:55-29°
Astrosession begin18:07-37°
Iris rise00:54
Astrosession end03:4334°
Civil sunrise04:4345°
Sunrise05:1150°
Moon Set07:0564°

Track Iris Position Throughout the Night

← Wed, 8 October 2025 →

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 2.561 AU (383,120,147 km) from Earth, and it is located in the constellation Leo.

Current position of Iris in Solar System

Earth Iris
DateWed, 8 October 2025
Distance from Earth to Iris2.559 AU (382,820,951km)
Elongation54°
Angular diameter"
Magnitude10.42
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 coordinates9.4973211533879, 11.736500972197
Center coordinates9.4973211533879, 11.736500972197

Annual motion of Iris

Time
DateWed, 8 October 2025
Twighlight start18:03
Twighlight end03:36
Twighlight duration10h 33m
Rise00:54
Set14:04
Elevation at transit64°
Transit time07:29
Equatorial coordinatesRA: 09h 31m 33s", Dec: 11° 33' 45s
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 Ascension9.4973211533879°
Declination11.736500972197°
Magnitude10.42
ConstellationLeo
Elevation25.6°
Azimuth94.7°

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.