AF LEPORIS

AF LEPORIS

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Orion (constellation) thumbnail

Orion (constellation)

Orion is a prominent set of stars visible during winter in the northern celestial hemisphere. It is one of the 88 modern constellations; it was among the 48 constellations listed by the 2nd-century astronomer Ptolemy. It is named after a hunter in Greek mythology. Orion is most prominent during winter evenings in the Northern Hemisphere, as are five other constellations that have stars in the Winter Hexagon asterism. Orion's two brightest stars, Rigel (β) and Betelgeuse (α), are both among the brightest stars in the night sky; both are supergiants and slightly variable. There are a further six stars brighter than magnitude 3.0, including three making the short straight line of the Orion's Belt asterism. Orion also hosts the radiant of the annual Orionids, the strongest meteor shower associated with Halley's Comet, and the Orion Nebula, one of the brightest nebulae in the sky.

In connection with: Orion (constellation)

Orion

constellation

Title combos: constellation Orion

Description combos: 2nd six are brightest making the radiant with in

List of stars in Lepus

This is the list of notable stars in the constellation Lepus, sorted by decreasing brightness.

In connection with: List of stars in Lepus

List

of

stars

in

Lepus

Title combos: in stars List of stars List of Lepus stars

Description combos: This constellation sorted list in the in brightness list

List of directly imaged exoplanets thumbnail

List of directly imaged exoplanets

This is a list of extrasolar planets that have been directly observed, sorted by observed separations. This method works best for young planets that emit infrared light and are far from the glare of the star. Currently, this list includes both directly imaged planets and imaged planetary-mass companions (objects that orbit a star but formed through a binary-star-formation process, not a planet-formation process). This list does not include free-floating planetary-mass objects in star-forming regions or young associations, which are also referred to as rogue planets. The data given for each planet is taken from the latest published paper on the planet to have that data. In many cases it is not possible to have an exact value, and an estimated range is instead provided. The coldest and oldest planet directly imaged is Epsilon Indi Ab, which has six times Jupiter's mass, an effective temperature of 275 K, and an age of about 3.5 Ga. This list includes the four members of the multi-planet system that orbit HR 8799. It is unlikely or at least unclear if objects on a wide orbit (≥100 AU) formed in circumstellar disks and these objects are therefore more often referred as planetary-mass companions. Only in rare cases, such as for HD 106906 b, the formation of the object in the disk is seen plausible.

In connection with: List of directly imaged exoplanets

List

of

directly

imaged

exoplanets

Title combos: of imaged List of exoplanets imaged of exoplanets directly

Description combos: list data unlikely list planets four for formation possible

Iota Leporis thumbnail

Iota Leporis

Iota Leporis (ι Leporis) is a triple star system in the southern constellation of Lepus. It is visible to the naked eye as a point source of blue-white light with an apparent visual magnitude of 4.45. Based upon an annual parallax shift of 14.07 mas as measured from Earth, the system is located roughly 232 light years from the Sun. The primary, designated component A, is a B-type main-sequence star with a stellar classification of B7.5 Vn, where the 'n' suffix indicates "nebulous" absorption lines caused by rotation. It is about 94 million years old and has a high rate of spin with a projected rotational velocity of 185 km/s. With an estimated 3.4 times the mass of the Sun, it is radiating 153 times the Sun's luminosity from its photosphere at an effective temperature of around 13,781 K. There is a close companion that is a source of X-ray emission. Most likely this star has at least 1.05 times the mass of the Sun. The third component, AM Leporis, is a BY Draconis variable of apparent magnitude 9.92, and spectral type G8Ve at an angular separation of 12.7".

In connection with: Iota Leporis

Iota

Leporis

Title combos: Iota Leporis

Description combos: Leporis close old is source companion that this at

List of exoplanets discovered in 2023

This list of exoplanets discovered in 2023 is a list of confirmed exoplanets that were first reported in 2023. For exoplanets detected only by radial velocity, the listed value for mass is a lower limit. See Minimum mass for more information.

In connection with: List of exoplanets discovered in 2023

List

of

exoplanets

discovered

in

2023

Title combos: in 2023 2023 List of of List 2023 in

Description combos: is of mass were listed See confirmed were by

AF Leporis thumbnail

AF Leporis

AF Leporis, also known as HD 35850, is a young variable star located 87.5 light-years (26.8 parsecs) away from the Solar System in the constellation of Lepus. With an apparent magnitude of 6.3, it is near the limit of naked eye visibility under ideal conditions. AF Leporis is a member of the Beta Pictoris moving group, with an astronomically young age of about 24 million years. It hosts a circumstellar disk and one known exoplanet.

In connection with: AF Leporis

AF

Leporis

Title combos: AF Leporis

Description combos: AF of away also Solar one 35850 and constellation

List of star systems within 85–90 light-years

This is a list of star systems within 85–90 light years of Earth. The closest M-type red giant star, Gacrux, is in this list. Most data from this list come from the SIMBAD database.

In connection with: List of star systems within 85–90 light-years

List

of

star

systems

within

85

90

light

years

Title combos: light star light star of light within systems List

Description combos: 85 This of years 85 within 90 this closest

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