Lepus Constellation: The Ultimate Guide
Lepus (The hare)
Lepus is one of the brightest and most prominent constellations. The name of the constellation provides from Latin and means hare.
The location of the constellation Lepus is essentially in the southern hemisphere. Still, it is possible to visualize it in all northern hemisphere countries, and we can find it in the night sky throughout the winter.
The constellation Lepus is small and adjacent to the constellation Canis Major.
The brightest star in the constellation Lepus is Arneb (α Leporis / α Lep / 11 Leporis), with an apparent magnitude of +2.58.
The constellation Lepus is home to profuse sky objects such as galaxies, nebulae, and star clusters.
There is no record of meteor shower sightings within the boundaries of the constellation Lepus.
The Mythology And History Of The Lepus Constellation
Ancient Inca
In the ancient culture of the Inca empire, the constellation Lepus appears as part of the constellation of what we know today as "Orion."
It is thought that Lepus was associated with the figure of a mountain rabbit in this culture. As Lepus is near the equator, explorers might have used it to avoid getting lost in the mountains.
Greek Mythology
In Greek mythology, there is a myth associated with the constellation; according to the writer Hyginus, it was a hare that fled from Orion's dog and was so fast that it was impossible to catch.
The astronomer Eratosthenes added that the Olympian god Hermes put Lepus among the constellations because of his incredible speed as an example of a small but unattainable creature and symbol of speed.
Early Modern Period
During the nineteenth century, Lepus was designated as one of the 88 official night sky constellations by the International Astronomical Union. The boundaries between this constellation and the belt of Orion were marked.
Despite being much brighter than other constellations, Lepus did not acquire greater fame because it was overshadowed by being right next to Canis Major. This constellation contains Sirius, the brightest star in the sky, of which there are many stories and myths.
Nowadays
Currently, Lepus remains one of the official constellations and occupies an area of 290 square degrees in the night sky, which places it in 51st place in size among the 88 constellations that exist.
It is also known that deep-sky objects have been found significant for modern astronomy and the study of the universe within the constellation's boundaries.
How To Find The Lepus Constellation?
Visibility By Region
Lepus resides in the second quadrant of the Southern Hemisphere (SQ2) at latitudes between 63° N and 90° S, which means we can see the constellation in the night sky from every country in the world.
The constellation Lepus is visible in America, Europe, Asia, Australia, and Antarctica.
Lepus is not visible in areas above 63° N latitude, such as northern Canada, northern Greenland, Siberia, and the Arctic Circle.
Visibility By Season
Lepus is a constellation close to the celestial equator, so it is visible almost all year round for the southern hemisphere; however, the best month to visualize it is January.
Lepus is mostly visible during the winter in the northern hemisphere since it remains more timely in the sky during this season. In the northern hemisphere, it ceases to be visible in summer.
Finding Lepus Constellation
Lepus is essentially close to the celestial equator, so you will have to direct your gaze to the south in the northern hemisphere.
One way to locate the Lepus constellation is by finding its brightest star Arneb, which is in the central part of the constellation.
You can look for the constellation Orion to find Lepus since both constellations are very close.
The easiest way to locate the constellation Lepus is by drawing an imaginary straight line from the constellation of Orion to the constellation Columba; in the middle of the two, you will find the constellation Lepus.
Related Constellations
Lepus's constellations are Orion, Monoceros, Canis Major, Columba, Caelum, and Eridanus.
In addition, Lepus belongs to the Orion family of constellations, including Canis Major, Canis Minor, Monoceros, and Orion.
Stars in Lepus Constellation
The constellation Lepus officially contains 73 stars, of which 11 form the central figure of the constellation; these are Arneb, Nihal, Sasin, Neshmet, Theta Leporus, Zeta Leporus, Gamma Leporus, Eta Leporus, Delta Leporus, Lambda Leporus, and Kappa Leporus.
Arneb (α Leporis / α Lep / 11 Leporis)
With an apparent magnitude of +2.58, Arneb is the brightest star in the constellation Lepus. Arneb is a yellow supergiant about 1300 light-years from the Solar System.
It is one of the most intrinsically luminous stars that can be observed with the naked eye, its luminosity being equivalent to 13,000 suns. Its diameter is also huge, 75 times larger than the Sun. It has a surface temperature of 7000 K.
Nihal (β Leporis / β Lep / 9 Leporis / HD 36079)
Nihal is the second brightest star in the constellation Lepus, second only in brightness to Arneb (α Leporis). With an apparent magnitude of +2.81, it is located 159 light-years from the Solar System.
