
Rafael Leão - Wikipedia
Rafael Alexandre da Conceição Leão (Portuguese pronunciation: [ʁɐfɐˈɛl ˈljɐ̃w]; born 10 June 1999) is a Portuguese professional footballer who plays as a left winger for Serie A club [ [AC Milan|]and the Portugal national team. He is known for his dribbling and speed. [2][3][4]
R Leonis - Wikipedia
R Leonis is a red giant Mira-type variable star located approximately 370 light years away in the constellation Leo. The apparent magnitude of R Leonis varies between 4.31 and 11.65 with a period of 312 days. At maximum it can be seen with the naked eye, while at minimum a telescope of at least 7 cm is needed.
Rafael Leão - Player profile 24/25 - Transfermarkt
Jun 10, 1999 · Rafael Leão, 25, from Portugal AC Milan, since 2019 Left Winger Market value: €75.00m * Jun 10, 1999 in Almada, Portugal
Rafael Leão: Stats and Biography - AC Milan
Birth Date:10 June 1999. Birth Place:Almada Setúbal. Nationality:Portugal. Height:188. Weight:81. Preferred Foot:Right. At AC Milan since:2019. Rafael Alexandre da Conceição Leão was born in Almada to Angolan parents on 10 June 1999. Rafa grew up in footballing terms at Sporting Lisbon and was soon making his debut both domestically and internationally. In October 2017, he was given his ...
R Leonis - aavso
R Leonis boldly boasts to be one the brightest and easiest to observe variable stars in the sky. With a mean visual magnitude range of 5.8 to 10.0, this mighty star can easily be seen without the aid of any costly equipment.
Take a Look at R Leonis, Leo's Giant Ticker - Sky & Telescope
Jan 29, 2025 · Like the prototype Mira, R Leo is a long-period variable star, a relatively cool, pulsating red giant star in the final stages of life. These bloated behemoths begin their lives with masses similar to the Sun's.
Variable Star R Leonis - theskyscrapers.org
The magnitude range and period attributed to R Leonis are typical of a class of variable stars known as Mira-type, or Long-Period Variables (LPVs). Like its kindred LPVs, R Leonis is a cool red giant – a dying star whose brightness changes result from internal pulsations.
Rho Leonis - Wikipedia
Rho Leonis (ρ Leo), also named Shaomin, [9] is a binary star in the zodiac constellation of Leo, and, like the prominent nearby star Regulus, is near the ecliptic. With an apparent visual magnitude of 3.9, [4] this star can be readily seen with the naked eye.
R Leonis - University of Illinois Urbana-Champaign
R Leo is a deep class M (M8) giant, whose class also varies, between M7 and M9, giving it a lovely color described by Burnham as "rosy scarlet with often a seeming touch of purple." Three thousand days in the variation of R Leonis are plotted as visual magnitudes versus the running count of Julian Day number , which begins January 1, 4713 BCE.
The variable star R Leonis - ASSA
Like its kindred LPVs, R Leonis is a cool red giant – a dying star whose brightness changes result from internal pulsations. Based on recent observations, R Leonis has a magnitude of about 10 and is declining to a predicted minimum later this month ( April 2014).