Zosma Star Facts (Delta Leonis)
By : John Whitworth / Updated : Mar 30th, 2026 22:05
Contents
Zosma, also known as Delta Leonis (Bayer) is a main sequence star located in the constellation of Leo, The Lion. Zosma colour is blue - white, although not the hottest stars, they are considerably hotter than our own star which is white.
Zosma temperature range is between 7,500 and 10,000 Kelvin. Based on the spectral type (A4V) as we don't have the exact temperature', we can deduce that the surface temperature of Zosma is in the order of 7,500 and 10,000K based on the notes from Harvard University. To put this in context, the temperature of our Sun is about 5,778 Kelvin as said by Google.
Based on a parallax of 55.82, Zosma distance from Earth can be calculated at being 58.43 light years away or 17.69 parsecs.
Zosma is a naked-eye star, so you don't need a telescope or binoculars when you look up on a clear night. The lower the magnitude, the easier it will be to see it.
Zosma is a major star and forms part of the constellation.
Zosma is one of the brightest stars in the constellation of Leo. It is about 2.2x, or read it another way, twice as big as the Sun. Its name is Arabic for Girdle from where it gets its name from, i.e. its location in the constellation. It is one of the brightest in the night sky compared to the other stars but is not the brightest in Leo, that honour goes to Regulus. As it is travelling through the galaxy at a speed of 26.6km/s relative to the Sun, it will come close to the Sun in about 518,000 years when it will brighten in the night sky but not any where near as the Sun or Moon. 1
Although Zosma is fourth brightest evident by the fact it is Delta, the fourth letter of the Greek constellation, it is brighter than the third star, Algieba which is a double star. Zosma is brighter than both stars but it falls in the pecking order because the sum of the brightness of the two Algieba stars is brighter than Zosma. It is a dying star and is over half way through its dying process. 2
Physical Properties
Zosma Colour and Spectral Type
Zosma spectral type of A4V which means its colour and type is blue - white main sequence star. There is no relationship between colour and size. For example, a red star can be large or small. Small stars are more energy efficient than larger stars and live longer.
Zosma Luminosity
Luminosity is the amount of energy a star pumps out relative to the amount that our star, the Sun, gives out. Our star, the Sun's value is 1. Zosma luminosity figure of 25.61 is based on the value in the Simbad Hipparcos Extended Catalogue at the University of Strasbourg from 2012. The star generates more energy than our star.
Zosma Size (Radius)
Zosma radius has been calculated as being 2.14 times bigger than the Sun. The Sun's radius is 695,800km, therefore, the Zosma radius is an estimated 1,489,012 km. The error range for the radius is between 0.04000 and 0.04000.
Zosma Mass
The Zosma mass is 2.2 times that of our star, the Sun (Solar Masses). The Sun's Mass is 1,989,100,000,000,000,000,000 billion kg. which to calculate using this website is too large. To give idea of size, the Sun is 99.86% the mass of the solar system.
Zosma Lifespan
Using the mass amount above, we can get an idea of the life span of the star using the formula from Georgia State University, we estimate Zosma Lifespan at 1.39 billion years . The more massive a star is, the less efficient it is with its fuel so will live shorter lives than a less massive star.
Zosma Death
We can't be sure when Zosma will die, we can have estimations based on its spectral type and mass. Based on current estimations with Zosma having less than 10 solar masses, Zosma will most likely first start losing its mass in solar winds in a Planetary Nebula phase before the nebula disperses leaving behind a White Dwarf.
Iron Abundance
Zosma Iron Abundance is -0.18 with an error value of 9.99 Fe/H, with the Sun having a value of 1 to put it into context. The value comes from the Hipparcos Extended Catalog.
Zosma Age
Zosma is believed to be about 600 million years old. To put in context, the Sun is believed to be about five billion years old and the Universe is about 13.8 billion years old. The smaller star is, the more efficient it is with its fuel and so will live longer than a star which is very large.
Zosma Location
Zosma location in sky is determined by the right ascension (R.A.) and declination (Dec.). These are equivalent to the Longitude and Latitude on Earth. The Right Ascension (Longitude) is expressed in time (hh:mm:ss) and is how far the star is along Earth's celestial equator. If the R.A. is positive, then it's eastwards and vice versa.
The Declination (Latitude) is how far north or south the object is compared to the celestial equator and is expressed in degrees. If the value is positive, it is north of the celestial equator. For Zosma, the location is 11h 14m 06.41 and +20° 31` 26.5 .
Based on the location of Leo, Zosma can be located in the northern hemisphere of the celestial sky. The celestial hemisphere is equivalent to the hemispheres on Earth. Zosma is on the Ecliptic. The Ecliptic is the path that the Earth takes as it orbits the Sun. As the Earth is titled, we therefore have Celestial and Ecliptic hemispheres and they can be different for a star.
Zosma Magnitude (Apparent / Absolute / Visible)
A number represents a star’s magnitude, whether apparent/visual or absolute. The smaller the number, the brighter the star is. The Sun is the brightest star and therefore has the lowest of all magnitudes, -26.74. A faint star will have a high number.
Zosma apparent magnitude is 2.56, which is a measure of the star's brightness as seen from Earth. Apparent Magnitude is also known as Visual Magnitude.
If you use the 1997 parallax value, Zosma' absolute magnitude is 1.32. If you use the 2007 parallax value, Zosma' absolute magnitude is 1.29. Absolute Magnitude is the star's apparent magnitude from 10 parsecs or 32.6 light years. The magnitude assumes nothing is between the object and the viewer, such as dust clouds. To compare different stars' actual brightness, you would best use Absolute rather than Apparent Magnitude.