Nihal is a luminous yellow giant of spectral type G5II, whose surface temperature of 5209 K is somewhat lower than the Sun.
Epsilon Leporis (ε Lep / 2 Leporis / HD 32887 / HR 1654)
Also known as Sasin, it is the third most brilliant star in the constellation Lepus with an apparent magnitude of +3.19. It is located 213 light-years away from the Solar System.
It is a star of spectral type K4III, Epsilon Leporis, which has an effective temperature of 4131 K, and its radius is 40 times more grande than the radius of the sun.
Other Lepus Stars:
- δ Leporis is an orange subgiant star and coarse disk star of magnitude 3.81.
- ε Leporis is an orange giant star of magnitude 3.19, the third brightest star in Lepus.
- ζ Leporis: A white main-sequence star that appears to be surrounded by an asteroid belt.
- η Leporis: A yellow-white star of magnitude 3.72 surrounded by a circumstellar dust disk.
- ι Leporis: Double star whose components, a blue-white star and a yellow star, are separated by 17 arcseconds.
- λ Leporis: It is a blue subgiant star of magnitude 4.27.
- μ Leporis: A mercury-manganese star of magnitude 3.28, one of the brightest of its kind.
- 8 Leporis: It is a blue-white subgiant star of magnitude 5.22.
- 17 Leporis (SS Leporis): A nearby binary star—the two components are very close to each other—consisting of a white star and a red giant.
- R Leporis (Crimson Hind Star): Variable Mira twine whose brightness varies between magnitude 5.5 and 11.7. It is a carbon star of intense red color.
- S Leporis is a red and variable semi-irregular giant star whose brightness fluctuates between 6.0 and 7.6.
- T Leporis is a Mira variable star whose brightness ranges between magnitude 7.4 and 14.3.
- RX Leporis: It is a red giant star and irregular variable star.
- TX Leporis is a variable star Alpha2 Canum Venaticorum of magnitude 6.54.
- AC Leporis (HD 40745): A variable star Gamma Doradus of magnitude 6.21.
- AF Leporis (HD 35850): A variable star RS Canum Venaticorum of magnitude 6.31.
- AH Leporis (HD 36869): It is a yellow dwarf star and variable BY Draconis.
- HD 33283: It is a yellow dwarf star with an extrasolar planet.
- HD 38382: It is a yellow dwarf star distant 83 light-years.
- Gliese 229: A red dwarf star accompanied by a brown dwarf 18.8 light-years away.
Deep Sky Objects
Lepus is also known as home to several deep-sky objects. Deep-sky objects often mean star clusters, nebulae (interstellar cloud bodies), or galaxies.
In the case of Lepus, it has very few deep sky objects since it is a tiny constellation.
Messier 79 (M79 or NGC 1904)
M79 is the most notable deep sky object in the constellation Lepus, consisting of a globular cumulus with a magnitude of +8.56.
Pierre Méchain discovered it in 1780. M79 is at a distance of about 41,000 light-years from Earth and 60,000 light-years from the galactic center.
Other Notable Deep Sky Objects In Lepus:
- IC 418 is a planetary nebula of magnitude 11, whose central star has magnitude 11. Informally it is known as the "Spirograph Nebula." Its current diameter is 0.3 light-years.
- NGC 1964 is a barred spiral galaxy; it is the brightest galaxy in the constellation with 10.8.
Interesting Facts
- In some cultures of the southern hemisphere, such as the Aborigines of Australia, the constellation Lepus is represented with a kangaroo due to the abundance of these animals in the region.
- Lepus is not considered an independent constellation in other cultures such as China but is part of other more prominent constellations such as Orion or Canis Major.
Conclusions
- Lepus is a constellation located primarily in the southern hemisphere; the constellation's name comes from Latin and means Hare.
- Lepus is a small constellation, so very few myths are associated.
- The best month to see the Lepus constellation is in January, between the latitudes of 63° N and 90° S.
- The easiest way to locate the constellation Lepus is by drawing an imaginary straight line from the constellation of Orion to the constellation Columba; in the middle of the two, you will find the constellation Lepus.
- The brightest star in Lepus is Arneb (α Leporis / α Lep / 11 Leporis) which has an apparent magnitude of +2.58.
- The most notable deep-sky body of the constellation Lepus is Messier 79 (M79 or NGC 1904), a globular cluster of magnitude +8.56.