#794201830496
Belongs to Gemini Dreams's Pride
(View Former Prides)

Quasar | Rough Ruby|Special

"Plummage"

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This lioness gave birth in the past two years. She is on a breeding cool down and will be breedable again in 2 real life days.

Lion Stats
Experience	0 / 100 (0%)
Level	1
Strength	55	Speed	37
Stamina	64	Smarts	67
Agility	47	Skill	1
Total Stats:		271

Lion Currents
Age	6 years, 3 months old
Hunger	12%
Mood	100%
Sex	Female
Pose	Kind
Personality	Sassy (Snarky)

Adult Stage

Breeding Info
Father	Sgaeyl	Mother	Mercy	View Full Heritage
Last Bred	21 days ago	Fertility	Low	View All Cubs Bred (0)

Appearance		Markings
Base	Rough Ruby (White Skin)	Slot 5: Feline 9 Elysian (62%) Tier 5 Slot 7: Interstellar Smoke (89%) Tier 3 Slot 8: Feline 6 Elysian (64%) Tier 5 Slot 9: White Freckles 1 (78%) Tier 3 This lion has 1 marking hidden on the following slot: 11
Genetics	Red Dark Countershaded Special
Eyes	Pink
Mane Type	Diabolic
Mane Color	Aufeis
Mutation	Patches (Plumage)
Marking Slots	10

Equipped Decorations Hide/Show
Conjunction Above Draconid Horns [Black] Draco Whiskers [Black] Dragon Leg Morph [Onyx] Dragon Tail Morph [Onyx] Star Cluster - High Small Dragon [Chiral] Meteor Shards Necklace Draconic Eyes [Red] Below Star Halo

Lifetime Hunting Results
Total Hunts	0	Successful Hunts	0	Success Rate	0%

Biography
A quasar is an extremely luminous active galactic nucleus (AGN). It is pronounced /ˈkweɪzɑːr/ KWAY-zar, and sometimes known as a quasi-stellar object, abbreviated QSO. This emission from a galaxy nucleus is powered by a supermassive black hole with a mass ranging from millions to tens of billions of solar masses, surrounded by a gaseous accretion disc. Gas in the disc falling towards the black hole heats up because of friction and releases energy in the form of electromagnetic radiation.

Biography

A quasar is an extremely luminous active galactic nucleus (AGN). It is pronounced /ˈkweɪzɑːr/ KWAY-zar, and sometimes known as a quasi-stellar object, abbreviated QSO. This emission from a galaxy nucleus is powered by a supermassive black hole with a mass ranging from millions to tens of billions of solar masses, surrounded by a gaseous accretion disc. Gas in the disc falling towards the black hole heats up because of friction and releases energy in the form of electromagnetic radiation.

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