Zosma is a naked-eye star, that is one is visible from Earth without needing binoculars or a telescope. The lower the Apparent Magnitude of a star or other object is, the easier it is to see in the night sky. An object with a magnitude greater than 6.5 cannot be seen without a telescope or other device.
Meteor Showers
There are 3 meteor showers that radiate from a location near Zosma during the year.
- Delta Leonids Meteor Shower Feb 15 - Mar 10 (Peak: 25th Feb).
- Northern Delta Leonids Meteor Shower (Peak: 27th Feb).
- Southern Delta Leonids Meteor Shower (Peak: 23th Feb).
Zosma Distance from Earth
Zosma distance from Earth is 57.71 light-years away from Earth or 17.69 parsecs. If you want that in miles, it is about 339,255,470,286,426.133, based on 1 Ly = 5,878,625,373,183.61 miles. The distance is calculated using the parallax from the original Hipparcos data released in 1997 which is 56.52000.
In 2007, Hipparcos data was revised with a new parallax of 55.82000, which puts the Zosma distance from Earth as 58.43 light years or 17.91 parsecs. It should not be taken as though the star is moving closer or further away from Earth. It is purely that the distance was recalculated.
An Astronomical Unit is the distance between Earth and the Sun. The number of A.U. is the number of times that the star is from the Earth compared to the Sun. When you use the 2007 distance, Zosma is roughly 3,694,176.939 Astronomical Units from the Earth/Sun give or take a few.
Zosma Galacto-Centric Distance is 7,405 Parsecs or 24,152.396 Light Years. The Galacto-Centric Distance is the distance from the Zosma to the Centre of the Galaxy which is Sagittarius A*.
How long it will take to get to Zosma
The time it takes to travel to Zosma depends on how fast you are going. U.G. has done some calculations as to how long it will take to go at differing speeds. A note about the calculations, when I'm talking about years, I'm talking about non-leap years only (365 days).
The New Horizons space probe is the fastest one that we've sent into space at the time of writing. Its primary mission was to visit Pluto, which at the time of launch (2006), Pluto was still a planet.
Mach 1 is the speed of sound; Mach 2 is twice the speed. |Before retiring, Concorde was the fastest commercial aeroplane and the only passenger jet that could do Mach 2.
For some small screens, you may need to swipe the table to see the information. If you need an explanation, hover over the bold text. At methods are assuming you have unlimited fuel and travel at a constant speed.
- Walking - 9,796,032,408.118
- Car - 559,773,280.464
- Airbus A380 - 53,239,306.566
- Mach 1 - 51,069,611.352
- Mach 2 - 28,939,534.441
- New Horizons - 1,076,487.078
- Speed of Light - 58.43
Zosma Radial Velocity and Proper Motion
In simplistic terms, all non-rogue stars, like planets, orbit around a central object, although that is actually not true. Where is the centre of the Solar System. For simplicity it's the central star, such as the Sun. In the case of a star, it's the galactic centre. The constellations we see today will be different than they were 50,000 years ago or 50,000 years from now.
Proper motion details the movements of these stars and is measured in milliarcseconds. Zosma is moving -129.88 ± 0.15 milliarcseconds/year towards the north and 143.42 ± 0.25 milliarcseconds/year east if we saw them in the horizon.
The radial velocity, the speed at which the Zosma is towards the Sun, is -20.90000 km/s with an error of about 0.60 km/s . When the value is negative, the star and the Sun are getting closer to one another; likewise, a positive number means that two stars are moving away. It's nothing to fear as the stars are so far apart they won't collide in our lifetime, if ever.
Star Map

Zosma Facts
Any red fact description is not peer reviewed; it is estimated using other pieces of facts, e.g. temperature if in red is based on the colour of the star.
| Primary Name | Zosma |
| Alternative Names | Delta Leonis, Del Leo, Duhr, HD 97603, TYC 1439-2479-1, HIP 54872, HR 4357, 68 Leonis, 68 Leo, BD +21 2298, Gliese 419, 2MASS J11140651-2031258 |
| Spectral Type | A4V |
| Star Type | High proper-motion Star |
| Colour | blue - white |
| Galaxy | Milky Way |
| Constellation | Leo |
| Main Star | Yes |
| Age | 600 million years |
| Absolute Magnitude | 1.32 / / 1.29 |
| Visual / Apparent Magnitude | 2.56 |
| Visible From Earth | Yes |
| Right Ascension (R.A.) | 11h 14m 06.41 |
| Declination (Dec.) | +20° 31` 26.5 |
| Galactic Latitude | 66.82731038 ° |
| Galactic Longitude | 224.22743328 ° |
| 1997 Distance from Earth | 56.52 Parallax (milliarcseconds) |
| 57.71 Light Years | |
| 17.69 Parsecs | |
| 2007 Distance from Earth | 55.82 Parallax (milliarcseconds) |
| 58.43 Light Years | |
| 17.91 Parsecs | |
| 3694176.9385027236 Astronomical Units | |
| Galacto-Centric Distance | 24152.3956232 Light Years / 7405 Parsecs |
| Proper Motion Dec. | -129.88 ± 0.15 milliarcseconds/year |
| Proper Motion RA. | 143.42 ± 0.25 milliarcseconds/year |
| B-V Index | 0.12 |
| Radial Velocity | -20.9 ± 0.6 km/s |
| Iron Abundance (Fe/H) | -0.18 ± 9.99 |
| Eccentricity | 0.2302 |
| Semi-Major Axis | 8718 |
| Luminosity (Lsun) | 25.61 |
| Mass (Solars) | 2.2 |
| Radius | 2.14 (-0.04 / +0.04) |
| Source Date | January 2015 |
| SIMBAD Source | Link |
